Loading…
Relation of internal gravity wave anisotropy with neutral wind characteristics in the upper atmosphere
This paper studies the interaction of internal gravity waves (IGW) with neutral wind using the statistics of traveling ionospheric disturbances (TID) from the Radio Physical Complex of the Institute of Solar‐Terrestrial Physics. The complex includes the Irkutsk Incoherent Scatter Radar (IISR), Irkut...
Saved in:
Published in: | Journal of geophysical research. Space physics 2017-07, Vol.122 (7), p.7567-7580 |
---|---|
Main Authors: | , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | cdi_FETCH-LOGICAL-c3073-ed8f4499499223b978a9b82cad8243772fc057ef63baa6c897711f00414506213 |
---|---|
cites | cdi_FETCH-LOGICAL-c3073-ed8f4499499223b978a9b82cad8243772fc057ef63baa6c897711f00414506213 |
container_end_page | 7580 |
container_issue | 7 |
container_start_page | 7567 |
container_title | Journal of geophysical research. Space physics |
container_volume | 122 |
creator | Medvedev, А. V. Ratovsky, K. G. Tolstikov, M. V. Oinats, A. V. Alsatkin, S. S. Zherebtsov, G. A. |
description | This paper studies the interaction of internal gravity waves (IGW) with neutral wind using the statistics of traveling ionospheric disturbances (TID) from the Radio Physical Complex of the Institute of Solar‐Terrestrial Physics. The complex includes the Irkutsk Incoherent Scatter Radar (IISR), Irkutsk Ionosonde (DPS‐4), and Ekaterinburg HF Radar (EKB). The aim of this study is to give a common explanation for the TID azimuth distributions obtained with the IISR‐ionosonde and HF coherent radar and show that the measurements of 3‐D TID characteristics put into the hands of researchers an important tool to study neutral wind in the thermosphere. The distinctive features of this study are the following: (1) using different TID statistics from independent tools and, correspondingly, independent methods for determining TID characteristics; (2) using the 3‐D TID characteristics for testing the wind‐filtering hypothesis, which allows us to separate the IGW‐induced TIDs from TIDs of other nature and identify three TID types depending on their elevation angles; and (3) using the local time‐azimuth distribution of the TID number for testing the wind‐filtering hypothesis. This study allowed us to conclude that the observed IGW azimuth anisotropy can be mainly explained by the wind filtration mechanism with considering winds at 90–250 km heights. Using the 3‐D IGW characteristics allows us to estimate neutral wind parameters. Proposed methods are applicable for any tool which can obtain TID 3‐D characteristics. Using the proposed methods will enable us to organize a worldwide campaign to improve the existing neutral wind models.
Key Points
At least 60% of observed TID induced by IGW; TID LT‐azimuth distributions can be mainly explained by the wind filtration mechanism
There are differences between azimuth distributions of three TID types (source below, source above, and reflected)
Methods of neutral wind estimating were proposed |
doi_str_mv | 10.1002/2017JA024103 |
format | article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_1928082239</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1928082239</sourcerecordid><originalsourceid>FETCH-LOGICAL-c3073-ed8f4499499223b978a9b82cad8243772fc057ef63baa6c897711f00414506213</originalsourceid><addsrcrecordid>eNp9kE1LAzEQhoMoWGpv_oCAV1cnyX4kx1K0WgpC0fOSpombst2sSbal_96UKnhyGJgPnnlhXoRuCTwQAPpIgVSLKdCcALtAI0pKkYkc6OVvzzhco0kIW0jB04oUI2RWupXRug47g20Xte9kiz-93Nt4xAe511h2NrjoXZ9mGxvc6SH6BB1st8GqkV6qdGZDtCokCRwbjYe-1x7LuHOhb7TXN-jKyDboyU8do4_np_fZS7Z8m7_OpstMMahYpjfc5LkQKSlla1FxKdacKrnhNGdVRY2CotKmZGspS8VFVRFiAHKSF1BSwsbo7qzbe_c16BDrrRtOL4WaCMqBJ1mRqPszpbwLwWtT997upD_WBOqTmfVfMxPOzvjBtvr4L1sv5qtpwUrG2DdrqXVf</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1928082239</pqid></control><display><type>article</type><title>Relation of internal gravity wave anisotropy with neutral wind characteristics in the upper atmosphere</title><source>Wiley-Blackwell Read & Publish Collection</source><creator>Medvedev, А. V. ; Ratovsky, K. G. ; Tolstikov, M. V. ; Oinats, A. V. ; Alsatkin, S. S. ; Zherebtsov, G. A.</creator><creatorcontrib>Medvedev, А. V. ; Ratovsky, K. G. ; Tolstikov, M. V. ; Oinats, A. V. ; Alsatkin, S. S. ; Zherebtsov, G. A.