The Storm-Time Assessment of GNSS-SBAS Performance...

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The Storm-Time Assessment of GNSS-SBAS Performance within African Equatorial and Low Latitude Region O. E. Abe 1, 2 , C. Paparini 1 , R. H. Ngaya 1 , X. Otero Villamide 1 , S. M. Radicella 1 , and B. Nava 1 1 Abdus Salam International Centre for Theoretical Physics (ICTP), Trieste, Italy 2 Department of Physics, Federal University Oye-Ekiti, Ekiti State, Nigeria IONOSPHERIC EFFECTS SYMPOSIUM (IES) Alexandria, VA, 12-14 May 2015

Transcript of The Storm-Time Assessment of GNSS-SBAS Performance...

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The Storm-Time Assessment of GNSS-SBAS Performance within African Equatorial and Low

Latitude Region

O. E. Abe1, 2, C. Paparini1, R. H. Ngaya1, X. Otero Villamide1, S. M. Radicella1, and B. Nava1

1Abdus Salam International Centre for Theoretical Physics (ICTP), Trieste, Italy 2Department of Physics, Federal University Oye-Ekiti, Ekiti State, Nigeria

IONOSPHERIC EFFECTS SYMPOSIUM (IES)

Alexandria, VA, 12-14 May 2015

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Outline

Introduction Data Analysis Results and Discussion Summary Acknowledgements

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Introduction Storm-time refers to the period of increased

geomagnetic activity that influences the space environment.

it is an interaction of the sun’s magnetic field (solar

wind), interplanetary magnetic field and Earth’s magnetic field (magnetosphere).

This affects the ionospheric-thermospheric system and influence the performance and reliability of space-based and ground-based technological systems as well endanger human life.

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4

The specific condition of African Equatorial and Low Latitude Region

From ICAO: IONOSPHERIC EFFECT ON GNSS AVIATION OPERATIONS, First Meeting of Ionospheric Studies Task Force, Tokyo, February 2012

“For APV [Approach Procedures with Vertical Guidance] operations, ionospheric delay

corrections and associated integrity bounds must be obtained from a SBAS. SBAS is capable of broadcasting ionospheric integrity bounds that are sufficiently small to ensure a high availability of APV service in mid- and high-latitude regions However, the availability of APV service may be reduced or even severely limited in relatively rare occasions (roughly 1% of the time) due to disturbances caused by a severe ionospheric storm. APV service is also conceptually possible in low-latitude regions; however, the variability and unique phenomena of the equatorial ionosphere present a very difficult challenge to ensuring the integrity of the ionospheric corrections without causing frequent interruptions of APV service (i.e., frequent, and perhaps even daily, interruptions of service in the local evening hours during years near the peak of the solar cycle)” .

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Characteristics of Ionosphere over Low Latitudes

Low latitudes is considered here within the range of ± 25o magnetic latitudes or modip.

It shows two peaks of electron density and total electron content around ± 20o and a trough along the geomagnetic equator.

It is more complex to model than mid-latitude ionosphere.

Highly variable with time.

It causes more delay on L band frequency because of the high values of TEC.

It becomes highly irregular after sunset.

The irregularities produce large fluctuations in L band signals.

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Data Analysis • The data used were obtained from openly-

available GNSS receiver stations within the Northern and Southern crest of the African Equatorial Ionization Anomaly (EIA) region, for the month of July and October 2013.

• The stations were divided into two groups based on their local time.

• SBAS APV-1 availability maps were obtained using a SBAS emulator (magicSBAS platform) with a specific low-latitude algorithm developed by GMV and acquired by ICTP for TREGA project.

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Overview of GNSS stations in Africa

08/04/2015 European Navigation Conference, Bordeaux

ouag

cggn

unecy kro

nklg

bkf p

nurk rcmnmal2

adis

Sey 1

moiumbar

mzuz

sthl

dodm

FG07

MTWA

Arit

lnda

tezi

ADD

ASI

BHD

CVD

HEL

KAMKIS

abpo

ABUZ

acra

agui

alx2

bjab

bjka

bjco

bjnabjnibjsa

CLBR

dakr

f g06

f g08

f g42

f unc

FUTY

harb

hnus

HUKP

lamp

lpal

maua

mazo

MTND

OSFG

rabt

reun

sf er

tela

tias

v acs

wind

zamb

znzb

mas1

dragramo

dear

mf kg

sbok

suthsutmsutv

tdou

tetn

uldi

if r1dear bshm

graf

if r1

maun

bjpa

30° W 0° 30° E 60° E

30° S

30° N

7

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TREGA scenario

08/04/2015 European Navigation Conference, Bordeaux

ouagcggn

unecykro

bkfp

bjco

20° W 10° W 0° 10° E 20° E 0°

10° N

20° N

dakr

nklgfg07

futy

ID Location Geo. Lat (oN)

