Fourier Transform Spectroscopy (FTS) and Hyperspectral Imaging … · 2015. 2. 12. · Hot Tub:...

FTS/HISE • 1-4 March 2015 1

Fourier Transform Spectroscopy (FTS)

and

Hyperspectral Imaging and Sounding of the

Environment (HISE) Meetings Program 1-4 March 2015

UCLA Conference Center,

Lake Arrowhead, California, USA

Table of Contents

Chairs’ Welcome Letter ………………………………………………………… 2

Program Committee …………………………………………………………….. 3

General Information.……………………………………………………………...4

Stay Connected…………………………………………………………………...5

Special Events…….……………………………………………………………….5

Plenary Speakers....……………………………………………………………….6

Explanation of Session Codes …………………………………………………. 7

Agenda of Sessions…………….……………...………………...……….……… 8

Abstracts...……………………………………...…………...……...……………. 10

Key to Authors…............................…………...……………...………...…....... 28

Technical Digest Access…….…….…….…….…….…….…….…….……Inside Back Cover

2 FTS/HISE • 1-4 March 2015

Fourier Transform Spectroscopy (FTS) Meeting

Hyperspectral Imaging and Sounding of the Environment (HISE) Meeting

1-4 March 2015

Lake Arrowhead, California, USA

Welcome to beautiful Lake Arrowhead, California! This year the Fourier Transform Spectroscopy (FTS) Meeting and Hyperspectral

Imaging and Sounding of the Environment (HISE) Meeting have collocated in order to provide participants with the opportunity to

engage in discussions and critical knowledge-sharing with individuals from around the world in a multitude of fields.

The Fourier Transform Spectroscopy (FTS) Meeting provides a unique opportunity for scientists and engineers to share

advances in instrumentation, calibration, and algorithms, and to present applications to important problems in astrophys-

ics, atmospheric science, and laboratory spectroscopy. During this topical meeting, scientists and engineers will be pre-

sented with an important opportunity to showcase and discuss recent developments in instrument design and capabilities,

calibration and data processing algorithms, results from current applications, and development of novel applications. This

year’s meeting will feature two plenary talks, 15 invited speakers, and over 35 oral and poster contributed presentations.

The Hyperspectral Imaging and Sounding of the Environment (HISE) Meeting provides unprecedented opportunities to

monitor and understand our planetary system. Topics during the meeting will include atmospheric measurements, model-

ing and compensation methods; advanced detection, image segmentation, pattern recognition, and visualization algo-

rithms; new spectrometer designs, flight packing and sensor characterization, planned and deployed operation systems;

retrieval and inversion of hyperspectral measurements; active methods of multimodal fusion techniques; innovative uses

of hyperspectral measurements in earth and planetary sciences for both industrial and private sectors, and many more.

The HISE meeting will host a plenary talks, 14 invited speakers and 27 oral and poster contributed presentations.

We hope you enjoy all the meetings, and take full advantage of the scientific sessions and networking opportunities be-

fore you.

Sincerely,

David Johnson,

NASA Langley Research Center, USA

FTS Chair

Xianglei Huang

University of Michigan, USA, HISE Chair

Juliet Pickering

Imperial College London, UK FTS Chair

Alan Schaum

US Naval Research Laboratory, USA

HISE Chair


Fourier Transform Spectroscopy

(FTS)

Chairs David Johnson, NASA Langley Research Center, United States Juliet Pickering, Imperial College London, United Kingdom

Program Committee Members Peter Bernath, Old Dominion University, United States Christoph Englert, US Naval Research Laboratory, United States Adam Fleisher, National Inst of Standards & Technology, United States Felix Friedl-Vallon, Karlsruher Institut fuer Technologie, Germany Jerome Genest, Universite Laval, Canada John Mark Harlander, St Cloud State University, United States Donald E. Jennings, NASA Goddard Space Flight Center, United States Erik Kretschmer, Karlsruher Institut für Technologie, Germany Akihiko Kuze, Japan Aerospace Exploration Agency, Japan David Naylor, University of Lethbridge, Canada Luca Palchetti, Istituto Nazionale di Ottica (CNR), Italy Nathalie Picque, Max-Planck-Institut fur Quantenoptik, Germany Locke Spencer, University of Lethbridge, Canada Joe Taylor, University of Wisconsin-Madison, United States Geoffrey Toon, Jet Propulsion Laboratory, United States Kaley Walker, University of Toronto, Canada

Hyperspectral Imaging and Sound-ing of the Environment (HISE) Chairs Xianglei Huang, University of Michigan, United States Alan Schaum, US Naval Research Laboratory, United States

Program Committee Members Amit Banerjee, Johns Hopkins University, United States

Jocelyn Chanussot, Grenoble Inst. of Technology, France

David Gillis, US Naval Research Laboratory, United States

Brian Kahn, Jet Propulsion Laboratory, United States

John Kerekes, Rochester Institute of Technology,

United States

Fred Kruse, Naval Postgraduate School, United States

John Lee, US Naval Research Laboratory, United States

Martin Mlynczak, NASA Langley Research Ctr,

United States

Peter Pilewskie, University of Colorado at Boulder,

United States

Stanley Rotman, Ben Gurion University of the Negev,

Israel

Alan Stocker, West Coast Analytics, United States

L. Larrabee Strow, University of Maryland Baltimore

County, United States

James Theiler, Los Alamos National Laboratory,

United States

David Tobin, University of Wisconsin-Madison,

United States

Jun Wang, University of Nebraska Lincoln, United States

Michael Yetzbacher, Naval Research Laboratory,

United States

COMMITTEE


Sunday, 1 March 15:00—18:00

Monday, 2 March 08:00—16:30

Tuesday, 3 March 08:00—17:30

Wednesday, 4 March 08:00—17:30

Registration Hours Living Room

Meal Hours Dining Room Due to the remote location of the UCLA Conference Center at Lake Arrowhead California, accommodations and meals are included in the registration fees. Meals will be available during pre-determined hours. Below please find the meal hours for each day during the conference. Dinner will be available on check-in day (Sunday) and breakfast and lunch will be available on check-out day (Thursday).

Social Room

A Social Room is available for attendees during the

conference days to network and relax. Below are times

and locations.

UCLA Lake Arrowhead Conference

Center Information

Main Lodge: The Main Lodge is open daily from 06:00—23:59. The Front Desk is staffed daily from 07:00—23:59. The Conference Center is staffed 24-hours a day. Please dial “0” for assistance.

Food and Snacks: Complimentary coffee and tea service as well as complimentary whole fruit is available daily in the lobby. Vending machines are available outside the Tavern. Ice machines are located in the Laundry Room.

Laundry Services: Laundry machines are located across from the Iris Meeting Room.

Business Center: Business Center services are located at the Front Desk in the Main Lodge. Services include copying, printing, faxing, scanning, and complimentary laptop usage. Receiving of packages for meetings at no additional charge. Wifi is available free of charge throughout the UCLA Lake Arrowhead Conference Center Campus

Recreation Facilities

Fitness Center: Enjoy the state-of-the-art fitness center with 24/7 access with your room key.

Hiking Trails: There are a number of hiking trails

heading out from the UCLA Lake Arrowhead Conference

Center. Explore the area and enjoy beautiful lake and

forest views. Request a copy of our Trails to Enjoy guide

at the front desk for step-by-step directions around the

mountain or the lake.

Hot Tub: Relax in the indoor hot tub, located fireside adjacent to the swimming pool.

Recreational Sports: Enjoy a variety of sporting activities including basketball, bocce ball, golf, horseshoes, sand volleyball, shuffleboard, tennis, football, soccer, and Frisbee. Equipment is available for check out at the Front Desk in the Main Lodge. Board games are also available in the Main Lodge Living Room.

Zen Deck: For the best view of the lake, visit the Zen Deck, located at the upper edge of the property.

GENERAL INFORMATION

Breakfast Lunch Dinner

Sunday, 1

March 18:30—20:00

Monday, 2

March 07:45—09:00 12:00—13:00 18:30—20:00

Tuesday, 3

March 07:00—08:00 12:00—13:00 18:30—20:00

Wednesday,

4 March 07:45—08:00 12:00—13:00 18:30—20:00

Thursday, 5

March 07:45—08:00 12:00—13:00

Location Date and Time

Tavern Sunday, 1 March, 16:00 – 23:59

Lakeview Monday, 2 March, 20:00 – 23:59

Lakeview Tuesday, 3 March, 17:30 – 23:59

Lakeview Wednesday, 4 March, 16:30 – 23:59


Wi-Fi Connection The Lake Arrowhead Conference Center offers complimentary wireless access throughout the property. Access to the internet is not password protected.

Early Online Access to the Technical Digest and Postdeadline Papers Full Technical Attendees have both EARLY and FREE continuous access to the digest papers through Optics InfoBase. To access the papers go to www.osa.org/FTS_HISE and select the “Access digest papers” essential link on the right hand navigation. As access is limited to Full Technical Meeting Attendees only, you will be asked to validate your credentials by entering the same login email address and password provided during the Meeting registration process. If you need assistance with your login information, please use the “forgot password” utility or “Contact Help” link.

Poster Presentation PDFs The PDFs of select poster presentations will be available two weeks after the conference. While accessing the papers in Optics Infobase look for the multimedia symbol.

Update Sheet All technical program changes will be communicated in the onsite Conference Program Update Sheet. All attendees receive this information with registration materials, and we encourage you to review it carefully to stay informed to changes in the program.

Joint Poster Session Monday, 2 March, 13:00—14:30, Lakeview Room

Poster presentations offer an effective way to

communicate new research findings and provide a

venue for lively and detailed discussion between

presenters and interested viewers. Don’t miss this

opportunity to discuss current research one-on-one with

the presenters. Setup and tear-down times are listed

below.

Conference Reception Monday, 2 March, 17:30—18:30, Lakeview Room

Join your fellow attendees for the conference reception.

Enjoy delectable fare while networking. The reception is

open to committee/presenting author/student and full

Conference attendees. Meeting attendees may

purchase extra tickets for their guest.

Joint Plenary Session Tuesday, 3 March, 09:00—10:30, Pineview Room

This year’s FTS/HISE meetings will feature two joint

Plenary speakers: Henry Revercomb, Univ. of Wisconsin-

Madison, USA and James Theiler, Los Alamos National

Laboratory, USA. For more information on the plenary

presentations, see the Plenary descriptions on page 6 of

this program.

FTS Plenary Tuesday, 3 March, 13:00—13:45, Pineview Room

In addition to the two joint conference Plenary speakers,

FTS will feature an additional plenary presentation by

Jean-Pierre Maillard, Institut d’Astrophysique de Paris,

France. For more information on the plenary

presentations, see the Plenary descriptions on page 6 of

this program.

STAY CONNECTED SPECIAL EVENTS

Poster Session

Date / Time SETUP TEARDOWN

JM3A Monday, 2 March,

13:00 – 14:30

Monday, 2 March,

9:00 – 12:30

End of session at 14:30, no later than

16:30

Laser Applications to Chemical,

Security and Environmental

Analysis (LACSEA)

October 2016, Boston Area

Check www.osa.org regularly for more

information.