</creatorcontrib><description>This paper studies the interaction of internal gravity waves (IGW) with neutral wind using the statistics of traveling ionospheric disturbances (TID) from the Radio Physical Complex of the Institute of Solar‐Terrestrial Physics. The complex includes the Irkutsk Incoherent Scatter Radar (IISR), Irkutsk Ionosonde (DPS‐4), and Ekaterinburg HF Radar (EKB). The aim of this study is to give a common explanation for the TID azimuth distributions obtained with the IISR‐ionosonde and HF coherent radar and show that the measurements of 3‐D TID characteristics put into the hands of researchers an important tool to study neutral wind in the thermosphere. The distinctive features of this study are the following: (1) using different TID statistics from independent tools and, correspondingly, independent methods for determining TID characteristics; (2) using the 3‐D TID characteristics for testing the wind‐filtering hypothesis, which allows us to separate the IGW‐induced TIDs from TIDs of other nature and identify three TID types depending on their elevation angles; and (3) using the local time‐azimuth distribution of the TID number for testing the wind‐filtering hypothesis. This study allowed us to conclude that the observed IGW azimuth anisotropy can be mainly explained by the wind filtration mechanism with considering winds at 90–250 km heights. Using the 3‐D IGW characteristics allows us to estimate neutral wind parameters. Proposed methods are applicable for any tool which can obtain TID 3‐D characteristics. Using the proposed methods will enable us to organize a worldwide campaign to improve the existing neutral wind models.
Key Points
At least 60% of observed TID induced by IGW; TID LT‐azimuth distributions can be mainly explained by the wind filtration mechanism
There are differences between azimuth distributions of three TID types (source below, source above, and reflected)
Methods of neutral wind estimating were proposed</description><identifier>ISSN: 2169-9380</identifier><identifier>EISSN: 2169-9402</identifier><identifier>DOI: 10.1002/2017JA024103</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Anisotropy ; Atmospheric models ; Azimuth ; Coherent radar ; Filtration ; Gravitational waves ; Gravity waves ; HF radar ; Hypotheses ; Incoherent scatter radar ; internal gravitational waves ; Internal gravity waves ; Internal waves ; Ionospheric disturbances ; ionsphere ; neutral wind ; Parameter estimation ; Radar ; Thermosphere ; Traveling ionospheric disturbances ; Upper atmosphere ; wave‐wind interaction ; Wind ; Wind models</subject><ispartof>Journal of geophysical research. Space physics, 2017-07, Vol.122 (7), p.7567-7580</ispartof><rights>2017. American Geophysical Union. All Rights Reserved.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c3073-ed8f4499499223b978a9b82cad8243772fc057ef63baa6c897711f00414506213</citedby><cites>FETCH-LOGICAL-c3073-ed8f4499499223b978a9b82cad8243772fc057ef63baa6c897711f00414506213</cites><orcidid>0000-0002-0847-3553 ; 0000-0002-9176-5425 ; 0000-0002-1120-870X ; 0000-0003-0660-8474</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Medvedev, А. V.</creatorcontrib><creatorcontrib>Ratovsky, K. G.</creatorcontrib><creatorcontrib>Tolstikov, M. V.</creatorcontrib><creatorcontrib>Oinats, A. V.</creatorcontrib><creatorcontrib>Alsatkin, S. S.</creatorcontrib><creatorcontrib>Zherebtsov, G. A.</creatorcontrib><title>Relation of internal gravity wave anisotropy with neutral wind characteristics in the upper atmosphere</title><title>Journal of geophysical research. Space physics</title><description>This paper studies the interaction of internal gravity waves (IGW) with neutral wind using the statistics of traveling ionospheric disturbances (TID) from the Radio Physical Complex of the Institute of Solar‐Terrestrial Physics. The complex includes the Irkutsk Incoherent Scatter Radar (IISR), Irkutsk Ionosonde (DPS‐4), and Ekaterinburg HF Radar (EKB). The aim of this study is to give a common explanation for the TID azimuth distributions obtained with the IISR‐ionosonde and HF coherent radar and show that the measurements of 3‐D TID characteristics put into the hands of researchers an important tool to study neutral wind in the thermosphere. The distinctive features of this study are the following: (1) using different TID statistics from independent tools and, correspondingly, independent methods for determining TID characteristics; (2) using the 3‐D TID characteristics for testing the wind‐filtering hypothesis, which allows us to separate the IGW‐induced TIDs from TIDs of other nature and identify three TID types depending on their elevation angles; and (3) using the local time‐azimuth distribution of the TID number for testing the wind‐filtering hypothesis. This study allowed us to conclude that the observed IGW azimuth anisotropy can be mainly explained by the wind filtration mechanism with considering winds at 90–250 km heights. Using the 3‐D IGW characteristics allows us to estimate neutral wind parameters. Proposed methods are applicable for any tool which can obtain TID 3‐D characteristics. Using the proposed methods will enable us to organize a worldwide campaign to improve the existing neutral wind models.
