Loading…
Near-UV Pulsations in the Aurora Region Measured by Orbital Telescope TUS during High-Intensity and Long-Duration Continuous AE Activity
Tracking Ultraviolet Set-up (TUS) on board the Lomonosov satellite measured the UV intensity pulsations in the auroral region. Sixty-four events with pulsations were registered during two measurement periods from 26 December 2016–10 January 2017 and 8–15 November 2017. During both periods, a high-in...
Saved in:
Published in: | Remote sensing (Basel, Switzerland) Switzerland), 2023-01, Vol.15 (1), p.147 |
---|---|
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-c361t-9a31afd58a1671be80b4e3e449d67afff1bac564586a96a69bcc35bf125b4a533 |
---|---|
cites | cdi_FETCH-LOGICAL-c361t-9a31afd58a1671be80b4e3e449d67afff1bac564586a96a69bcc35bf125b4a533 |
container_end_page | |
container_issue | 1 |
container_start_page | 147 |
container_title | Remote sensing (Basel, Switzerland) |
container_volume | 15 |
creator | Klimov, Pavel Kalegaev, Vladimir Sigaeva, Ksenia Ivanova, Alexandra Antonyuk, Grigory Benghin, Viktor Zolotarev, Ivan |
description | Tracking Ultraviolet Set-up (TUS) on board the Lomonosov satellite measured the UV intensity pulsations in the auroral region. Sixty-four events with pulsations were registered during two measurement periods from 26 December 2016–10 January 2017 and 8–15 November 2017. During both periods, a high-intensity, long-duration, continuous auroral activity (HILDCAA) was detected. Simultaneous measurements in LEO by Lomonosov (DEPRON detector) and Meteor-M2 satellites show the enhanced fluxes of the trapped and precipitated energetic electrons in the region of the Earth’s outer radiation belt during these periods. We found that most of the UV-events correspond to energetic electron (E > 100 keV) precipitation. One can suggest that particles of these and higher energies cause a pulsating emission relatively deep in the atmosphere. |
doi_str_mv | 10.3390/rs15010147 |
format | article |
fullrecord | <record><control><sourceid>proquest_doaj_</sourceid><recordid>TN_cdi_doaj_primary_oai_doaj_org_article_602dc96b1db64cde9411f97713e48dc6</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><doaj_id>oai_doaj_org_article_602dc96b1db64cde9411f97713e48dc6</doaj_id><sourcerecordid>2761198450</sourcerecordid><originalsourceid>FETCH-LOGICAL-c361t-9a31afd58a1671be80b4e3e449d67afff1bac564586a96a69bcc35bf125b4a533</originalsourceid><addsrcrecordid>eNpNkd2KFDEQhRtRcNndG58g4J3Qmuqk053LYVx3B2Zd0Rlvm8pP92ZokzE_wryBj227I2rdVHE4fKfgVNUroG8Zk_RdTNBSoMC7Z9VFQ7um5o1snv93v6yuUzrQZRgDSflF9fOjxVjvv5JPZU6YXfCJOE_yoyWrEkNE8tlOi0ruLaYSrSHqRB6ichlnsrOzTTocLdntvxBTovMTuXPTY73x2frk8omgN2Qb_FS_L_GJT9bBZ-dLKImsbshKZ_djMV5VL0ack73-sy-r_Yeb3fqu3j7cbtarba2ZgFxLZICjaXsE0YGyPVXcMsu5NKLDcRxBoW4Fb3uBUqCQSmvWqhGaVnFsGbusNmeuCXgYjtF9w3gaArrhSQhxGjBmp2c7CNoYLYUCowTXxkoOMMqugyWvN1osrNdn1jGG78WmPBxCiX55f2g6ASB73tLF9ebs0jGkFO34NxXo8Lu44V9x7Be1XYtD</addsrcrecordid><sourcetype>Open Website</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2761198450</pqid></control><display><type>article</type><title>Near-UV Pulsations in the Aurora Region Measured by Orbital Telescope TUS during High-Intensity and Long-Duration Continuous AE Activity</title><source>Publicly Available Content Database</source><creator>Klimov, Pavel ; Kalegaev, Vladimir ; Sigaeva, Ksenia ; Ivanova, Alexandra ; Antonyuk, Grigory ; Benghin, Viktor ; Zolotarev, Ivan</creator><creatorcontrib>Klimov, Pavel ; Kalegaev, Vladimir ; Sigaeva, Ksenia ; Ivanova, Alexandra ; Antonyuk, Grigory ; Benghin, Viktor ; Zolotarev, Ivan</creatorcontrib><description>Tracking Ultraviolet Set-up (TUS) on board the Lomonosov satellite measured the UV intensity pulsations in the auroral region. Sixty-four events with pulsations were registered during two measurement periods from 26 December 2016–10 January 2017 and 8–15 November 2017. During both periods, a high-intensity, long-duration, continuous auroral activity (HILDCAA) was detected. Simultaneous measurements in LEO by Lomonosov (DEPRON detector) and Meteor-M2 satellites show the enhanced fluxes of the trapped and precipitated energetic electrons in the region of the Earth’s outer radiation belt during these periods. We found that most of the UV-events correspond to energetic electron (E > 100 keV) precipitation. One can suggest that particles of these and higher energies cause a pulsating emission relatively deep in the atmosphere.