Henry E. Revercomb, University of Wisconsin-Madison, USA

Advancing Climate Benchmark Measurements Tuesday, 3 March, 09:00—09:45 Dr. Henry E. Revercomb (Hank), director

of the Space Science and Engineering Center (SSEC), University of Wisconsin-Madison, has been engaged in using radiation measurements to study the atmospherics of the earth and other planets. Specialties include, high spectral resolution instrumentation for atmospheric remote sensing and spectroscopy, operational temperature and water vapor sounders, climate observing systems, and net radiative flux observations of Venus and Jupiter.

James Theiler, Los Alamos National

Laboratory, USA

Anomalousness: How to Measure What

You Can't Define

Tuesday, 3 March, 09:45—10:30

James Theiler received a Ph.D. in physics from Caltech in 1987, and subsequently held appointments at UCSD, MIT Lincoln Laboratory, Los Alamos National Laboratory, and the Santa Fe Institute. He joined the technical staff at Los Alamos in 1994, and was named a Laboratory Fellow in 2005. His professional interests include statistical modeling, machine learning, image processing, and remote sensing.

Jean-Pierre Maillard, Institut

d’Astrophysique de Paris, France

From 1D-Fourier Transform

Spectroscopy to Imaging Fourier

Transform Spectroscopy in Astronomy

Tuesday, 3 March, 13:00—13:45

Jean-Pierre Maillard is currently director of research emeritus at Institut d’Astrophysique de Paris. He started his scientific career by his PhD thesis devoted to the application in astronomy of FT spectroscopy, which was just at the beginning, in Professor Jacquinot’s lab under Pierre Connes supervision. Few years later, he was in charge of building a high-resolution infrared FTS for the 3.6-m Canada-France-Hawaii Telescope. With this instrument, in operation for almost twenty years, he obtained important results on the solar system planetary atmospheres, the atmosphere of evolved stars, on star forming molecular clouds. By coupling the CFHT-FTS to an infrared camera he built the first astronomical Imaging FTS to study the environment of the Galactic Center black hole, the envelope of planetary nebulae. He has been actively participating to several IFTS proposals, for space and ground-based telescopes, the last one being a wide-field IFTS for CFHT, ready to start observing.

JOINT PLENARY SPEAKERS FTS PLENARY SPEAKER

http://www.google.com/url?sa=i&rct=j&q=&esrc=s&frm=1&source=images&cd=&cad=rja&docid=4kGj_7x3fTWB_M&tbnid=ZisIP7ZCV5OOxM:&ved=0CAUQjRw&url=http%3A%2F%2Flearnjapanesepod.com%2Fjapanese-etiquette-2%2F&ei=uT_yUvaDOIG3kQeh6oCwAQ&bvm=bv.60799247,d.eW0&psig=AF


EXPLANATION OF SESSION CODES

Meeting Name Number

Day of the Week Series Session Designation The first letter of the code designates the meeting (FTS=F, HISE=H, Joint=J). The second element denotes the day of the week (Monday=M, Tuesday=T, Wednesday = W). The third element indicates the session series in that day (for instance, 1 would denote the first sessions in that day). Each day begins with the letter A in the fourth element and continues alphabetically through the parallel session. The lettering then restarts with each new series. The number on the end of the code (separated from the session code with a period) signals the position of the talk within the session (first, second, third, etc.). For example, a presentation coded FT2A.4 indi-cates that this paper is being presented as part of the FTS meeting on Tuesday (T) in the second series of ses-sions (2), and is the first parallel session (A) in that series and the fourth paper (4) presented in that session.

FT2A.4

Example

Online Access to Technical Digest Now Available!

Full Technical Attendees have both EARLY and FREE perpetual access to the digest papers through Optics In-

foBase. To access the papers go to www.osa.org/FTS_HISE and select the “Access digest

papers” essential link on the right hand navigation. As access is limited to Full Technical Conference Attendees

only, you will be asked to validate your credentials by entering the same login email address and password

provided during the Conference registration process. If you need assistance with your login information,

please use the “forgot password” utility or “Contact Help” link.

1=1st of series 2=2nd of series 3=3rd of series 4=4th of series

5=5th of series

A=1st Parallel Session

B=2nd Parallel Session

F=FTS H=HISE

J=Joint

Presentation order

within session

M=Monday T=Tuesday W= Wednesday


AGENDA OF SESSIONS

Sunday, 1 March

15:00 - 18:00 Registration, Living Room

18:30 - 20:00 Dinner, Dining Room

Monday, 2 March

Pineview Room Iris Conference Room

FTS HISE

07:45 - 09:00 Breakfast, Dining Room


09:00 - 10:30 JM1A ● New Results from FTS Sounders, Pineview Room

10:30 - 11:00 Coffee Break

11:00 - 12:00 FM2A • Comb I HM2B • New Spectrometer Design and Sensor

Characterization

12:00 - 13:00 Lunch, Dining Room

13:00 - 14:30 JM3A ● Joint Poster Session, Lakeview Room

14:30 - 15:00 Beverage Break

15:00 - 17:00 FM4A ● New Instruments/SIFTS HM4B ● New Spectrometer Design and Sensor

Characterization II

17:30 - 18:30 Welcome Reception, Lakeview Room


The Pineview Room (FTS and joint sessions) is located in the Main Lodge Building. The Iris Conference Room is located

in a separate building directly across the parking lot from the Main Lodge. All other locations are in the Main Lodge

Building. Coffee and Beverage breaks will be located within or nearby the presentation rooms. Please see the map on

the inside cover of the program for more details.


AGENDA OF SESSIONS

Tuesday, 3 March


FTS HISE

07:00- 08:00 Breakfast, Dining Room


09:00 - 10:30 JT1A • Joint Plenary Session, Pineview Room


11:00 - 12:00 FT2A • Comb II/Dispersed Interferometry HT2B • Retrieval and Inversion of Hyperspectral

Measurements I


13:00 - 15:00 FT3A ● Astronomy, Planetary, Imaging FTS HT3B ● Retrieval and Inversion of Hyperspectral

Measurements II (ends at 14:45)


15:30 - 17:30 FT4A ● Imaging FTS in Astronomy HT4B ● Atmospheric Measurements, Modeling

and Compensation


Wednesday, 4 March

Pineview Room Iris Conference Center

FTS HISE

07:45 - 09:00 Breakfast, Dining Room


09:00 - 10:30 FW1A ● Calibration and Validation (ends at

10:15) HW1B ● Planned and Deployed

Operational Systems


11:00 - 12:00 FW2A ● Lab Measurements HW2B ● Advanced Detection, Image Segmenta-

tion and Pattern Recognition


13:00 - 15:00 FW3A ● Earth Atmosphere Algorithms

and Instruments HW3B ● Multimodal Fusion and

Visualization Algorithms (ends at 14:30)


15:30 - 17:15 FW4A • Earth Atmosphere Instruments



Pineview Room

Joint FTS/HISE

09:00 -- 10:30 JM1A • New Results from FTS Sounders Presiders: Joe Taylor; Space Science and Engineering Center, Univ. of Wisconsin-Madison, USA and Xianglei Huang; Univ. of Michigan, USA

JM1A.1 • 09:00 Future JPSS Cross-track Infrared Sounder (CrIS) Ground Calibration Algorithm Improvements, Joe Predina1, Yong Han2, Dan Mooney3, Shankar Atre1, Lawrence Suwinski4; 1Logistikos Engineering LLC, USA; 2NOAA, USA; 3MIT Lincoln Lab, USA; 4Exelis Inc., USA. Future CrIS atmospheric sounder calibration algorithms will further reduce radiometric measurement uncertainty by improved ground calibration methods that better model and compensate for spectral ringing present in the unapodized Instrument Line Shape (ILS).

JM1A.2 • 09:30 A New Marine Atmospheric Emitted Radiance Interferometer for Shipboard Atmospheric and Oceanic Observations, Jonathan Gero1, Robert Knuteson1, Denny Hackel1, Fred Best1, Raymond Garcia1, Coda Phillips1, Henry E. Revercomb1, William L. Smith1, Eric Verret2, Stephane Lantagne2, Claude Roy2; 1Univ. of Wisconsin, USA; 2ABB Inc., Canada. The Marine-Atmospheric Emitted Radiance Interferometer (M-AERI) is a robust, accurate seagoing instrument that measures thermal emission spectra from the sea surface and marine atmosphere. Results from the first shipboard deployment of a new M-AERI instrument are presented.

JM1A.3 • 09:45 The Three-dimensional Reconstruction of Temperature and Trace Gas Distributions from Measurements of the Airborne Limb-imager GLORIA, Jörn Ungermann1; 1Forschungszentrum Julich GmbH, Germany. This paper describes the tomographic processing of dynamics mode measurements of the airborne Fourier-transform spectrometer GLORIA. First trace gas results are presented including validation against in situ measurements.

JM1A.4 • 10:15 Atmospheric Chemistry Experiment, ACE: Recent Results, Peter F. Bernath1; 1Old Dominion Univ., USA. ACE is a satellite mission that is measuring the concentrations of more than thirty atmospheric constituents by absorption spectroscopy using the sun as a light source. A selected overview of some recent ACE results in the last 2 years will be presented.

07:45—09:00 • Breakfast, Dining Room

08:00—16:30 • Registration, Living Room

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FTS HISE

11:00 -- 12:00 FM2A • Comb I Presider: Nathalie Picque; Max Planck Institute of Quantum Optics, Germany

11:00 -- 12:00 HM2B • New Spectrometer Design and Sensor Characterization I Presider: Michael Yetzbacher; Naval Research Laboratory, USA

FM2A.1 • 11:00 Dual Comb Spectroscopy - Static Fourier Transform Spectroscopy with Frequency Combs, Birgitta C. Bernhardt1,3, Takuro Ideguchi1, Simon Holzner1,3, Guy Guelachvili2; 1Max-Planck-Institut fuer Quantenoptik, Germany; 2Institut des Sciences Moléculaires d'Orsay, CNRS, France; 3Ludwig-Maximilians-Universität München, Germany. Dual frequency comb spectroscopy relying on two pulsed laser oscillators rather than a scanning Michelson interferometer can outperform traditional FTS in sensitivity, spectral resolution and acquisition time. Several experiments are presented that highlight this potential.

HM2B.1 • 11:00 MX-20SW Short Wave Infrared Stabilized Hyperspectral Imager for Oblique Viewing Geometries, Jonathan G. Neumann1, Eric C. Allman1, Grant J. Howard1; 1US Naval Research Laboratory, USA. This presentation will discuss MX-20SW short wave infrared stabilized hyperspectral imager for oblique viewing geometries.

FM2A.2 • 11:30 Development of a Transportable Dual-comb Spectrometer for Remote Sensing of Greenhouse Gases Over Kilometer-scale Air Paths, Jean-Daniel Deschênes1, Gar-Wing Truong1, Laura Sinclair1, Gregory Rieker1, Fabrizio Giorgetta1, William Swann1, Esther Baumann1, Ian Coddington1, Nathan Newbury1; 1National Inst of Standards & Technology, Canada. We report on the recent work at NIST to develop new frequency comb sources to perform spectroscopy of carbon dioxide, methane and oxygen in the atmosphere over 1 to 4 kilometer free-space paths.

