Difference spectrum fitting of the ion-neutral collision frequency from dual-frequency EISCAT measurements

The plasma–neutral coupling in the mesosphere–lower thermosphere strongly depends on the ion–neutral collision frequency across that region. Most commonly, the collision frequency profile is calculated from the climatologies of atmospheric models. However, previous measurements indicated that the co...

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Main Authors: Günzkofer, Florian, Stober, Gunter, Pokhotelov, Dimitry, Miyoshi, Yasunobu, Borries, Claudia
Format: Text
Language:English
Published: 2023
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2023-1495
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1495/
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spelling ftcopernicus:oai:publications.copernicus.org:egusphere112989 2024-01-07T09:42:59+01:00 Difference spectrum fitting of the ion-neutral collision frequency from dual-frequency EISCAT measurements Günzkofer, Florian Stober, Gunter Pokhotelov, Dimitry Miyoshi, Yasunobu Borries, Claudia 2023-12-08 application/pdf https://doi.org/10.5194/egusphere-2023-1495 https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1495/ eng eng doi:10.5194/egusphere-2023-1495 https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1495/ eISSN: Text 2023 ftcopernicus https://doi.org/10.5194/egusphere-2023-1495 2023-12-11T17:24:19Z The plasma–neutral coupling in the mesosphere–lower thermosphere strongly depends on the ion–neutral collision frequency across that region. Most commonly, the collision frequency profile is calculated from the climatologies of atmospheric models. However, previous measurements indicated that the collision frequency can deviate notably from the climatological average. Direct measurement of the ion–neutral collision frequency with multifrequency incoherent scatter radar (ISR) measurements has been discussed before, though actual measurements have been rare. The previously applied multifrequency analysis method requires a special simultaneous fit of the two incoherent scatter spectra, which is not possible with standard ISR analysis software. The difference spectrum method allows us to infer ion–neutral collision frequency profiles from multifrequency ISR measurements based on standard incoherent scatter analysis software, such as the Grand Unified Incoherent Scatter Design and Analysis Package (GUISDAP) software. In this work, we present the first results by applying the difference spectrum method. Ion–neutral collision frequency profiles obtained from several multifrequency EISCAT ISR campaigns are presented. The profiles obtained with the difference spectrum method are compared to previous collision frequency measurements, both from multifrequency ISR and other measurements, as well as results from empirical and comprehensive atmosphere models. Ion–neutral collision frequency measurements can be applied to improve first-principle ionospheric models. Text EISCAT Copernicus Publications: E-Journals
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description The plasma–neutral coupling in the mesosphere–lower thermosphere strongly depends on the ion–neutral collision frequency across that region. Most commonly, the collision frequency profile is calculated from the climatologies of atmospheric models. However, previous measurements indicated that the collision frequency can deviate notably from the climatological average. Direct measurement of the ion–neutral collision frequency with multifrequency incoherent scatter radar (ISR) measurements has been discussed before, though actual measurements have been rare. The previously applied multifrequency analysis method requires a special simultaneous fit of the two incoherent scatter spectra, which is not possible with standard ISR analysis software. The difference spectrum method allows us to infer ion–neutral collision frequency profiles from multifrequency ISR measurements based on standard incoherent scatter analysis software, such as the Grand Unified Incoherent Scatter Design and Analysis Package (GUISDAP) software. In this work, we present the first results by applying the difference spectrum method. Ion–neutral collision frequency profiles obtained from several multifrequency EISCAT ISR campaigns are presented. The profiles obtained with the difference spectrum method are compared to previous collision frequency measurements, both from multifrequency ISR and other measurements, as well as results from empirical and comprehensive atmosphere models. Ion–neutral collision frequency measurements can be applied to improve first-principle ionospheric models.
format Text
author Günzkofer, Florian
Stober, Gunter
Pokhotelov, Dimitry
Miyoshi, Yasunobu
Borries, Claudia
spellingShingle Günzkofer, Florian
Stober, Gunter
Pokhotelov, Dimitry
Miyoshi, Yasunobu
Borries, Claudia
Difference spectrum fitting of the ion-neutral collision frequency from dual-frequency EISCAT measurements
author_facet Günzkofer, Florian
Stober, Gunter
Pokhotelov, Dimitry
Miyoshi, Yasunobu
Borries, Claudia
author_sort Günzkofer, Florian
title Difference spectrum fitting of the ion-neutral collision frequency from dual-frequency EISCAT measurements
title_short Difference spectrum fitting of the ion-neutral collision frequency from dual-frequency EISCAT measurements
title_full Difference spectrum fitting of the ion-neutral collision frequency from dual-frequency EISCAT measurements
title_fullStr Difference spectrum fitting of the ion-neutral collision frequency from dual-frequency EISCAT measurements
title_full_unstemmed Difference spectrum fitting of the ion-neutral collision frequency from dual-frequency EISCAT measurements
title_sort difference spectrum fitting of the ion-neutral collision frequency from dual-frequency eiscat measurements
publishDate 2023
url https://doi.org/10.5194/egusphere-2023-1495
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1495/
genre EISCAT
genre_facet EISCAT
op_source eISSN:
op_relation doi:10.5194/egusphere-2023-1495
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1495/
op_doi https://doi.org/10.5194/egusphere-2023-1495
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