</description><identifier>ISSN: 2072-4292</identifier><identifier>EISSN: 2072-4292</identifier><identifier>DOI: 10.3390/rs15010147</identifier><language>eng</language><publisher>Basel: MDPI AG</publisher><subject>Altitude ; Auroras ; Cameras ; Charged particles ; Electrons ; energetic electrons ; Magnetic fields ; multi-satellite measurements ; Outer radiation belt ; pulsating aurora ; Radiation ; Radiation belts ; Satellite tracking ; Sensors ; Telescopes</subject><ispartof>Remote sensing (Basel, Switzerland), 2023-01, Vol.15 (1), p.147</ispartof><rights>2022 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c361t-9a31afd58a1671be80b4e3e449d67afff1bac564586a96a69bcc35bf125b4a533</citedby><cites>FETCH-LOGICAL-c361t-9a31afd58a1671be80b4e3e449d67afff1bac564586a96a69bcc35bf125b4a533</cites><orcidid>0000-0002-3214-7184 ; 0000-0001-9815-6123</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/2761198450/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/2761198450?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,777,781,25734,27905,27906,36993,44571,74875</link.rule.ids></links><search><creatorcontrib>Klimov, Pavel</creatorcontrib><creatorcontrib>Kalegaev, Vladimir</creatorcontrib><creatorcontrib>Sigaeva, Ksenia</creatorcontrib><creatorcontrib>Ivanova, Alexandra</creatorcontrib><creatorcontrib>Antonyuk, Grigory</creatorcontrib><creatorcontrib>Benghin, Viktor</creatorcontrib><creatorcontrib>Zolotarev, Ivan</creatorcontrib><title>Near-UV Pulsations in the Aurora Region Measured by Orbital Telescope TUS during High-Intensity and Long-Duration Continuous AE Activity</title><title>Remote sensing (Basel, Switzerland)</title><description>Tracking Ultraviolet Set-up (TUS) on board the Lomonosov satellite measured the UV intensity pulsations in the auroral region. Sixty-four events with pulsations were registered during two measurement periods from 26 December 2016–10 January 2017 and 8–15 November 2017. During both periods, a high-intensity, long-duration, continuous auroral activity (HILDCAA) was detected. Simultaneous measurements in LEO by Lomonosov (DEPRON detector) and Meteor-M2 satellites show the enhanced fluxes of the trapped and precipitated energetic electrons in the region of the Earth’s outer radiation belt during these periods. We found that most of the UV-events correspond to energetic electron (E > 100 keV) precipitation. One can suggest that particles of these and higher energies cause a pulsating emission relatively deep in the atmosphere.</description><subject>Altitude</subject><subject>Auroras</subject><subject>Cameras</subject><subject>Charged particles</subject><subject>Electrons</subject><subject>energetic electrons</subject><subject>Magnetic fields</subject><subject>multi-satellite measurements</subject><subject>Outer radiation belt</subject><subject>pulsating aurora</subject><subject>Radiation</subject><subject>Radiation belts</subject><subject>Satellite