HM2B.2 • 11:30 Hyperspectral Radiometric Accuracy Improvements, Greg Kopp1, Chris Belting1, Zach Castleman1, Ginger Drake1, Joey Espejo1, Karl Heuerman1, Bret Lamprecht1, Peter Pilewskie1, Paul Smith1; 1Laboratory for Atmospheric and Space Physics, Univ. of Colorado at Boulder, USA. Using on-orbit solar cross calibrations, the HyperSpectral Imager for Climate Science improves radiometric accuracy of measured Earth scenes to <0.5%, helping establish benchmark measurements for space-borne climate studies in the 350-2300 nm spectral range.

08:50—10:30 • BS1A Opening Remarks and Plenary Session I, Symphony III & IV

12:00—13:00 • Lunch, Dining Room



foBase. To access the papers go to www.osa.org/FTS_HISE and select the “Access digest papers”

essential link on the right hand navigation. As access is limited to Full Technical Congress Attendees only, you

will be asked to validate your credentials by entering the same login email address and password provided

during the congress registration process. If you need assistance with your login information, please use the

“forgot password” utility or “Contact Help” link.

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13:00 -- 14:30 JM3A • Joint Poster Session, Lakeview Room

JM3A.1 High Resolution FTS Studies of the Effects of Trace Molecular Gases on Glow Discharge Spectra and Industrial Applications, Juliet C. Pickering1, Sohail Mushtaq2, Edward Steers2, Zdenek Weiss3; 1Imperial College London, UK; 2London Metropolitan Univ., UK; 3LECO Instrumente, Czech Republic. Analytical Glow Discharge (GD) Optical Emission Spectroscopy and GD Mass Spectrometry have important industrial applications. The analytical accuracy may be affected by trace molecular gases. High resolution FTS is used to investigate fundamental discharge processes.

JM3A.2 S-HIS Dual Regression Retrieval Analysis Relating to the HS3 Field Campaign, Daniel DeSlover1, Henry Revercomb1, Joe Taylor1, Fred Best1, David Tobin1, William L. Smith1, Elisabeth Weisz1; 1UW-Madison / SSEC, USA. Atmospheric state retr ievals f rom S-HIS measurements from NASA's Global Hawk during the HS3 aircraft field campaign during the 2012 through 2014 hurricane seasons. Results will be compared to colocated AVAPS d ropsonde and CP L l ida r measurements--flown alongside S-HIS on the Globalhawk. JM3A.3 Demonstrating Spectro-Spatial Interferometry in the Thermal Infrared: Recent progress, Roser Juanola-Parramon1, Giorgio Savini1; 1Univ. College London, UK. The recent developments of the Thermal Spectro-Spatial Interferometric Testbed (SSIT), a Double Fourier Modulation (DFM) interferometer operating in the thermal infrared wavelength range are presented. The optical design is described and the technical challenges discussed.

JM3A.4 Herschel SPIRE FTS data processing of partially extended sources, Edward Polehampton1,2, Rosalind Hopwood4, Ivan Valtchanov5, Nanyao Lu6, Nicola Marchili7, Trevor Fulton2, Jeremy Zaretski8, Ronin Wu9, Gibion Makiwa2, Bruce Swinyard1, Matthijs H. van der Wiel3, Locke D. Spencer2, David A. Naylor2; 1Rutherford Appleton Laboratory, UK; 2Inst. for Space Imaging Science, Canada; 3Niels Bohr Inst., Denmark; 4Imperial College London, UK; 5Herschel Science Centre, Spain; 6NASA Herschel Science Centre, USA; 7Dipartimento di Fisica e Astronomia, Italy; 8Blue Sky Spectroscopy, Canada; 9Univ. of Tokyo, Japan. The Herschel SPIRE imaging FTS pipeline processing assumed either point-like or uniformly extended emission. This paper describes the interactive processing required to correct partially extended sources to account for the changing beam size with frequency.

JM3A.5 FTS-2 Commissioning Update, Brad Gom1, David A. Naylor1, Per Friberg2, Graham Bell2, Daniel Bintley2; 1Univ. of Lethbridge, Canada; 2Joint Astronomy Centre, USA. We present an update on the ongoing commissioning of FTS-2, the imaging Fourier transform spectrometer ancillary instrument for use with the SCUBA-2 camera at the James Clerk Maxwell Telescope.

JM3A.6 A Cryogenic FTS Translation Mechanism: Test-Bed Design and Anticipated Challenges, Ian Veenendaal1, David A. Naylor1, Brad Gom1; 1Univ. of Lethbridge, Canada. Cryogenic optical equipment will become a standard requirement for future far infrared observatories. Here we outline the design of a cryogenic test bed for optical metrology and discuss its role in regards to component testing of future space-borne instruments.

JM3A.7 The Herschel/SPIRE Spectrometer Phase Correction Data Processing Tasks, Trevor Fulton1, David A. Naylor1, Edward Polehampton2,1, Rosalind Hopwood3, Ivan Valtchanov4, Nanyao Lu5, Nicola Marchili6, Jeremy Zaretski7; 1Univ. of Lethbridge, Canada; 2RAL Space, Rutherford Appleton Laboratory, UK; 3Imperial College London, UK; 4ESAC, Spain; 5NHSC/IPAC, USA; 6Universitá di Padova, Italy; 7Blue Sky Spectroscopy, Canada. Asymmetries in the recorded interferograms of Fourier Transform Spectrometers (FTS) result in spectra with a non-zero phase. We describe the causes of non-zero phase particular to the Herschel/SPIRE FTS and present the phase correction processing steps employed.

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13:00 -- 14:30 JM3A • Joint Poster Session, Lakeview Room

JM3A.8 Frequency Scale Calibration of the Herschel/SPIRE Imaging Fourier Transform Spectrometer, Locke D. Spencer1, David A. Naylor1, Gibion Makiwa1, Trevor Fulton1, Edward Polehampton2,1, Ivan Valtchanov3, Rosalind Hopwood4, Matthijs van der Wiel5, Jeremy Scott1, Courteney Hamilton1, Adam Lefaivre1; 1Physics and Astronomy, Univ. of Lethbridge, Canada; 2RAL Space, Rutherford Appleton Laboratory, UK; 3Herschel Science Centre, ESA, Spain; 4Imperial College London, UK; 5Niels Bohr Inst., Denmark. The Herschel Spectral and Photometric Imaging Receiver (SPIRE) employs a dual-band imaging Fourier-transform-spectrometer (IFTS). We discuss the frequency calibration of both on- and off-axis SPIRE IFTS detectors using CO emission lines from observations of Orion.

JM3A.9 FIInS - A Python Simulator for a Far-infrared Double Fourier Interferometer in Space, John Lightfoot1, Roser Juanola-Parramon2, Giorgio Savini2; 1U.K.A.T.C., UK; 2Univ. College London, UK. FIInS is a Python software package developed to simulate the performance of a Double Fourier Interferometer in space. FIInS will ‘observe' a model sky and incorporate the physics and errors expected from a real system.

JM3A.10 Performance Requirements for a Spectral-Spatial Calibration Source for DFM Interferometers, Nicola Baccichet1, Giorgio Savini1, Roser Juanola-Parramon1, Roger Stabbins1; 1Univ. College London, UK. The performance required for a spectral-spatial calibration source to be used in a Double Fourier Modulating Interferometer at far-infrared wavelengths is discussed. Different requirement sets are considered, depending on the possible usage of such sources.

JM3A.11 Modeling and Simulation of the Optical Properties of Low-speed Target in Near Space, Hang Chen1; 1The Academy of Equipment, China. We present an optical properties modeling method based on the reverse Monte Carlo optical tracking techniques. Some numerical simulations are achieved to demonstrate the accuracy and capability of the proposed modeling method.

JM3A.12 The Reconstruction of Interference Hyperspectral Image Based on Multi-DSP Parallel Processing Technique, Jiwen Guo1, Xing Ming1, Bo Q. Lv1, Yue X. Liu1; 1Chinese Academy of Sciences, China. This presentation will discuss Interference spectroscopy, parallel processing, spectral inversion, and Multi-DSP.

JM3A.13 The Spatial Modulated Spectrometer Based on the Fabry-Perot Etalon, Du Shusong1; 1Academy of Opto-Electronics (AOE), China. A new kind of spatial modulated spectrometer based on the special Fabry-Perot Etalon was described. The most merit of the spectrometer is the simple and compact structure. It can be used in remote sensing fields.

JM3A.14 The Cirrus Coupled Cloud-Radiation Experiment: CIRCCREX, Juliet C. Pickering1, Cathryn Fox1, Jonathan Murray1, Alan Last1; 1Imperial College London, UK. We report early results from the Cirrus Coupled Cloud-Radiation Experiment CIRCCREX investigating cirrus through airborne campaigns including radiation measurements (0.3-125µm). Cirrus models and parameterizations used in radiative transfer codes and numerical weather prediction will be tested.

JM3A.15 Investigating BRDF effects based on optical multi-angular laboratory and hyperspectral UAV measurements, Peter Roosjen1, Harm Bartholomeus1, Juha Suomalainen1, Jan Clevers1; 1Wageningen Univ., Netherlands. We investigated BRDF effects of sugar beet crops under field and laboratory conditions based on hyperspectral measurements with a UAV, flown parallel to the sun and multi-angular laboratory measurements.

JM3A.16 High Spatial Resolution LWIR Hyperspectral Sensor, Carson Roberts1, William A. Bodkin1, James T. Daly1 ; 1Bodkin Design and Engineering, USA. A multiplexed, slit-scanning hyperspectral imager with spatial resolution of 320x240 pixels and spectral resolution of 20 nm over 8 to 12.5 microns has been developed. The system can acquire hyperspectral images at 3 Hz.

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FTS HISE

15:00 -- 17:00 FM4A • New Instruments/SIFTS Presider: Geoffrey Toon; Jet Propulsion Laboratory, USA

15:00 -- 17:00 HM4B • New Spectrometer Design and Sensor Characterization II Presider: Jonathan Neumann; US Naval Research Laboratory, USA

FM4A.1 • 15:00 MIGHTI: The Spatial Heterodyne Instrument for Thermospheric Wind Measurements on Board the ICON Mission, Christoph R. Englert1, John Mark Harlander2, Charles Brown1, Jonathan Makela3, Kenneth Marr4, Thomas Immel5; 1US Naval Research Laboratory, USA; 2St Cloud State Univ., USA; 3Univ. of Illinois at Urbana-Champaign, USA; 4Praxis, USA; 5Univ. of California - Berkeley, USA. We describe the Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI), an instrument currently being built to measure thermospheric wind and temperature as part of the NASA Ionospheric Connection (ICON) Explorer mission.

HM4B.1 • 15:00 Compact Hyperspectral Sensor Development, Michael Yetzbacher1, Christopher Miller1, Michael DePrenger2; 1Naval Research Laboratory, USA; 2Tekla Research Inc., USA. Users of spectral information desire more compact, lower cost sensors. We examine design considerations for different types of compact hyperspectral sensors and propose a basis of metrics for the comparison of dissimilar spectrometers.

FM4A.2 • 15:30 Palm-Size Portable Apparatus of Wide-Field Fourier-Spectroscopic-Imaging for Mid Infrared Light, Ichirou Ishimaru1; 1Kagawa Univ., Japan. This presentation will discuss palm-size portable apparatus of wide-field fourier-spectroscopic-imaging for mid infrared light.