Geo. Lon (oE)

Modip (o)

Groups

cggn Toro (Nigeria)

10.12 9.12 -1.96 B

ouag Ouagadougou (Burkina Faso)

12.35 -1.51 2.86 A

futy Yola (Nigeria)

9.35 12.50 -3.34 B

bkfp Kebbi (Nigeria)

12.47 4.23 3.50 B

ykro Yamoussoukro (Cote d’Ivorie)

6.87 -5.24 -10.63 A

unec Enugu (Nigeria)

6.42 7.51 -10.89 B

bjco Cotonou (Benin)

6.23 2.27 -11.83 B

dakr Dakar (Senegal)

14.75 -17.49 11.86 A

nklg Libreville (Gabon)

0.35 9.67 -23.90 B

fg07 Sao-Tome (Soa-Tome)

0.34 6.73 -24.60 A

8

Main drivers:

• Spatial gaps

•Temporal gaps

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ROTI and DvTEC Estimation • Rate of change of TEC (ROT) is defined as:

𝑅𝑅𝑅𝑅𝑅𝑅 =𝑅𝑅𝑇𝑇𝑇𝑇𝑘𝑘

𝑖𝑖 − 𝑅𝑅𝑇𝑇𝑇𝑇𝑘𝑘−1𝑖𝑖

𝑡𝑡𝑘𝑘 − 𝑡𝑡𝑘𝑘−1

it is computed: along the line of sight from satellite to receiver; and for each 1 min interval ROTI is defined as the standard deviation of ROT for 5 min interval:

𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅 = < 𝑅𝑅𝑅𝑅𝑅𝑅2 > −< 𝑅𝑅𝑅𝑅𝑅𝑅 >2 where i is the visible satellite and k is the time of epoch, TEC is the total electron content, ROT is the rate of change of TEC and ROTI is the change of change of TEC index • Percentage of the relative deviation of the vertical TEC (DvTEC)

from the quiet reference level for each station was calculated

𝐷𝐷𝐷𝐷𝑅𝑅𝑇𝑇𝑇𝑇 =𝐷𝐷𝑅𝑅𝑇𝑇𝑇𝑇𝑑𝑑 − 𝐷𝐷𝑅𝑅𝑇𝑇𝑇𝑇𝑞𝑞

𝐷𝐷𝑅𝑅𝑇𝑇𝑇𝑇𝑞𝑞 × 100

where DvTEC is the relative percentage deviation of vertical TEC from the reference level, vTECq is the reference level (monthly mean of vTEC for the most 10 quietest days of the month of the storm), vTECd is the vTEC of the disturbed day.

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Results and Discussion

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Toro (Nigeria)

Yola (Nigeria)

Kebbi (Nigeria)

Enugu (Nigeria)

Cotonou (Benin)

Libreville (Gabon)

05-July 2013 06-July 2013 07-July 2013

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Toro (Nigeria)

Yola (Nigeria)

Kebbi (Nigeria)

Enugu (Nigeria)

Cotonou (Benin)

Libreville (Gabon)

Group A

Group B

Transient Variations of Dst (red), DvTEC (blue) and ROTI (green) indicating Ionospheric irregularities inhibition for 6th July 2013

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July 5

July 7

July 6

SBAS APV-1 availability maps indicating enhancements in SBAS performance for July 6th

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Transient Variations of Dst (red), DvTEC (blue) and ROTI (green) indicating Ionospheric irregularities enhancements

for 10th July 2013

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Ouagadougou (Burkina Faso)

Yamoussoukro (Cote d’Ivorie)

Dakar (Senegal)

Sao-Tome (Soa-Tome)

09-July 2013 10-July 2013 11-July 2013

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Toro (Nigeria)

Yola (Nigeria)

Kebbi (Nigeria)

Enugu (Nigeria)

Cotonou (Benin)

Libreville (Gabon)

01-July 2013 10-July 2013 11-July 20130

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Toro (Nigeria)

Yola (Nigeria)

Kebbi (Nigeria)

Enugu (Nigeria)

Cotonou (Benin)

Libreville (Gabon)