tracking</subject><subject>Sensors</subject><subject>Telescopes</subject><issn>2072-4292</issn><issn>2072-4292</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><sourceid>DOA</sourceid><recordid>eNpNkd2KFDEQhRtRcNndG58g4J3Qmuqk053LYVx3B2Zd0Rlvm8pP92ZokzE_wryBj227I2rdVHE4fKfgVNUroG8Zk_RdTNBSoMC7Z9VFQ7um5o1snv93v6yuUzrQZRgDSflF9fOjxVjvv5JPZU6YXfCJOE_yoyWrEkNE8tlOi0ruLaYSrSHqRB6ichlnsrOzTTocLdntvxBTovMTuXPTY73x2frk8omgN2Qb_FS_L_GJT9bBZ-dLKImsbshKZ_djMV5VL0ack73-sy-r_Yeb3fqu3j7cbtarba2ZgFxLZICjaXsE0YGyPVXcMsu5NKLDcRxBoW4Fb3uBUqCQSmvWqhGaVnFsGbusNmeuCXgYjtF9w3gaArrhSQhxGjBmp2c7CNoYLYUCowTXxkoOMMqugyWvN1osrNdn1jGG78WmPBxCiX55f2g6ASB73tLF9ebs0jGkFO34NxXo8Lu44V9x7Be1XYtD</recordid><startdate>20230101</startdate><enddate>20230101</enddate><creator>Klimov, Pavel</creator><creator>Kalegaev, Vladimir</creator><creator>Sigaeva, Ksenia</creator><creator>Ivanova, Alexandra</creator><creator>Antonyuk, Grigory</creator><creator>Benghin, Viktor</creator><creator>Zolotarev, Ivan</creator><general>MDPI AG</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7QF</scope><scope>7QO</scope><scope>7QQ</scope><scope>7QR</scope><scope>7SC</scope><scope>7SE</scope><scope>7SN</scope><scope>7SP</scope><scope>7SR</scope><scope>7TA</scope><scope>7TB</scope><scope>7U5</scope><scope>8BQ</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F28</scope><scope>FR3</scope><scope>H8D</scope><scope>H8G</scope><scope>HCIFZ</scope><scope>JG9</scope><scope>JQ2</scope><scope>KR7</scope><scope>L6V</scope><scope>L7M</scope><scope>L~C</scope><scope>L~D</scope><scope>M7S</scope><scope>P5Z</scope><scope>P62</scope><scope>P64</scope><scope>PCBAR</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PTHSS</scope><scope>DOA</scope><orcidid>https://orcid.org/0000-0002-3214-7184</orcidid><orcidid>https://orcid.org/0000-0001-9815-6123</orcidid></search><sort><creationdate>20230101</creationdate><title>Near-UV Pulsations in the Aurora Region Measured by Orbital Telescope TUS during High-Intensity and Long-Duration Continuous AE Activity</title><author>Klimov, Pavel ; Kalegaev, Vladimir ; Sigaeva, Ksenia ; Ivanova, Alexandra ; Antonyuk, Grigory ; Benghin, Viktor ; Zolotarev, Ivan</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c361t-9a31afd58a1671be80b4e3e449d67afff1bac564586a96a69bcc35bf125b4a533</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Altitude</topic><topic>Auroras</topic><topic>Cameras</topic><topic>Charged particles</topic><topic>Electrons</topic><topic>energetic electrons</topic><topic>Magnetic fields</topic><topic>multi-satellite measurements</topic><topic>Outer radiation belt</topic><topic>pulsating aurora</topic><topic>Radiation</topic><topic>Radiation belts</topic><topic>Satellite tracking</topic><topic>Sensors</topic><topic>Telescopes</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Klimov, Pavel</creatorcontrib><creatorcontrib>Kalegaev, Vladimir</creatorcontrib><creatorcontrib>Sigaeva, Ksenia</creatorcontrib><creatorcontrib>Ivanova, Alexandra</creatorcontrib><creatorcontrib>Antonyuk, Grigory</creatorcontrib><creatorcontrib>Benghin, Viktor</creatorcontrib><creatorcontrib>Zolotarev, Ivan</creatorcontrib><collection>CrossRef</collection><collection>Aluminium Industry Abstracts</collection><collection>Biotechnology Research Abstracts</collection><collection>Ceramic Abstracts</collection><collection>Chemoreception Abstracts</collection><collection>Computer and Information Systems Abstracts</collection><collection>Corrosion Abstracts</collection><collection>Ecology Abstracts</collection><collection>Electronics & Communications Abstracts</collection><collection>Engineered Materials Abstracts</collection><collection>Materials Business File</collection><collection>Mechanical & Transportation Engineering Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>METADEX</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>ANTE: Abstracts in New Technology & Engineering</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Copper Technical Reference Library</collection><collection>SciTech Premium Collection</collection><collection>Materials Research Database</collection><collection>ProQuest Computer Science Collection</collection><collection>Civil Engineering