HM4B.2 • 15:30 1-km Resolution Mapping from Space with a Sub-Nanometer Spectral Resolut ion Imaging Spectrometer, Akihiko Kuze1, Tadashi Imai1, Hiroshi Suto1; 1Japan Aerospace Exploration Agency, Japan. A compact grating imaging spectrometer with sub-nanometer resolution achieved by limiting spectral coverage is presented. Its applications include monitoring gross primary production of forests and farms, cloud top height, and air quality of mega cities.

HMHM4B.3 • 15:45 Hyperspectral Imaging in the Thermal Infrared: Existing and Future Instruments, William R. Johnson1, Simon J. Hook1, Glynn Hulley1, David Ting1, Daniel W. Wilson1; 1Jet Propulsion Laboratory, USA. HyTES is a compact, high etendue, wide swath sensor which acquires both high spatial and spectral resolution. Future concepts utilize a similar architecture but expand the wavelengths region to include mid wave as well as long wave hyperspectral sensing in one instrument.

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FTS HISE

15:00 -- 17:00 FM4A • New Instruments/SIFTS—Continued

15:00 -- 17:00 HM4B • New Spectrometer Design and Sensor Characterization II—Continued

FM4A.3 • 16:00 Design and Laboratory Tests of the Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI) on the Ionospheric Connection Explorer (ICON) Satellite, John Mark Harlander1, Christoph R. Englert2, Charles Brown2, Kenneth Marr2, Ian Miller3; 1St Cloud State Univ., USA; 2Space Science Division, Naval Research Laboratory, USA; 3LightMachinery, Inc., Canada. We describe the design and laboratory tests of the Michelson Interferometer for Global High-resolution Thermospheric Imaging (MIGHTI), designed to measure thermospheric wind and temperature for the NASA-sponsored Ionospheric Connection (ICON) Explorer mission.

HM4B.4 • 16:00 A Novel Hyperspectral Imager Based on Microslice Technology, Ray M. Sharples1; 1Physics, Univ. of Durham, UK. We present the design and initial performance metrics for a novel snapshot hyperspectral imager based on the use of advanced micro-optics technology. We discus design optimisation process and some initial results from the integration and test of a prototype laboratory demonstrator.

FM4A.4 • 16:15 Current status and perspectives for Microspoc, the miniature Fourier transform spectrometer, Yann Ferrec1, Florence de la Barrière1, Etienne Le Coarer2, Thomas Diard1,2, Nicolas Guérineau1, Guillermo Martin2, Sylvain Rommeluère1, Bernard Schmitt2, Fabrice Thomas2; 1ONERA, France; 2IPAG, France. Microspoc is a family of miniaturized static Fourier transform spectrometers based on a wedge interferometer directly integrated on the focal plane array. Current status and perspective for visible and infrared instruments are presented.

HM4B.5 • 16:15 The Portable Remote Imaging Spectrometer (PRISM): Recent Campaigns and Developments, Pantazis Mouroulis1; 1Jet Propulsion Laboratory, USA. We present results from recent PRISM campaigns in Florida and California as well as a summary of improvements that enable operation on NASA's ER-2 high altitude aircraft and their impact on instrument performance.

FM4A.5 • 16:30 Results from the First Flight Campaign of Sieleters, an Airborne Infrared Imaging Fourier Transform Spectrometer, Yann Ferrec1, Christophe Coudrain1, Laurent Poutier2, Jérôme Primot1, Laurent Rousset-Rouvière1, Sophie Thétas1; 1ONERA, France; 2ONERA, France. Sieleters is an airborne MWIR and LWIR imaging Fourier Transform Spectrometer developed at Onera. The first flight campaign was led at the end of 2013. Experimental results are presented, including a comparison with simulated data.

HM4B.6 • 16:30 Aberration Control of a Concave Grating for Hyperspectral Imager, Cheng-Hao Ko1, Chia-Hui Tang1, Jih-Run Tsai2, Bang-Ji Wang2; 1National Taiwan Univ of Science & Tech, Taiwan; 2National Space Organization, Taiwan. An optimization process to control the aberration of a concave grating is developed. The approach has a dramatic improvement in aberration reduction and spectral resolution. Calculated result is in good agreement with measurement.

FM4A.6 • 16:45 Multiple Beam Fourier Transform Spectroscopy, Christopher Miller1, Michael Yetzbacher1, Michael DePrenger2; 1Applied Optics, U. S. Naval Research Laboratory, USA; 2Tekla Research Inc., USA. Fourier processing has previously been applied to multiple-beam interferograms. However, Fourier theory is only strictly valid in the two-beam limit. We present a solution method for spectral recovery from multi-beam interferograms.

HM4B.7 • 16:45 A Panoramic Short-wave Infrared Hyperspectral Imager for Wide Area Maritime Sensing, K Peter Judd1, Jonathan Nichols1, Katherine Lee1, John Fisher2, Dan Guerin2, Colin Olson3, Costa Colbert4; 1NRL, USA; 2Brandywine Photonics, USA; 3Sotera Defense Solutions, USA; 4Smart Logic Inc., USA. This presentation examines the design, operation, and application of a prototype panoramic compact passive short-wave infrared hyperspectral imager for sensing of maritime environments. Performance characteristics of the system and representative imagery are presented.

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Pineview

09:00 -- 10:30 JT1A • Joint Plenary Session Presider: Alan Schaum; US Naval Research Laboratory, USA

JT1A.1 • 09:00 Advancing Climate Benchmark Measurements, Henry E. Revercomb1; 1Univ. of Wisconsin-Madison, USA. Abstract not available.

JT1A.2 • 09:45 Anomalousness: How to Measure What You Can't Define, James Theiler1; 1Los Alamos National Laboratory, USA. Because it is hard to define an anomaly, it is problematic to measure the effectiveness of anomaly detectors. One proposed definition leads to a volume-based performance measure, which is illustrated on some kernel-based anomaly detectors.

10:30—11:00 • Coffee Break



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FTS HISE

11:00 -- 12:00 FT2A • Comb II/Dispersed Interfermetry Presider: Juliet Pickering; Imperial College London, UK

11:00 -- 12:00 HT2B • Retrieval and Inversion of Hyperspectral Measurements I Presider: Jun Wang; Univ. of Nebraska Lincoln, USA

FT2A.1 • 11:00 Fourier Transform Spectroscopy with Laser Frequency Combs, Nathalie Picque1; 1Max Planck Inst. of Quantum Optics, Germany. New opportunities for Fourier transform spectroscopy are opened up by laser frequency combs. Nonlinear Fourier transform spectroscopy demonstrates an intriguing potential for Doppler-free spectroscopy as well as for hyperspectral imaging.

HT2B.1 • 11:00 Advanced Radiative Models and Retrieval Algorithms for Hyperspectral Remote Sensing Data, Xu Liu1; 1NASA Langley Research Center, USA. A super-fast and accurate radiative transfer model and an optimal estimation retrieval algorithm have been developed specifically for hyperspectral sensors. Using all spectral channels, the algorithm retrieves cloud, atmospheric, and surface properties under both clear and cloudy sky conditions.

FT2A.2 • 11:30 Multiheterodyne Infrared Spectroscopy with Pitch-agile Optical Frequency Comb Generators, Adam J. Fleisher1, David A. Long1, Joseph T. Hodges1, David F. Plusquellic1; 1National Inst of Standards & Technology, USA. Multiheterodyne spectroscopy performed with electro-optic modulator frequency combs generated from a single continuous-wave seed laser provides comb-mode-spacing (pitch) agility by simply tuning the drive frequency of a fast microwave source.

HT2B.2 • 11:30 Temperature-Emissivity Separation Algorithms for Hyperspectral Imaging Spectrometers, Christoph C. Borel-Donohue1; 1Air Force Inst. of Technology, USA. The ARTEMISS (Automatic Retrieval of Temperature and Emissivity using Spectral Smoothness) method was developed over the last 13 years to retrieve temperature, emissivity and associated uncertainties from data collected with hyper-spectral imaging spectrometers.

FT2A.3 • 11:45 Phase Stepping Algorithm For Unknown Irregular Steps: Applications in Dispersed Interferometry, David J. Erskine1; 1Lawrence Livermore National Laboratory, USA. We process externally dispersed interferometer spectral data with a novel phase-stepping algorithm tolerating steps of unknown irregular phase and visibility, which change significantly across a 0.9 to 2.5 micron bandwidth.

Congress Program Update Sheet

All technical program changes will be communicated in the onsite Congress Program

Update Sheet. All attendees receive this information with registration materials, and we

encourage you to review it carefully to stay informed to changes in the program.

Accepted postdeadline papers will also be announced on the Update Sheet.

12:00—13:00 • Lunch, Dining Room

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FTS HISE

13:00 -- 15:00 FT3A • Astronomy, Planetary, Imaging FTS Presider: David Naylor; Univ. of Lethbridge, Canada

13:00 -- 14:45 HT3B • Retrieval and Inversion of Hyperspectral Measurements II Presider: Christoph Borel; Air Force Inst. of Technology, USA

FT3A.1 • 13:00 From 1D-Fourier Transform Spectroscopy to Imaging Fourier Transform Spectroscopy in Astronomy, Jean-Pierre Maillard1; 1Institut d'astrophysique de Paris, France. FT spectroscopy started successfully in astronomy almost 50 years by 1D-FT on planets and stars. Today, Imaging FTSs only remain in use, providing unique capabilities of integral wide-field spectroscopy on a variety of extended sources, from the visible to the submillimetric domain.

HT3B.1 • 13:00 Satellite, Airborne, and Ground-based Remote Sensing, William L. Smith1, Allen Larar2, Bradley Pierce3, Henry E. Revercomb1, Nadia Smith1, Joseph Turner1, Elisabeth Weisz1, Melissa Yesalusky4; 1Space Science and Engineering Center, Univ. of Wisconsin, USA; 2NASA Langley Research Center, USA; 3NOAA/NESDIS CIMSS, Univ. of Wisconsin, USA; 4Hampton Univ., USA. Results from combining satellite, or airborne, FTS measurements with ground-based FTS , chemistry model, and in-situ observations, obtained during several satellite validation campaigns, are presented to demonstrate the synergistic use multi-platform remote sensing and in-situ observations.

HT3B.2 • 13:30 Emissivity Retrieval in LWIR Hyperspectral Desert Scenes, Steven M. Adler-Golden1; 1Spectral Sciences, Inc., USA. Atmospheric compensation algorithms for LWIR hyperspectral imagery typically require the presence of blackbody surfaces, resulting in failure with many desert scenes. The FLAASH-IR algorithm is successfully applied to challenging SEBASS and HyTES desert images.

FT3A.2 • 13:45 Observing the South Pole of Enceladus using Cassini/CIRS as a Radiometer, Nicolas J. Gorius1, John Spencer2, Carly Howett2, Donald E. Jennings3, John Brasunas3, Shane Albright4; 1Inst. for Astrophysics & Computational Sciences, The Catholic Univ. of America, USA; 2Southwest Research Inst., USA; 3NASA Goddard Space Flight Center, USA; 4System & Software Designers, Inc, USA. The Composite Infrared Spectrometer aboard the Cassini spacecraft has been making numerous observations of the Saturnian system since 2004. This talk will present the instrument models specifically developed to analyze our observations of the South Pole of Enceladus while using CIRS as a radiometer.

