Auroral Ionospheric Irregularity Properties via Estimation and Inverse Modeling of GNSS Scintillations

Seebany Datta-Barua; Kshitija B. Deshpande; Donald Hampton; Gary S. Bust

doi:10.23919/URSIAP-RASC.2019.8738665

Auroral Ionospheric Irregularity Properties via Estimation and Inverse Modeling of GNSS Scintillations

Seebany Datta-Barua
, Kshitija B. Deshpande
, Donald Hampton
, Gary S. Bust

Illinois Institute of Technology
Embry-Riddle Aeronautical University
University of Alaska Fairbanks
Johns Hopkins University Applied Physics Laboratory

Research output: Contribution to journal › Article › peer-review

Original language	American English
Journal	URSI Asia-Pacific Radio Science Conference
DOIs	https://doi.org/10.23919/URSIAP-RASC.2019.8738665
State	Published - Mar 9 2019
Externally published	Yes

Disciplines

Physics
Remote Sensing

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10.23919/URSIAP-RASC.2019.8738665License: Unspecified

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@article{4d776aa87ed24c8caf126d8193b19dd9,

title = "Auroral Ionospheric Irregularity Properties via Estimation and Inverse Modeling of GNSS Scintillations",

author = "Seebany Datta-Barua and Deshpande, \{Kshitija B.\} and Donald Hampton and Bust, \{Gary S.\}",

note = "When Global Navigation Satellite System (GNSS) signals traverse the ionosphere, variations in plasma density cause the received signal at the ground to scintillate, i.e., exhibit a rapid fluctuation in power and/or phase. Scintillation at high latitudes near the auroral zone can be frequent, and are typically observed, with standard GNSS receiver processing, as phase scintillations.",

year = "2019",

month = mar,

day = "9",

doi = "10.23919/URSIAP-RASC.2019.8738665",

language = "American English",

journal = "URSI Asia-Pacific Radio Science Conference",

issn = "2768-2129",

}

TY - JOUR

T1 - Auroral Ionospheric Irregularity Properties via Estimation and Inverse Modeling of GNSS Scintillations

AU - Datta-Barua, Seebany

AU - Deshpande, Kshitija B.

AU - Hampton, Donald

AU - Bust, Gary S.

N1 - When Global Navigation Satellite System (GNSS) signals traverse the ionosphere, variations in plasma density cause the received signal at the ground to scintillate, i.e., exhibit a rapid fluctuation in power and/or phase. Scintillation at high latitudes near the auroral zone can be frequent, and are typically observed, with standard GNSS receiver processing, as phase scintillations.

PY - 2019/3/9

Y1 - 2019/3/9

UR - https://ieeexplore.ieee.org/document/8738665/

U2 - 10.23919/URSIAP-RASC.2019.8738665

DO - 10.23919/URSIAP-RASC.2019.8738665

M3 - Article

SN - 2768-2129

JO - URSI Asia-Pacific Radio Science Conference

JF - URSI Asia-Pacific Radio Science Conference

ER -

Auroral Ionospheric Irregularity Properties via Estimation and Inverse Modeling of GNSS Scintillations

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