Abstracts</collection><collection>ProQuest Engineering Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Computer and Information Systems Abstracts Academic</collection><collection>Computer and Information Systems Abstracts Professional</collection><collection>Engineering Database</collection><collection>ProQuest advanced technologies & aerospace journals</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Biotechnology and BioEngineering Abstracts</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>Engineering collection</collection><collection>DOAJ Directory of Open Access Journals</collection><jtitle>Remote sensing (Basel, Switzerland)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Klimov, Pavel</au><au>Kalegaev, Vladimir</au><au>Sigaeva, Ksenia</au><au>Ivanova, Alexandra</au><au>Antonyuk, Grigory</au><au>Benghin, Viktor</au><au>Zolotarev, Ivan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Near-UV Pulsations in the Aurora Region Measured by Orbital Telescope TUS during High-Intensity and Long-Duration Continuous AE Activity</atitle><jtitle>Remote sensing (Basel, Switzerland)</jtitle><date>2023-01-01</date><risdate>2023</risdate><volume>15</volume><issue>1</issue><spage>147</spage><pages>147-</pages><issn>2072-4292</issn><eissn>2072-4292</eissn><abstract>Tracking Ultraviolet Set-up (TUS) on board the Lomonosov satellite measured the UV intensity pulsations in the auroral region. Sixty-four events with pulsations were registered during two measurement periods from 26 December 2016–10 January 2017 and 8–15 November 2017. During both periods, a high-intensity, long-duration, continuous auroral activity (HILDCAA) was detected. Simultaneous measurements in LEO by Lomonosov (DEPRON detector) and Meteor-M2 satellites show the enhanced fluxes of the trapped and precipitated energetic electrons in the region of the Earth’s outer radiation belt during these periods. We found that most of the UV-events correspond to energetic electron (E > 100 keV) precipitation. One can suggest that particles of these and higher energies cause a pulsating emission relatively deep in the atmosphere.</abstract><cop>Basel</cop><pub>MDPI AG</pub><doi>10.3390/rs15010147</doi><orcidid>https://orcid.org/0000-0002-3214-7184</orcidid><orcidid>https://orcid.org/0000-0001-9815-6123</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 2072-4292 |
ispartof | Remote sensing (Basel, Switzerland), 2023-01, Vol.15 (1), p.147 |
issn | 2072-4292 2072-4292 |
language | eng |
recordid | cdi_doaj_primary_oai_doaj_org_article_602dc96b1db64cde9411f97713e48dc6 |
source | Publicly Available Content Database |
subjects | Altitude Auroras Cameras Charged particles Electrons energetic electrons Magnetic fields multi-satellite measurements Outer radiation belt pulsating aurora Radiation Radiation belts Satellite tracking Sensors Telescopes |
title | Near-UV Pulsations in the Aurora Region Measured by Orbital Telescope TUS during High-Intensity and Long-Duration Continuous AE Activity |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-19T14%3A32%3A43IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_doaj_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Near-UV%20Pulsations%20in%20the%20Aurora%20Region%20Measured%20by%20Orbital%20Telescope%20TUS%20during%20High-Intensity%20and%20Long-Duration%20Continuous%20AE%20Activity&rft.jtitle=Remote%20sensing%20(Basel,%20Switzerland)&rft.au=Klimov,%20Pavel&rft.date=2023-01-01&rft.volume=15&rft.issue=1&rft.spage=147&rft.pages=147-&rft.issn=2072-4292&rft.eissn=2072-4292&rft_id=info:doi/10.3390/rs15010147&rft_dat=%3Cproquest_doaj_%3E2761198450%3C/proquest_doaj_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c361t-9a31afd58a1671be80b4e3e449d67afff1bac564586a96a69bcc35bf125b4a533%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2761198450&rft_id=info:pmid/&rfr_iscdi=true |