HT3B.3 • 13:45 Derivation of clear-sky longwave spectral flux solely from hyperspectral observations: a case study with AIRS observations, Xiuhong Chen1, Xianglei Huang1; 1Univ. of Michigan, USA. We extend the algorithm developed by Huang et al. (2008) to derive clear-sky longwave spectral fluxes exclusively from AIRS radiance alone. Clear-sky and scene-type information are determined using AIRS radiances. Performance of the algorithms is quantified.

HT3B.4 • 14:00 Polarized above sea surface hyperspectral observations and their relationship with measured water properties, Robert Foster1, Amir Ibrahim1, Alexander Gilerson1, Carlos Carrizo1, Ahmed El-Habashi1, Sam Ahmed1; 1CUNY City College, USA. Polarized radiometric measurements above and below the sea surface are combined to develop a glint correction scheme for the polarized signal from the ocean, and compare it with one simulated by a vector RT code.

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FTS HISE

13:00 -- 15:00 FT3A • Astronomy, Planetary, Imaging FTS—Continued

13:00 -- 14:45 HT3B • Retrieval and Inversion of Hyperspectral Measurements II—Continued

FT3A.3 • 14:15 Observations of Titan from the Cassini Composite Infrared Spectrometer, Donald E. Jennings1; 1NASA Goddard Space Flight Center, USA. The Composite Infrared Spectrometer (CIRS) is a Fourier transform spectrometer flying on the Cassini spacecraft at Saturn. Since 2004 CIRS has observed the atmosphere and surface of Titan in the 7-1000 micron spectral range.

HT3B.5 • 14:15 Attribution of Earth-reflected Hyperspectral Data using Bayesian Positive Source Separation, Odele M. Coddington1, Peter Pilewskie1,2, Bruce C. Kindel1; 1LASP/Univ. of Colorado Boulder, USA; 2Atmospheric and Oceanic Science, Univ. of Colorado Boulder, USA. We treat Earth-reflected radiation as mixtures of spectra unique to sources of scattering and absorption in Earth's atmosphere and surface. We identify the signals and quantify their mixtures using source separation in a Bayesian framework.

FT3A.4 • 14:30 Pre-Shipment Characterization of SITELLE, a Wide-field Imaging Fourier Transform Spectrometer for the Canada-France-Hawaii Telescope, Julie Mandard1, Frederic J. Grandmont1, Laurent Drissen2, Simon Thibault2, Marc Baril3, Louis Moreau1; 1ABB, Canada; 2Département de physique, de génie physique et d'optique, Universite Laval, Canada; 3CFHT Corporation, USA. SITELLE is a wide-field imaging FTS to be deployed at the Canada-France-Hawaii Telescope. It is a challenging instrument with a unique combination of characteristics. We present the instrument and a summary of the pre-shipment tests.

HT3B.6 • 14:30 An algorithm for simultaneous inversion of aerosol properties and surface reflectance from airborne GeoEO-TASO hyperspectral data, Jun Wang1; 1Univ. of Nebraska Lincoln, USA. This paper presents an inversion method to simultaneously retrieve aerosol and surface properties from the hyperspectral data collected by airborne GeoEO-TASO (Geostationary Trance gas and Aerosol Sensor Optimization).

FT3A.5 • 14:45 Herschel SPIRE FTS Spectral Line Source Calibrators, Rosalind Hopwood1, Edward Polehampton2,3, Ivan Valtchanov4, Trevor Fulton3, Nanyao Lu5, Nicola Marchili6, David A. Naylor3, Gibion Makiwa3, Locke D. Spencer3, Bruce Swinyard2,7, Matthijs van der Wiel3,8; 1Imperial College London, UK; 2RAL Space, UK; 3Inst. for Space Imaging Science Centre, Univ. of Lethbridge, Canada; 4ESAC, Spain; 5NASA Herschel Science Center, Califonia Inst. of Technology, USA; 6Univ. of Padova, Italy; 7Physics and Astronomy, Univerity College London, UK; 8Niels Bohr Inst., Denmark. We present a summary of the Herschel SPIRE/FTS calibration programme to monitor the repeatability of spectral lines. Observations of planetary nebulae and post-AGB stars are used to assess repeatability and model the asymmetry of the instrument line shape.

15:00—15:30 • Beverage Break

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FTS HISE

15:30 -- 17:30 FT4A • Imaging FTS in Astronomy Presider: David Johnson; NASA Langley Research Center, USA

15:30 -- 17:30 HT4B • Atmospheric Measurements, Modeling and Compensation Methods Presider: Xu Liu; NASA Langley Research Center, USA

FT4A.1 • 15:30 Aperture Synthesis Imaging with Fourier and Intensity Interferometers, Hiroshi Matsuo1; 1National Astronomical Observatory Japan, Japan. Aperture synthesis imaging technologies using direct detectors are discussed; one with multi-Fourier transform interferometry and another with intensity interferometry. Direct detector interferometry will open high sensitivity and high angular resolution interferometry in terahertz frequencies.

HT4B.1 • 15:30 Status of Atmospheric Effects Modeling and Compensation for Hyperspectral Imagery, Steven M. Adler-Golden1; 1Spectral Sciences, Inc., USA. This talk summarizes the current state of the art in atmospheric effects modeling and compensation for HSI, distinguishing straightforward from difficult cases, assessing approximate RT schemes, and highlighting current directions and unsolved problems.

FT4A.2 • 16:00 Astronomical Far-infrared Imaging Fourier Transform Spectroscopy: the Challenges and the Potential, David A. Naylor1; 1Univ. of Lethbridge, Canada. Many leading questions in modern astrophysics will be addressed by sensitive imaging spectroscopic observations at far-infrared wavelengths. The technical challenges associated with far-infrared Imaging Fourier transform spectrometers, which have emerged as the solution of choice, are reviewed.

HT4B.2 • 16:00 Examining the Role Geometry Plays in Spectral Emissivity Retrieval, Joseph Meola1; 1US Air Force Research Laboratory, USA. Remotely sensed longwave infrared hyperspectral imagery is often used for material identification. This imagery must be compensated for atmospheric effects in order to retrieve emissivity information about the objects in the scene. This work examines how surface geometry and sensor viewing geometry can impact the retrieved emissivity of objects.

FT4A.3 • 16:30 Progress in the Critical Assessment for a Far-Infrared Space Interferometer with Double Fourier Modulation (FP7-FISICA), Giorgio Savini1, Peter A. Ade2, Nicola Baccichet1, Colm Bracken3, Kjetil Dohlen4, Anthony Donohoe3, Brad Gom5, Matthew J. Griffin2, Wayne Holland6, Valerio Iafolla7, Rob Ivison8, Martyn Jones9, Roser Juanola-Parramon1, John Lightfoot6, Scige Liu10, Alison McMillan9, J. A. Murphy3, David A. Naylor5, Creidhe O'Sullivan3, Enzo Pascale2, Stefano Pezzuto10, Eddy Rakotonimbahy4, Daniele Schito7, Locke D. Spencer5, Luigi Spinoglio10, Bruce Swinyard1, Ian Veenendaal5, Sebastien Vives4, David Walker9, David T. Leisawitz11, Sheng-Cai Shi12, Hiroshi Matsuo13; 1Univ. College London, UK; 2Physics & Astronomy, Cardiff Univ., UK; 3Physics, National Univ. of Ireland Maynooth, Ireland; 4L.A.M., France; 5Physics & Astronomy, Univ. of Lethbridge, Canada; 6UK-ATC, UK; 7Assist in Gravitation and Instrumentation, Italy; 8Royal Observatory of Edinburgh, UK; 9Physics, Glyndwr Univ., UK; 10IAPS-INAF, Italy; 11NASA - Goddard Space Flight Centre, USA; 12Purple Mountain Observatory, China; 13National Astronomical Observatory Japan, Japan. The progress and results of the ongoing FP7-FISICA programme to re-asses the scientific goals of a Far-Infrared Space Interfereometer and push the development of some of its key technology elements are reported.

HT4B.3 • 16:30 Accounting for Sub-Pixel Variability of Clouds and/or Unresolved Spectral Variability, as Needed, with Generalized Radiative Transfer Theory, Anthony B. Davis1,3, Feng Xu1, William D. Collins2,4; 1Jet Propulsion Laboratory, USA; 2Department of Earth and Planetary Science, Univ. of California - Berkeley, USA; 3JIFRESSE, UCLA, USA; 4Earth Sciences Division, Lawrence Berkeley National Laboratory, USA. Atmospheric hyperspectral VNIR sensing struggles with sub-pixel variability of clouds and limited spectral resolution mixing molecular lines. Our generalized radiative transfer model addresses both issues with new propagation kernels characterized by power-law decay in space.

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FTS HISE

15:30 -- 17:30 FT4A • Imaging FTS in Astronomy—Continued

15:30 -- 17:30 HT4B • Atmospheric Measurements, Modeling and Compensation Methods—Continued

FT4A.4 • 16:45 Astrophysical Capabilities of a Double Fourier Modulation Interferometer in Space, Roser Juanola-Parramon1, Danielle Fenech1, Giorgio Savini1; 1Univ. College London, UK. Here we present how the Far-infrared Interferometer Instrument Simulator (FIInS) is used to simulate an observation of astronomical targets. The selection of the instrument parameters (spectral and spatial) is discussed and the obtained results analyzed.

HT4B.4 • 16:45 Observations Of Downwelling Far-Infrared Radiance At Earth's Surface with FIRST, Martin G. Mlynczak1, Richard Cageao1, Harri Latvakoski2, David Kratz1, Jeffrey Mast3, David G. Johnson1; 1NASA Langley Research Ctr, USA; 2Space Dynamics Laboratory, USA; 3SSAI, USA. Far-infrared radiance from the atmosphere was observed at Earth's surface at Cerro Toco, Chile, and Table Mountain, CA with the NASA FIRST instrument. Measurements are compared with model calculations, showing agreement within their combined uncertainty.

FT4A.5 • 17:00 Longwavelength Issues for Far Infrared Ipace interferometers, J. A. Murphy1, Creidhe O'Sullivan1, Anthony Donohoe1, Colm Bracken1, Marcin Gradziel1, Giorgio Savini2, Roser Juanola-Parramon2, John Lightfoot3, Locke Spencer4, Peter Ade5; 1National Univ. of Ireland, Maynooth, Ireland; 2Univ. College London, UK; 3Astronomy Techonolgy Centre Royal Observatory, UK; 4Univ. of Leithbridge, Canada; 5Cardiff Univ., UK. We discuss issues associated with diffraction effects in far-infared space interferometers, particularly wide field spacio-spectral space interferometers now being proposed. We present examples of the application of various useful quasi-optical approaches in such instruments.

HT4B.5 • 17:00 Effective multi-scattering-stream model for fast radiative transfer simulation, Qiguang Yang1, Xu Liu1, Ping Yang2, Chenxi Wang2; 1NASA Langley Research Center, Hampton, VA 23681, USA; 2Department of Atmospheric Sciences, Texas A & M Univ., USA. A fast solar spectral radiative transfer model with high accuracy and fast computation speed is developed based on a new effective multi-scattering-stream model for hyperspectral remote-sensing applications in cloudy atmosphere.