Key Points
At least 60% of observed TID induced by IGW; TID LT‐azimuth distributions can be mainly explained by the wind filtration mechanism
There are differences between azimuth distributions of three TID types (source below, source above, and reflected)
Methods of neutral wind estimating were proposed</description><subject>Anisotropy</subject><subject>Atmospheric models</subject><subject>Azimuth</subject><subject>Coherent radar</subject><subject>Filtration</subject><subject>Gravitational waves</subject><subject>Gravity waves</subject><subject>HF radar</subject><subject>Hypotheses</subject><subject>Incoherent scatter radar</subject><subject>internal gravitational waves</subject><subject>Internal gravity waves</subject><subject>Internal waves</subject><subject>Ionospheric disturbances</subject><subject>ionsphere</subject><subject>neutral wind</subject><subject>Parameter estimation</subject><subject>Radar</subject><subject>Thermosphere</subject><subject>Traveling ionospheric disturbances</subject><subject>Upper atmosphere</subject><subject>wave‐wind interaction</subject><subject>Wind</subject><subject>Wind models</subject><issn>2169-9380</issn><issn>2169-9402</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp9kE1LAzEQhoMoWGpv_oCAV1cnyX4kx1K0WgpC0fOSpombst2sSbal_96UKnhyGJgPnnlhXoRuCTwQAPpIgVSLKdCcALtAI0pKkYkc6OVvzzhco0kIW0jB04oUI2RWupXRug47g20Xte9kiz-93Nt4xAe511h2NrjoXZ9mGxvc6SH6BB1st8GqkV6qdGZDtCokCRwbjYe-1x7LuHOhb7TXN-jKyDboyU8do4_np_fZS7Z8m7_OpstMMahYpjfc5LkQKSlla1FxKdacKrnhNGdVRY2CotKmZGspS8VFVRFiAHKSF1BSwsbo7qzbe_c16BDrrRtOL4WaCMqBJ1mRqPszpbwLwWtT997upD_WBOqTmfVfMxPOzvjBtvr4L1sv5qtpwUrG2DdrqXVf</recordid><startdate>201707</startdate><enddate>201707</enddate><creator>Medvedev, А. V.</creator><creator>Ratovsky, K. G.</creator><creator>Tolstikov, M. V.</creator><creator>Oinats, A. V.</creator><creator>Alsatkin, S. S.</creator><creator>Zherebtsov, G. A.</creator><general>Blackwell Publishing Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-0847-3553</orcidid><orcidid>https://orcid.org/0000-0002-9176-5425</orcidid><orcidid>https://orcid.org/0000-0002-1120-870X</orcidid><orcidid>https://orcid.org/0000-0003-0660-8474</orcidid></search><sort><creationdate>201707</creationdate><title>Relation of internal gravity wave anisotropy with neutral wind characteristics in the upper atmosphere</title><author>Medvedev, А. V. ; Ratovsky, K. G. ; Tolstikov, M. V. ; Oinats, A. V. ; Alsatkin, S. S. ; Zherebtsov, G. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c3073-ed8f4499499223b978a9b82cad8243772fc057ef63baa6c897711f00414506213</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Anisotropy</topic><topic>Atmospheric models</topic><topic>Azimuth</topic><topic>Coherent radar</topic><topic>Filtration</topic><topic>Gravitational waves</topic><topic>Gravity waves</topic><topic>HF radar</topic><topic>Hypotheses</topic><topic>Incoherent scatter radar</topic><topic>internal gravitational waves</topic><topic>Internal gravity waves</topic><topic>Internal waves</topic><topic>Ionospheric disturbances</topic><topic>ionsphere</topic><topic>neutral wind</topic><topic>Parameter estimation</topic><topic>Radar</topic><topic>Thermosphere</topic><topic>Traveling ionospheric disturbances</topic><topic>Upper atmosphere</topic><topic>wave‐wind interaction</topic><topic>Wind</topic><topic>Wind models</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Medvedev, А. V.</creatorcontrib><creatorcontrib>Ratovsky, K. G.</creatorcontrib><creatorcontrib>Tolstikov, M. V.</creatorcontrib><creatorcontrib>Oinats, A. V.</creatorcontrib><creatorcontrib>Alsatkin, S. S.</creatorcontrib><creatorcontrib>Zherebtsov, G. A.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Journal of geophysical research. Space physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Medvedev, А. V.</au><au>Ratovsky, K. G.</au><au>Tolstikov, M. V.</au><au>Oinats, A. V.</au><au>Alsatkin, S. S.</au><au>Zherebtsov, G. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Relation of internal gravity wave anisotropy with neutral wind characteristics in the upper atmosphere</atitle><jtitle>Journal of geophysical research. Space physics</jtitle><date>2017-07</date><risdate>2017</risdate><volume>122</volume><issue>7</issue><spage>7567</spage><epage>7580</epage><pages>7567-7580</pages><issn>2169-9380</issn><eissn>2169-9402</eissn><abstract>This paper studies the interaction of internal gravity waves (IGW) with neutral wind using the statistics of traveling ionospheric disturbances (TID) from the Radio Physical Complex of the Institute of Solar‐Terrestrial Physics. The complex includes the Irkutsk Incoherent Scatter Radar (IISR), Irkutsk Ionosonde (DPS‐4), and Ekaterinburg HF Radar (EKB). The aim of this study is to give a common explanation for the TID azimuth distributions obtained with the IISR‐ionosonde and HF coherent radar and show that the measurements of 3‐D TID characteristics put into the hands of researchers an important tool to study neutral wind in the thermosphere. The distinctive features of this study are the following: (1) using different TID statistics from independent tools and, correspondingly, independent methods for determining TID characteristics; (2) using the 3‐D TID characteristics for testing the wind‐filtering hypothesis, which allows us to separate the IGW‐induced TIDs from TIDs of other nature and identify three TID types depending on their elevation angles; and (3) using the local time‐azimuth distribution of the TID number for testing the wind‐filtering hypothesis. This study allowed us to conclude that the observed IGW azimuth anisotropy can be mainly explained by the wind filtration mechanism with considering winds at 90–250 km heights. Using the 3‐D IGW characteristics allows us to estimate neutral wind parameters. Proposed methods are applicable for any tool which can obtain TID 3‐D characteristics. Using the proposed methods will enable us to organize a worldwide campaign to improve the existing neutral wind models.
Key Points
At least 60% of observed TID induced by IGW; TID LT‐azimuth distributions can be mainly explained by the wind filtration mechanism
There are differences between azimuth distributions of three TID types (source below, source above, and reflected)
Methods of neutral wind estimating were proposed</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1002/2017JA024103</doi><tpages>14</tpages><orcidid>https://orcid.org/0000-0002-0847-3553</orcidid><orcidid>https://orcid.org/0000-0002-9176-5425</orcidid><orcidid>https://orcid.org/0000-0002-1120-870X</orcidid><orcidid>https://orcid.org/0000-0003-0660-8474</orcidid></addata></record> |
fulltext | fulltext |
identifier | ISSN: 2169-9380 |
ispartof | Journal of geophysical research. Space physics, 2017-07, Vol.122 (7), p.7567-7580 |
issn | 2169-9380 2169-9402 |
language | eng |
recordid | cdi_proquest_journals_1928082239 |
source | Wiley-Blackwell Read & Publish Collection |
subjects | Anisotropy Atmospheric models Azimuth Coherent radar Filtration Gravitational waves Gravity waves HF radar Hypotheses Incoherent scatter radar internal gravitational waves Internal gravity waves Internal waves Ionospheric disturbances ionsphere neutral wind Parameter estimation Radar Thermosphere Traveling ionospheric disturbances Upper atmosphere wave‐wind interaction Wind Wind models |
title | Relation of internal gravity wave anisotropy with neutral wind characteristics in the upper atmosphere |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-27T03%3A52%3A34IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Relation%20of%20internal%20gravity%20wave%20anisotropy%20with%20neutral%20wind%20characteristics%20in%20the%20upper%20atmosphere&rft.jtitle=Journal%20of%20geophysical%20research.%20Space%20physics&rft.au=Medvedev,%20%D0%90.%20V.&rft.date=2017-07&rft.volume=122&rft.issue=7&rft.spage=7567&rft.epage=7580&rft.pages=7567-7580&rft.issn=2169-9380&rft.eissn=2169-9402&rft_id=info:doi/10.1002/2017JA024103&rft_dat=%3Cproquest_cross%3E1928082239%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c3073-ed8f4499499223b978a9b82cad8243772fc057ef63baa6c897711f00414506213%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1928082239&rft_id=info:pmid/&rfr_iscdi=true |