Group A

Group B

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July 9

July 11

July 10

SBAS APV-1 availability maps indicating degradations in SBAS performance for July 10th

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Transient Variations of Dst (red), DvTEC (blue) and ROTI (green) indicating usual Ionospheric irregularities

for 2nd October 2013

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03-Octber 201302-Octber 201301-Octber 2013

Ouagadougou (Burkina Faso)

Yamoussoukro (Cote d’Ivorie)

Dakar (Senegal)

Sao-Tome (Soa-Tome)

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Enugu (Nigeria)

Cotonou (Benin)

Libreville (Gabon)

Yola (Nigeria)

Toro (Nigeria) 0

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Toro (Nigeria)

Yola (Nigeria)

Enugu (Nigeria)

Cotonou (Benin)

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Group B

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October 1

October 3

October 2

SBAS APV-1 availability maps indicating usual operation in SBAS performance for October 2nd

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Transient Variations of Dst (red), DvTEC (blue) and ROTI (green) indicating increased in Ionospheric irregularities

for 9th October 2013

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10-October 2013

Ouagadougou (Burkina Faso)

Yamoussoukro (Cote d'Ivorie)

Dakar (Senegal)

Sao-Tome (Sao-Tome)

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Yola (Nigeria)

Toro (Nigeria)

Enugu (Nigeria)

Cotonou (Benin)

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October 8

October 10

October 9

SBAS APV-1 availability maps indicating degradation in SBAS performance for October 9th

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Transient Variations of Dst (red), DvTEC (blue) and ROTI (green) indicating inhibition in Ionospheric irregularities

for 14th October 2013

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Enugu (Nigeria)

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Toro (Nigeria)

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Yola (Nigeria)

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Enugu (Nigeria)

Kebbi (Nigeria)

Group A

Group B

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October 13

October 15

October 14

SBAS APV-1 availability maps indicating enhancements in SBAS performance for October 14th

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Transient Variations of Dst (red), DvTEC (blue) and ROTI (green) indicating inhibition/reduction in Ionospheric

irregularities for 30th October 2013

Group A

Group B

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-1000

100200300

01:00 07:00 13:00 19:00 01:00 07:00 13:00 19:00 01:00 07:00 13:00 19:00 01:00-100

0100200300

LT (hrs)

Toro (Nigeria)

Yola (Nigeria)

Kebbi (Nigeria)

Enugu (Nigeria)

Cotonou (Benin)

Libreville (Gabon)

30-Octber 2013 31-Octber 201329-Octber 2013 0

0.5

1

LT (hrs)

0

0.5

1

LT (hrs)

0

0.5

1

RO

TI(T

EC

u/m

in)

LT (hrs)

0

0.5

1

RO

TI(T

EC

u/m

in)

LT (hrs)

0

0.5

1

LT (hrs)

01:00 07:00 13:00 19:00 01:00 07:00 13:00 19:00 01:00 07:00 13:00 19:00 01:000

0.5

1

LT (hrs)

Toro (Nigeria)

Yola (Nigeria)

Kebbi (Nigeria)

Enugu (Nigeria)

Cotonou (Benin)

Libreville (Gabon)

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SBAS APV-1 availability maps indicating enhancements in SBAS performance for October 30th

October 29

October 31

October 31

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Summary • This study assessed the effect of the ionosphere at African

low-latitudes on SBAS system performance using real GNSS data stations from African equatorial latitudes during increased in Geomagnetic activity.

• Both positive and negative phases of the storm are observed; though positive phases are more frequent than negative.

• These effects modify the morphology and the physics of the ionosphere at post sunset to post mid-night periods leading to inhibition or increase of ionospheric irregularities.

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• The SBAS system behaviour during an increased geomagnetic activity cannot be based only to geomagnetic indices and depends on specific conditions that influence the occurrence of ionospheric irregularities

• The present study reveals that ROTI is a good proxy to indicate such occurrence also during geomagnetic disturbed conditions.

• During the storm-time conditions considered, three out of seven geomagnetic storm induced enhancement to SBAS system performance, three reduced the system performance while one does not have effect on SBAS system performance in corresponded to ROTI values.

• ROTI is a representative index of SBAS performance: it indicates enhancements in the system performance when there is inhibition of usual ionospheric irregularities activity and degradations in system performance when there is increase of irregularities activity.

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Acknowledgements

This presentation contains results obtained during the “training through research" activities of the TREGA Project financed by the European Union under the Contribution Agreement between the European Commission and the ICTP.

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Thanks for your attention