FT4A.6 • 17:15 Development of a Far-Infrared Double Fourier Spatial/Spectral Interferometery Laboratory Testbed Instrument, Locke D. Spencer1, Peter A. Ade2, William F. Grainger4, Matthew J. Griffin2, Roser Juanola-Parramon3, David A. Naylor1, Enzo Pascale2, Giorgio Savini3, Bruce Swinyard3; 1Univ. of Lethbridge, Canada; 2School of Physics and Astronomy, Cardiff Univ., UK; 3Physics and Astronomy, Univ. College London, UK; 4STFC Rutherford Appleton Laboratory, UK. The design of a laboratory-based far-infrared double Fourier spatial/spectral interferometer is presented. This instrument is a testbed platform for the development of imaging techniques, data processing algorithms, and component characterization for space-based astronomical applications.

HT4B.6 • 17:15 Estimating Index of Refraction from Polarimetric Hyperspectral Imagery, Jacob Martin1, Kevin Gross1; 1AFIT/ENP, USA. This works shows that spectral refractive index can be estimated to within 15\% from laboratory polarimetric hyperspectral imaging measurements, without \emph{a priori} knowledge of surface temperature or downwelling radiance.

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Optics and Photonics for Energy & the Environment (E2)

2-6 November 2015, Suzhou China

Visit www.osa.org/E2 for more information.




FTS HISE

09:00 -- 10:15 FW1A • Calibration and Validation Presider: To be Announced

09:00 -- 10:30 HW1B • Planned and Deployed Operational Systems Presider: Xianglei Huang; Univ. of Michigan, USA

FW1A.1 • 09:00 Ensuring Consistency of the Total Carbon Column Observing Network (TCCON) Stations, Frank Hase1; 1Universität Fridericiana Karlsruhe, Germany. TCCON is a network of ground-based FTIR spectrometers which provides accurate and precise atmospheric abundances of greenhouse gases. This talk presents measures taken for ensuring that the observations are highly consistent across the network.

HW1B.1 • 09:00 Implementation of Tropospheric Emissions: Monitoring of Pollution (TEMPO), Kelly V. Chance1; 1Harvard-Smithsonian Ctr for Astrophysics, USA. TEMPO, the first NASA Earth Venture Instrument, will launch in 2019 to measure atmospheric pollution for greater North America from space. Using ultraviolet and visible spectroscopy, TEMPO will measure hourly at about 10 km2 resolution.

FW1A.2 • 09:30 Radiometric calibration of the Radiation Explorer in the Far InfraRed prototype, Luca Palchetti1, Giovanni Bianchini1; 1Istituto Nazionale di Ottica (CNR), Italy. The calibration procedure applied to the wideband REFIR-PAD infrared spectrometer is described along with the results obtained in ground-based campaigns performed since 2009 from high-altitude sites in extremely dry air conditions.

HW1B.2 • 09:30 The MTG-IRS Mission, Stephen Tjemkes1, Stefano Gigli1, Gary Fowler1, Rolf Stuhlmann1; 1EUMETSAT, Germany. This presentation describes the METEOSAT Third Generation - InfraRed Sounder (MTG-IRS) mission in terms of its objective, instrument, ground segment and derived products.

FW1A.3 • 09:45 Suomi NPP/JPSS Cross-track Infrared Sounder (CrIS): Calibration Validation With The Aircraft Based Scanning High-resolution Interferometer Sounder (S-HIS), Joe Taylor1, David Tobin1, Henry Revercomb1, Fred Best1, Raymond Garcia1, Howard Motteler2, Mitch Goldberg3; 1Univ. of Wisconsin-Madison, USA; 2Univ. of Maryland Baltimore County, USA; 3Joint Polar Satellite Systems Office, National Oceanic and Atmospheric Administration, USA. A summary of the Cross-track Infrared Sounder (CrIS) radiometric calibration validation assessment conducted using the aircraft based Scanning High-resolution Interferometer Sounder (S-HIS) during the SNPP 2013 calibration

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FTS HISE

09:00 -- 10:15 FW1A • Calibration and Validation– Continued

09:00 -- 10:30 HW1B • Planned and Deployed Operational Systems—Continued

FW1A.4 • 10:00 Atmospheric Chemistry Experiment Fourier Transform Spectrometer (ACE-FTS) Version 3.5 Validation, Kaley A. Walker1,2, Patrick E. Sheese1, Chris D. Boone2, Peter F. Bernath3; 1Univ. of Toronto, Canada; 2Univ. of Waterloo, Canada; 3Old Dominion Univ., USA. This paper will describe current validation results for the Atmospheric Chemistry Experiment Fourier Transform Spectrometer (ACE-FTS) focusing on version 3.5 of the data set.

HW1B.3 • 10:00 Calibration Demonstration System for the Reflected Solar, Kurtis J. Thome1; 1NASA Goddard Space Flight Center, USA. The CLARREO mission addresses the need to observe high-accuracy, long-term climate change trends and advance the accuracy of SI traceable absolute calibration. The current work describes the calibration demonstration system for the reflected solar portion of CLARREO.


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FTS HISE

11:00 -- 12:00 FW2A • Lab Measurements Presider: Adam Fleisher; National Inst of Standards & Technology, USA

11:00 -- 12:00 HW2B • Advanced Detection, Image Segmentation and Pattern Recognition Presider: Fred Kruse; Naval Postgraduate School, USA

FW2A.1 • 11:00 Recent Developments in FT Laboratory Spectroscopy at DLR, Manfred Birk1, Georg Wagner1, Joep Loos1; 1German Aerospace Center, Germany. Absorption cells were improved regarding absorption path, temperature homogeneity and spectral coverage. Multispectrum fitting was introduced using most advanced line profiles. Species investigated recently are BrONO2, H2O, CH4 and N2O.

HW2B.1 • 11:00 A Compressive Hyperspectral Imaging System based on Parallel Processing, Mohammad Azari1, Mehrdad Abolbashari2, Faramarz Farahi1; 1UNC Charlotte, USA; 2OPTONIKS CORP, USA. A new approach to hyperspectral compressive imaging system based on parallel processing is developed. The architecture of system is based on single-pixel compressive imaging. By parallelizing the recovery algorithm and using multicore CPUs and GPUs, we address high computational requirement.

HW2B.2 • 11:15 Analytical Modeling of a Linear Variable Filter for Computational Hyperspectral Imaging, Cheng-Hao Ko1, Kuei-Ying Chang1, You-Min Huang1, Jih-Run Tsai2, Bang-Ji Wang2; 1National Taiwan Univ of Science & Tech, Taiwan; 2National Space Organization, Taiwan. An analytical thin film thickness model calculates the profiles of linear variable filters, which perform spectral filtering. Coupled with an image sensor and using a computational algorithm, this device becomes a LVF-hyperspectral imager.

FW2A.2 • 11:30 IFTS for Harmonically Unsteady Combustion, Michael Rhoby1, Kevin Gross1; 1ENP, Air Force Inst. of Technology, USA. Combustion studies can benefit from spatially- and temporally-resolved wide-band spectra. We demonstrate an algorithm permitting reconstruction of "snapshot" spectra from harmonically unsteady diffuse laminar flames using a measurement ensemble from a free-running imaging FTS.

HW2B.3 • 11:30 Multimodal Data Fusion via Graph- and Operator-based Techniques, Alexander Cloninger2, Wojciech Czaja3, Timothy Doster1; 1Naval Research Laboratory, USA; 2Department of Mathematics, Yale Univ., USA; 3Norbert Wiener Center - Department of Mathematics, Univ. of Maryland, College Park, USA. Utilizing Laplacian Eigenmaps we are able to leverage information from multimodal sensors (i.e., hyperspectral and LIDAR) to improve image classification results. We develop distance measures, joint kernels, and utilize feature space rotations to achieve fusion.

FW2A.3 • 11:45 Reduction of Artifacts from Scene Intensity Fluctuations in Hyperspectral Images Using Four-Port Imaging Spectroradiomete, Florent Prel1, Stephane Lantagne1, Louis Moreau1, Claude Roy1; 1ABB, Canada. Scene intensity fluctuations during acquisition create artifacts in the acquired spectra of imaging Fourier Transform Spectrometers. We describe a correction process based on the information provided by the second output of a four-port imaging FTS.

HW2B.4 • 11:45 Use of Polarimetric Imaging for Discrimination of Oil from Water, Amber L. Iler1, Patrick D. Hamilton1; 1Integrity Applications Incorporated, USA. IAI collected visible polarimetric data of crude oil and vegetable oil on water at multiple sun angles and found the degree of linear polarization (DOLP) product to be capable of discriminating these liquids.

12:00—13:00 • Lunch Break , Dining Room

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FTS Room HISE Room

FTS HISE

13:00 -- 15:00 FW3A • Earth Atmosphere Algorithms and Instruments Presider: Peter Bernath; Old Dominion Univ., USA

13:00 -- 14:30 HW3B • Multimodal Fusion and Visualization Algorithms Presider: Joseph Meola; US Air Force Research Laboratory, USA

FW3A.1 • 13:00 A Fourier Transform Spectroradiometer for the Remote Sensing of the Atmospheric Emission from Ground Bases in Extreme Environments, Giovanni Bianchini1, Gianluca Di Natale1, Francesco Castagnoli1, Luca Palchetti1; 1INO-CNR, Italy. A ground based FT spectroradiometer with a 5-100 μm spectral range, room temperature detectors, low power consumption and a robust optical and electronic design is operating continuously from the Concordia Station, Antarctica.

HW3B.1 • 13:00 Combined Analysis of Visible-near Infrared (VNIR), Shortwave Infrared (SWIR), and Longwave Infrared (LWIR) Imaging Spectrometer Data, Fred A. Kruse1,2, Meryl L. McDowell2,3, Shelli R. Cone2,3; 1Physics Department, Naval Postgraduate School, USA; 2Remote Sensing Center, Naval Postgraduate School, USA; 3Scitor Corporation, USA. VNIR, SWIR and LWIR imaging spectrometer data are typically analyzed using individual spectral ranges. Integrating modalities to extract complimentary information allows improved characterization and mapping that cannot be accomplished using a single spectral range.

FW3A.2 • 13:30 A Compact Automated FTS at the Desert Playa for Satellite Validation of the Total Column CO2 and CH4, Shuji Kawakami1, Akihiko Kuze1, Patrick W. Hillyard2, James Podolske2, Tomoaki Tanaka2, Laura Iraci2, Randal Albertson3, Andre Butz4, Fumie Kataoka5, Kazutaka Murakami6, Kei Shiomi1, Eri Katoh1, Hiroshi Suto1; 1Japan Aerospace Exploration Agency, Japan; 2Ames Research Center, NASA, USA; 3Armstrong Flight Research Center, NASA, USA; 4IMK-ASF, Karlsruhe Inst. of Technology, Germany; 5Remote Sensing Technology Center of Japan, Japan; 6National Inst. for Environmental Studies, Japan. A compact automated FTS using direct solar light provide accurate and precise column CO2 and CH4 at the desert playa, where surface albedo is high and the number of validation sites is limited.

HW3B.2 • 13:30 Measuring the Spatial and Spectral Performance of WorldView-3, Nathan W. Longbotham1, Fabio Pacifici1, Seth Malitz1, William Baugh1, Gustau Camps-Valls2; 1DigitalGlobe, USA; 2Universitat de València, Spain. The new WorldView-3 satellite provides a unique combination of very high spatial resolution and super-spectral capabilities. This presentation explores the practical and theoretical usefulness of this platform as compared against other hyperspectral and multispectral sensors.

