Thermospheric Parameters during Ionospheric G-Conditions

For the first time thermospheric parameters (neutral composition, exospheric temperature and vertical plasma drift related to thermospheric winds) have been inferred for ionospheric G-conditions observed with Millstone Hill ISR on 11–13 September 2005; 13 June 2005, and 15 July 2012. The earlier dev...

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Main Authors: Loredana Perrone, Andrey V. Mikhailov, Dario Sabbagh
Format: Article
Language:English
Published: MDPI AG 2021-08-01
Series:Remote Sensing
Subjects:
Online Access:https://www.mdpi.com/2072-4292/13/17/3440
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spelling doaj-77406a14973147128e6b95d88daead542021-09-09T13:55:21ZengMDPI AGRemote Sensing2072-42922021-08-01133440344010.3390/rs13173440Thermospheric Parameters during Ionospheric G-ConditionsLoredana Perrone0Andrey V. Mikhailov1Dario Sabbagh2Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, 00143 Rome, ItalyIstituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, 00143 Rome, ItalyIstituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, 00143 Rome, ItalyFor the first time thermospheric parameters (neutral composition, exospheric temperature and vertical plasma drift related to thermospheric winds) have been inferred for ionospheric G-conditions observed with Millstone Hill ISR on 11–13 September 2005; 13 June 2005, and 15 July 2012. The earlier developed method to extract a consistent set of thermospheric parameters from ionospheric observations has been revised to solve the problem in question. In particular CHAMP/STAR and GOCE neutral gas density observations were included into the retrieval process. It was found that G-condition days were distinguished by enhanced exospheric temperature and decreased by ~2 times of the column atomic oxygen abundance in a comparison to quiet reference days, the molecular nitrogen column abundance being practically unchanged. The inferred upward plasma drift corresponds to strong ~90 m/s equatorward thermospheric wind presumably related to strong auroral heating on G-condition days.https://www.mdpi.com/2072-4292/13/17/3440ionospheric G-conditionthermospheric parametersionosondeIncoherent Scatter Radar (ISR)CHAMPGOCE satellite
collection DOAJ
language English
format Article
sources DOAJ
author Loredana Perrone
Andrey V. Mikhailov
Dario Sabbagh
spellingShingle Loredana Perrone
Andrey V. Mikhailov
Dario Sabbagh
Thermospheric Parameters during Ionospheric G-Conditions
Remote Sensing
ionospheric G-condition
thermospheric parameters
ionosonde
Incoherent Scatter Radar (ISR)
CHAMP
GOCE satellite
author_facet Loredana Perrone
Andrey V. Mikhailov
Dario Sabbagh
author_sort Loredana Perrone
title Thermospheric Parameters during Ionospheric G-Conditions
title_short Thermospheric Parameters during Ionospheric G-Conditions
title_full Thermospheric Parameters during Ionospheric G-Conditions
title_fullStr Thermospheric Parameters during Ionospheric G-Conditions
title_full_unstemmed Thermospheric Parameters during Ionospheric G-Conditions
title_sort thermospheric parameters during ionospheric g-conditions
publisher MDPI AG
series Remote Sensing
issn 2072-4292
publishDate 2021-08-01
description For the first time thermospheric parameters (neutral composition, exospheric temperature and vertical plasma drift related to thermospheric winds) have been inferred for ionospheric G-conditions observed with Millstone Hill ISR on 11–13 September 2005; 13 June 2005, and 15 July 2012. The earlier developed method to extract a consistent set of thermospheric parameters from ionospheric observations has been revised to solve the problem in question. In particular CHAMP/STAR and GOCE neutral gas density observations were included into the retrieval process. It was found that G-condition days were distinguished by enhanced exospheric temperature and decreased by ~2 times of the column atomic oxygen abundance in a comparison to quiet reference days, the molecular nitrogen column abundance being practically unchanged. The inferred upward plasma drift corresponds to strong ~90 m/s equatorward thermospheric wind presumably related to strong auroral heating on G-condition days.
topic ionospheric G-condition
thermospheric parameters
ionosonde
Incoherent Scatter Radar (ISR)
CHAMP
GOCE satellite
url https://www.mdpi.com/2072-4292/13/17/3440
work_keys_str_mv AT loredanaperrone thermosphericparametersduringionosphericgconditions
AT andreyvmikhailov thermosphericparametersduringionosphericgconditions
AT dariosabbagh thermosphericparametersduringionosphericgconditions
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