GNSS-RO Deep Refraction Signals from Moist Atmospheric ...

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GNSS-RO Deep Refraction Signals from Moist Atmospheric Boundary Layer Dong L. Wu 1 and Jie Gong 1,2 1) NASA Goddard Space Flight Center, Greenbelt, MD 2) GESTAR, Universities Space Research Association, Columbia, MD 8th IROWG Virtual Meeting April 7-9, 12 and 13, 2021 Acknowledgments: Support from NASA GNSS research program UCAR/CDAAC GNSS data service

Transcript of GNSS-RO Deep Refraction Signals from Moist Atmospheric ...

GNSS-RO Deep Refraction Signals from Moist Atmospheric Boundary Layer

Dong L. Wu1 and Jie Gong1,2

1) NASA Goddard Space Flight Center, Greenbelt, MD2) GESTAR, Universities Space Research Association, Columbia, MD

8th IROWG Virtual Meeting April 7-9, 12 and 13, 2021

Acknowledgments: • Support from NASA GNSS research program• UCAR/CDAAC GNSS data service

Ducting/Diffraction

LEOReceiver

GPS Transmit

ter No bending

Deep SNR

Straight-Line Height (HSL

)

Atmospheric Refraction, Ducting and Diffraction

This Study

(Image Credit: Wikipedia)

Atmospheric Optics: Fata Morgana

Stra

ight

-Lin

e H

eigh

t (H

SL),

km

Normalized SNR/SNR0

Deep RefractedRO Signals

in RO

Water Vapor Bending

Grazing Reflection

Super Refraction

Melbourne [2004]

U-Shape COSMIC-1

U-S

hap

e

“Throw-Back”

• Thin phase screen model for refractive + diffractive + multi-path RO signals

• Analytical calculation for a sharp 0.5-km atmospheric layer

• U-shape and deep-refraction SNR from ‘shadow zone’ filled by ‘throw-back’ rays

Deep SNR

DiffractiveSignals

Sokolovskiy et al. [2014] • Numerical wave-optics model simulations

• Longer duct => Deeper SNR

Analysis of RO SNR Data

SNR0

• Different σ in setting and rising RO• Different σ from GPS and GLONASS ROs with same receiver (e.g., COSMIC-2)• Similar σ in the same receiver set (e.g., COSMIC-1)• Use of the data with strong signals (SNR0 > 600): still many samples

Receiver noise (σ) effect

GPS

LEO1

Tangent HeightAbove Surface (H

t)

Straight-Line Height (H

SL)

LEO2

Impact Parameter (a)

LEO Orbit Height (H

sat)

Radio Occultation

Path

Earth Radius (R

e)

LEO altitude effect

Stra

ight

-Lin

e H

eigh

t (H

SL),

km

SNR/SNR0

Red: Tropics

Jan

Correlation between Deep (HSL

=-100km) SNR/SNR0 (COSMIC 2008-2011) and ERA5 950-hPa H2O and Refractivity over Ocean

Jul

Red: TropicsAt -100km

At -100km

Red: Tropics

Red: Tropics

H2O

H2O

Refractivity

Refractivity

Contours = ERA5 vertical velocity (w)

SNR/SNR0(x0.001)Jan July

Impacts of Vertical Motions and Terrain at HSL

=-100 km

SNR/SNR0(x0.001)

• Low SNR over terrain except flat forest lands (e.g., Amazon)

• Low SNR in the region of high w (e.g., ITCZ)

Sensitive to GNSS Signal Jamming

• Anomalous COSMIC-2 GPS signals at deep HSL

over the East Mediterranean and Turkey

• Slightly stronger in night than day

• Present in GPS but not in GLONASS signals

• Increased jamming on GPS signals since 2017, including the period of COVID-19 Pandemic

‘Hot Spots’ Reported by International Air Transport Association (IATA)

IATA (Nov, 2020)

• Major aviation safety concern

• 12-month study (Sep 2019 – Sep 2020)

• Based on pilot reports from cruise flights

• Insufficient flights for reporting due to COVID-19 Pandemic

Summary

• Deep refraction RO SNR signals were studied for the effects of refraction, ducting and diffraction in the lower troposphere.

• Strong correlation is found between deep SNR/SNR0 and marine ABL water vapor abundance.

• Algorithm for inferring marine ABL water vapor from RO SNR is under development.

• Deep RO SNR is sensitive to GNSS jamming, in which the jamming to GPS signals has significantly increased over the East Mediterranean since 2017.