FW3A.3 • 14:00 The Univ. of Wisconsin Space Science and Engineering Center Absolute Radiance Interferometer (ARI): Demonstrated Radiometric Performance, Joe Taylor1,2, Henry Revercomb1, Fred Best1, Jonathan Gero1, David Tobin1, Robert O. Knuteson1, Henry Buijs3, Frederic Grandmont3, Jerome Genest2; 1Univ. of Wisconsin-Madison, USA; 2Université Laval, Canada; 3ABB-Bomem Inc., Canada. A summary of the Absolute Radiance Interferometer (ARI) radiometric performance demonstrated during vacuum testing at the Univ. of Wisconsin Space Science and Engineering Center (UW-SSEC) is presented.

HW3B.3 • 14:00 Hyperspectral Band Selection Using the Total Dependence Metric, Seyed Enayat Hosseini Aria1, Massimo Menenti1, Ben Gorte1; 1Delft Univ. of Technology, Netherlands. Selecting bands with the lowest redundant information from a hyperspectral dataset is always desirable. This study obtains the most independent bandset by using a state-of-the-art single metric measuring the overall dependence of multivariate systems.

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FTS HISE

13:00 -- 15:00 FW3A • Earth Atmosphere Algorithms and

Instruments—Continued

13:00 -- 14:30 HW3B • Multimodal Fusion and Visualization Algorithms—Continued

FW3A.4 • 14:15 Spike Detection and Correction of Interferograms Recorded by an Imaging Fourier Transform Spectrometer, Thomas Latzko1; 1Karlsruhe Inst. of Technology, Germany. A method for spike detection and correction of measurements from the GLORIA experiment is presented. The results shows that even if a spike is close to the interferogram peak, it can be detected and repaired.

HW3B.4 • 14:15 HSI Sharpening with High-Resolution Pen-Chromatic and RGB Cameras , Hai-Wen Chen1; 1Booz Allen Hamilton Inc., USA. A new Band Interpolation and Local Scaling (BILS) method has been developed to improve HSI spatial resolution by 4-16 times with a low-cost high-resolution pen-chromatic camera and a RGB camera. Preliminary results indicate that this new technique is promising.

FW3A.5 • 14:30 Evaluation of the pointing accuracy of a limb sounder using cloud edge detection, Thomas Latzko1, Frriederike Graf1; 1Karlsruhe Inst. of Technology, Germany. A method to extract cloud information from the raw data of the imaging Fourier transform spectrometer GLORIA is presented. The cloud information will deliver information about pointing stability.

FW3A.6 • 14:45 Correction of Ghosts in FTIR Spectra, Geoffrey Toon1; 1Jet Propulsion Laboratory, USA. A method is presented to identify and correct spectral ghosts caused by periodic mis-sampling of the interferogram. For applications in which high measurement accuracy is needed, even small systematic sampling errors (<0.1%) can cause problematic ghosts.




foBase. To access the papers go to www.osa.org/FTS_HISE and select the “Access digest papers”

essential link on the right hand navigation. As access is limited to Full Technical Congress Attendees only, you

will be asked to validate your credentials by entering the same login email address and password provided

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Pineview Room

FTS

15:30 -- 17:15 FW4A • Earth Atmosphere Instruments Presider: Luca Palchetti; Istituto Nazionale di Ottica (CNR), Italy

FW4A.1 • 15:30 From METOP to MTG Twenty Years of FTS Based Developments , Denis Simeoni1; 1Thales Alenia Space France, France. From METOP to MTG the presentation overviews twenty years of ThalesAleniaSpace developments in the field of Fourier Transform Spectrometry. It focuses on the most recent developments, and their contributions to the IR soundings.

FW4A.2 • 16:00 Panchromatic Fourier Transform Spectrometer Engineering Model (PanFTS-EM) for Geostationary Atmospheric Measurements, Stanley P. Sander1, Dmitriy Bekker1, Jean-Francois Blavier1, Maxwell B. Bryk1, Colin Donahue1, Renaud Goullioud1, Bruce Hancock1, Dean Johnson1, Richard Key1, Andrew Lamborn1, Kenneth S. Manatt1, James Moore1, Jamie Nastal1, Timothy J. Neville1, Daniel Preston1, David M. Rider1, Matthew V. Ryan1, James Wincentsen1, Yen-Hung Wu1; 1Jet Propulsion Laboratory, USA. The Panchromatic Fourier Transform Spectrometer Engineering Model is an imaging FTS to meet the requirements for air quality and carbon cycle science from geostationary orbit. PanFTS-EM is a flight-like engineering model which emulates the critical functions of the PanFTS flight instrument.

FW4A.3 • 16:15 On-board Processing to Advance the PanFTS Imaging System for Earth Observation, Jean-Francois Blavier1, Paula J. Pingree1, Dmitriy Bekker1, Rudi M. Bendig1, Maxwell B. Bryk1, Colin Donahue1, Megan E. Fazio1, Brian R. Franklin1, Kenneth S. Manatt1, Colin McKinney1, Nooshin Meshkaty1, Ryan M. Monroe1, David M. Rider1, Matthew V. Ryan1, Stanley P. Sander1, Thomas A. Werne1; 1Jet Propulsion Laboratory, USA. This paper describes the on-board processing approach for PanFTS, an imaging spectrometer designed to observe the Earth atmosphere from geosynchronous orbit.

FW4A.4 • 16:30 IASI-NG Program: A New Generation of Infrared Atmospheric Sounding interferometer, Francois Bermudo1; 1Centre National d'Etudes Spatiales, France. With notable improvements on spectral and radiometric performances compared with first generation, CNES will develop the New Generation of the Infrared Atmospheric Sounding Interferometer (IASI-NG) key element of the Second Generation of European Polar System. This will be a 30 minute contributed presentation.

FW4A.5 ● 17:00 Spatial Heterodyne Spectrometer for Observation of Water for a Balloon Flight: Overview of the Instrument & Preliminary Flight Data Results, Fabien Dupont1, Frederic Grandmont1, Brian Solheim2, Adam Bourassa3, Doug degenstein3, Nicholas Lloyd3, Ryan Cooney4 ; 1.ABB Inc, Canada; 2CRESS, York University, Canada; Inst. of Space and Atmospheric Studies, Univ. of Sakatchewan, Canada; 4Canadian Space Agency, Canada. SHOW is a Spatial Heterodyne Spectrometer designed to vertically resolve water profiles from limb scattered sunlight. The instrument successfully flew at 35 km float altitude. We present an overview of the instrument and preliminary

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A Abolbashari, Mehrdad - HW2B.1 Ade, Peter A. - FT4A.3, FT4A.6, FT4A.5 Adler-Golden, Steven M. - HT3B.2, HT4B.1 Ahmed, Sam - HT3B.4 Albertson, Randal - FW3A.2 Albright, Shane - FT3A.2 Allman, Eric C. - HM2B.1 Atre, Shankar - JM1A.1 Azari, Mohammad - HW2B.1

B

Baccichet, Nicola - FT4A.3, JM3A.10 Baril, Marc - FT3A.4 Bartholomeus, Harm - JM3A.15 Baugh, William - HW3B.2 Baumann, Esther - FM2A.2 Bekker, Dmitriy - FW4A.2, FW4A.3 Bell, Graham - JM3A.5 Belting, Chris - HM2B.2 Bendig, Rudi M. - FW4A.3 Bermudo, Francois - FW4A.4 Bernath, Peter F. - FW1A.4, JM1A.4, FW3A Bernhardt, Birgitta C. - FM2A.1 Best, Fred - FW1A.3, FW3A.3, JM1A.2,

JM3A.2 Bianchini, Giovanni - FW1A.2, FW3A.1 Bintley, Daniel - JM3A.5 Birk, Manfred - FW2A.1 Blavier, Jean-Francois - FW4A.2, FW4A.3 Bodkin, William A. - JM3A.16 Boone, Chris D. - FW1A.4 Borel, Christoph C. - HT3B, HT2B.2 Bourassa, Adam - FW4A.5 Bracken, Colm - FT4A.3, FT4A.5 Brasunas, John - FT3A.2 Brown, Charles - FM4A.1, FM4A.3 Bryk, Maxwell B. - FW4A.2, FW4A.3 Buijs, Henry - FW3A.3 Butz, Andre - FW3A.2

C

Cageao, Richard - HT4B.4 Camps-Valls, Gustau - HW3B.2 Carrizo, Carlos - HT3B.4 Castagnoli, Francesco - FW3A.1 Castleman, Zach - HM2B.2 Chance, Kelly V. - HW1B.1 Chang, Kuei-Ying - HW2B.2 Chen, Hai-Wen - HW3B.4 Chen, Hang - JM3A.11 Chen, Xiuhong - HT3B.3 Clevers, Jan - JM3A.15 Cloninger, Alexander - HW2B.3 Coddington, Ian - FM2A.2 Coddington, Odele M. - HT3B.5 Colbert, Costa - HM4B.7 Collins, William D. - HT4B.3 Cone, Shelli R. - HW3B.1 Cooney, Ryan - FW4A.5 Coudrain, Christophe - FM4A.5 Czaja, Wojciech - HW2B.3

D Daly, James T. - JM3A.16 Davis, Anthony B. - HT4B.3 de la Barrière, Florence - FM4A.4

Degenstein, Doug - FW4A.5 DePrenger, Michael - FM4A.6, HM4B.1 Deschênes, Jean-Daniel - FM2A.2 DeSlover, Daniel - JM3A.2 Di Natale, Gianluca - FW3A.1 Diard, Thomas - FM4A.4 Dohlen, Kjetil - FT4A.3 Donahue, Colin - FW4A.2, FW4A.3 Donohoe, Anthony - FT4A.3, FT4A.5 Doster, Timothy - HW2B.3 Drake, Ginger - HM2B.2 Drissen, Laurent - FT3A.4 Dupont, Fabien - FW4A.5

E El-Habashi, Ahmed - HT3B.4 Englert, Christoph R. - FM4A.1, FM4A.3 Erskine, David J. - FT2A.3 Espejo, Joey - HM2B.2

F Farahi, Faramarz - HW2B.1 Fazio, Megan E. - FW4A.3 Fenech, Danielle - FT4A.4 Ferrec, Yann - FM4A.4, FM4A.5 Fisher, John - HM4B.7 Fleisher, Adam J. - FW2A, FT2A.2 Foster, Robert - HT3B.4 Fowler, Gary - HW1B.2 Fox, Cathryn - JM3A.14 Franklin, Brian R. - FW4A.3 Friberg, Per - JM3A.5 Fulton, Trevor - FT3A.5, JM3A.4, JM3A.7,

JM3A.8

G Garcia, Raymond - FW1A.3, JM1A.2 Genest, Jerome - FW3A.3 Gero, Jonathan - FW3A.3, JM1A.2 Gigli, Stefano - HW1B.2 Gilerson, Alexander - HT3B.4 Giorgetta, Fabrizio - FM2A.2 Goldberg, Mitch - FW1A.3 Gom, Brad - FT4A.3, JM3A.5, JM3A.6 Gorius, Nicolas J. - FT3A.2 Gorte, Ben - HW3B.3 Goullioud, Renaud - FW4A.2 Gradziel, Marcin - FT4A.5 Graf, Frriederike - FW3A.5 Grainger, William F. - FT4A.6 Grandmont, Frederic J. - FW3A.3, FW4A.5,

FT3A.4 Griffin, Matthew J. - FT4A.3, FT4A.6 Gross, Kevin - FW2A.2, HT4B.6 Guelachvili, Guy - FM2A.1 Guerin, Dan - HM4B.7 Guérineau, Nicolas - FM4A.4 Guo, Jiwen - JM3A.12

H Hackel, Denny - JM1A.2 Hamilton, Courteney - JM3A.8 Hamilton, Patrick D. - HW2B.4 Han, Yong - JM1A.1 Hancock, Bruce - FW4A.2 Harlander, John Mark - FM4A.1, FM4A.3,

FW1A

Hase, Frank - FW1A.1 Heuerman, Karl - HM2B.2 Hillyard, Patrick W. - FW3A.2 Hodges, Joseph T. - FT2A.2 Holland, Wayne - FT4A.3 Holzner, Simon - FM2A.1 Hook, Simon J. - HM4B.3 Hopwood, Rosalind - FT3A.5, JM3A.4,

JM3A.7, JM3A.8 Hosseini Aria, Seyed Enayat - HW3B.3 Howard, Grant J. - HM2B.1 Howett, Carly - FT3A.2 Huang, Xianglei - HW1B, JM1A, HT3B.3 Huang, You-Min - HW2B.2

Hulley, Glynn - HM4B.3 I

Iafolla, Valerio - FT4A.3 Ibrahim, Amir - HT3B.4 Ideguchi, Takuro - FM2A.1 Iler, Amber L. - HW2B.4 Imai, Tadashi - HM4B.2 Immel, Thomas - FM4A.1 Iraci, Laura - FW3A.2 Ishimaru, Ichirou - FM4A.2 Ivison, Rob - FT4A.3

J Jennings, Donald E. - FT3A.2, FT3A.3 Johnson, David G. - FT4A, HT4B.4 Johnson, Dean - FW4A.2 Johnson, William R. - HM4B.3 Jones, Martyn - FT4A.3 Juanola-Parramon, Roser - FT4A.3, FT4A.4,

FT4A.5, FT4A.6, JM3A.10, JM3A.3, JM3A.9

Judd, K Peter - HM4B.7

K Kataoka, Fumie - FW3A.2 Katoh, Eri - FW3A.2 Kawakami, Shuji - FW3A.2 Key, Richard - FW4A.2 Kindel, Bruce C. - HT3B.5 Knuteson, Robert O. - JM1A.2, FW3A.3 Ko, Cheng-Hao - HM4B.6, HW2B.2 Kopp, Greg - HM2B.2 Kratz, David - HT4B.4 Kruse, Fred A. - HW2B, HW3B.1 Kuze, Akihiko - FW3A.2, HM4B.2

L Lamborn, Andrew - FW4A.2 Lamprecht, Bret - HM2B.2 Lantagne, Stephane - FW2A.3, JM1A.2 Larar, Allen - HT3B.1 Last, Alan - JM3A.14 Latvakoski, Harri - HT4B.4 Latzko, Thomas - FW3A.4, FW3A.5 Le Coarer, Etienne - FM4A.4 Lee, Katherine - HM4B.7 Lee, John - HM2B Lefaivre, Adam - JM3A.8 Leisawitz, David T. - FT4A.3 Lightfoot, John - FT4A.3, FT4A.5, JM3A.9 Liu, Scige - FT4A.3 Liu, Yue X. - JM3A.12

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Liu, Xu - HT2B.1, HT4B.5, HT4B Lloyd, Nicholas - FW4A.5 Locke, Ann - HW2B.4 Long, David A. - FT2A.2 Longbotham, Nathan W. - HW3B.2 Loos, Joep - FW2A.1 Lu, Nanyao - FT3A.5, JM3A.4, JM3A.7 Lv, Bo Q. - JM3A.12

M Maillard, Jean-Pierre - FT3A.1 Makela, Jonathan - FM4A.1 Makiwa, Gibion - FT3A.5, JM3A.4, JM3A.8 Malitz, Seth - HW3B.2 Manatt, Kenneth S. - FW4A.2, FW4A.3 Mandard, Julie - FT3A.4 Marchili, Nicola - FT3A.5, JM3A.4, JM3A.7 Marr, Kenneth - FM4A.1, FM4A.3 Martin, Guillermo - FM4A.4 Martin, Jacob - HT4B.6 Mast, Jeffrey - HT4B.4 Matsuo, Hiroshi - FT4A.1, FT4A.3 McDowell, Meryl L. - HW3B.1 McKinney, Colin - FW4A.3 McMillan, Alison - FT4A.3 Menenti, Massimo - HW3B.3 Meola, Joseph - HT4B.2, HW3B Meshkaty, Nooshin - FW4A.3 Miller, Christopher - FM4A.6, HM4B.1 Miller, Ian - FM4A.3 Ming, Xing - JM3A.12 Mlynczak, Martin G. - HT4B.4 Monroe, Ryan M. - FW4A.3 Mooney, Dan - JM1A.1 Moore, James - FW4A.2 Moreau, Louis - FT3A.4, FW2A.3 Motteler, Howard - FW1A.3 Mouroulis, Pantazis - HM4B.5 Murakami, Kazutaka - FW3A.2 Murphy, J. A. - FT4A.3, FT4A.5 Murray, Jonathan - JM3A.14 Mushtaq, Sohail - JM3A.1

N Nastal, Jamie - FW4A.2 Naylor, David A. - FT3A.5, FT4A.2, FT4A.3,

FT4A.6, JM3A.4, JM3A.5, JM3A.6, JM3A.7, JM3A.8, FT3A

Neumann, Jonathan - HM2B.1, HM4B Neville, Timothy J. - FW4A.2 Newbury, Nathan - FM2A.2 Nichols, Jonathan - HM4B.7

O Olson, Colin - HM4B.7 O'Sullivan, Creidhe - FT4A.3, FT4A.5

P Pacifici, Fabio - HW3B.2 Palchetti, Luca - FW1A.2, FW3A.1, FW4A Pascale, Enzo - FT4A.3, FT4A.6 Pezzuto, Stefano - FT4A.3 Phillips, Coda - JM1A.2 Pickering, Juliet C. - JM3A.1, JM3A.14,

FT2A Picque, Nathalie - FM2A, FT2A.1 Pierce, Bradley - HT3B.1 Pilewskie, Peter - HM2B.2, HT3B.5

Pingree, Paula J. - FW4A.3 Plusquellic, David F. - FT2A.2 Podolske, James - FW3A.2 Polehampton, Edward - FT3A.5, JM3A.4,

JM3A.7, JM3A.8 Poutier, Laurent - FM4A.5 Predina, Joe - JM1A.1 Prel, Florent - FW2A.3 Preston, Daniel - FW4A.2 Primot, Jérôme - FM4A.5

R Rakotonimbahy, Eddy - FT4A.3 Revercomb, Henry E. - FW1A.3, FW3A.3,

JM3A.2, HT3B.1, JM1A.2, JT1A.1 Rhoby, Michael - FW2A.2 Rider, David M. - FW4A.2, FW4A.3 Rieker, Gregory - FM2A.2 Roberts, Carson - JM3A.16 Rommeluère, Sylvain - FM4A.4 Roosjen, Peter - JM3A.15 Rousset-Rouvière, Laurent - FM4A.5 Roy, Claude - FW2A.3, JM1A.2 Ryan, Matthew V. - FW4A.2, FW4A.3

S Sander, Stanley P. - FW4A.2, FW4A.3 Savini, Giorgio - FT4A.3, FT4A.4, FT4A.5,

FT4A.6, JM3A.10, JM3A.3, JM3A.9 Schaum, Alan - JT1A Schito, Daniele - FT4A.3 Schmitt, Bernard - FM4A.4 Scott, Jeremy - JM3A.8 Sharples, Ray M. - HM4B.4 Sheese, Patrick E. - FW1A.4 Shi, Sheng-Cai - FT4A.3 Shiomi, Kei - FW3A.2 Shusong, Du - JM3A.13 Simeoni, Denis - FW4A.1 Sinclair, Laura - FM2A.2 Smith, Nadia - HT3B.1 Smith, Paul - HM2B.2 Smith, William L. - HT3B.1, JM1A.2, JM3A.2 Solheim, Brian - FW4A.5 Spencer, John - FT3A.2 Spencer, Locke D. - FT4A.5, FT3A.5, FT4A.3, FT4A.6, JM3A.4, JM3A.8 Spinoglio, Luigi - FT4A.3 Stabbins, Roger - JM3A.10 Steers, Edward - JM3A.1 Stuhlmann, Rolf - HW1B.2 Suomalainen, Juha - JM3A.15 Suto, Hiroshi - FW3A.2, HM4B.2 Suwinski, Lawrence - JM1A.1 Swann, William - FM2A.2 Swinyard, Bruce - FT3A.5, FT4A.3, FT4A.6, JM3A.4

T Tanaka, Tomoaki - FW3A.2 Tang, Chia-Hui - HM4B.6 Taylor, Joe - FW1A.3, FW3A.3, JM3A.2, JM1A Theiler, James - JT1A.2 Thétas, Sophie - FM4A.5 Thibault, Simon - FT3A.4 Thomas, Fabrice - FM4A.4 Thome, Kurtis J. - HW1B.3

Ting, David - HM4B.3 Tjemkes, Stephen - HW1B.2 Tobin, David - FW1A.3, FW3A.3, JM3A.2 Toon, Geoffrey - FM4A, FW3A.6 Truong, Gar-Wing - FM2A.2 Tsai, Jih-Run - HM4B.6, HW2B.2 Turner, Joseph - HT3B.1

U Ungermann, Jörn - JM1A.3

V Valtchanov, Ivan - FT3A.5, JM3A.4, JM3A.7, JM3A.8 van der Wiel, Matthijs H. - FT3A.5, JM3A.8, JM3A.4 Veenendaal, Ian - FT4A.3, JM3A.6 Verret, Eric - JM1A.2 Vives, Sebastien - FT4A.3

W Wagner, Georg - FW2A.1 Walker, David - FT4A.3 Walker, Kaley A. - FW1A.4 Wang, Bang-Ji - HM4B.6, HW2B.2 Wang, Chenxi - HT4B.5 Wang, Jun - HT2B, HT3B.6 Weiss, Zdenek - JM3A.1 Weisz, Elisabeth - HT3B.1, JM3A.2 Werne, Thomas A. - FW4A.3 Wilson, Daniel W. - HM4B.3 Wincentsen, James - FW4A.2 Wu, Ronin - JM3A.4 Wu, Yen-Hung - FW4A.2 Xu, Feng - HT4B.3

Y Yang, Ping - HT4B.5 Yang, Qiguang - HT4B.5 Yesalusky, Melissa - HT3B.1 Yetzbacher, Michael - FM4A.6, HM4B.1, HM2B

Z Zaretski, Jeremy - JM3A.4, JM3A.7

Key to Authors and Presiders

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Fourier Transform Spectroscopy (FTS) and Hyperspectral Imaging … · 2015. 2. 12. · Hot Tub:...

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Transcript of Fourier Transform Spectroscopy (FTS) and Hyperspectral Imaging … · 2015. 2. 12. · Hot Tub:...