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Longitudinal Dependence of Whistler Mode Electromagnetic Waves in the Earth's Inner Magnetosphere
We use the measurements performed by the DEMETER (2004–010) and the Van Allen Probes (2012–016, still operating) spacecraft to investigate the longitudinal dependence of the intensity of whistler mode waves in the Earth's inner magnetosphere. We show that a significant longitudinal dependence i...
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Published in: | Journal of geophysical research. Space physics 2018-08, Vol.123 (8), p.6562-6575 |
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container_end_page | 6575 |
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container_title | Journal of geophysical research. Space physics |
container_volume | 123 |
creator | Záhlava, J. Němec, F. Santolík, O. Kolmašova, I. Hospodarsky, G. B. Parrot, M. Kurth, W. S. Bortnik, J. Kletzing, C. |
description | We use the measurements performed by the DEMETER (2004–010) and the Van Allen Probes (2012–016, still operating) spacecraft to investigate the longitudinal dependence of the intensity of whistler mode waves in the Earth's inner magnetosphere. We show that a significant longitudinal dependence is observed inside the plasmasphere on the nightside, primarily in the frequency range 400 Hz to 2 kHz. On the other hand, almost no longitudinal dependence is observed on the dayside. The obtained results are compared to the lightning occurrence rate provided by the Optical Transient Detector/Lightning Imaging Sensor mission normalized by a factor accounting for the ionospheric attenuation. The agreement between the two dependencies indicates that lightning‐generated electromagnetic waves may be responsible for of the observed effect, thus substantially affecting the overall wave intensity in the given frequency range. Finally, we show that the longitudinal dependence is most pronounced for waves with oblique wave of normal angles.
Key Points
Longitudinal dependence of whistler mode waves in the inner magnetosphere is investigated
Significant longitudinal dependence at frequencies between about 0.4 and 2 kHz is found inside the plasmasphere
The dependence is primarily observed on the nightside and is likely related to lightning activity |
doi_str_mv | 10.1029/2018JA025284 |
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Key Points
Longitudinal dependence of whistler mode waves in the inner magnetosphere is investigated
Significant longitudinal dependence at frequencies between about 0.4 and 2 kHz is found inside the plasmasphere
The dependence is primarily observed on the nightside and is likely related to lightning activity</description><identifier>ISSN: 2169-9380</identifier><identifier>EISSN: 2169-9402</identifier><identifier>DOI: 10.1029/2018JA025284</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Attenuation ; DEMETER ; Dependence ; Earth magnetosphere ; Earth Sciences ; Electromagnetic radiation ; Geophysics ; Lightning ; Magnetism ; Magnetosphere ; Physics ; Plasmasphere ; Sciences of the Universe ; Space Physics ; Spacecraft ; Van Allen Probes ; whistler waves</subject><ispartof>Journal of geophysical research. Space physics, 2018-08, Vol.123 (8), p.6562-6575</ispartof><rights>2018. American Geophysical Union. All Rights Reserved.</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c4467-fd9d65b5729d032148afa9c5d637746d862b61954894274e67a2cb3d64473d793</citedby><cites>FETCH-LOGICAL-c4467-fd9d65b5729d032148afa9c5d637746d862b61954894274e67a2cb3d64473d793</cites><orcidid>0000-0002-3233-2718 ; 0000-0003-0905-5721 ; 0000-0002-5471-6202 ; 0000-0002-4891-9273 ; 0000-0002-2334-9331 ; 0000-0002-1704-3846 ; 0000-0002-4136-3348 ; 0000-0001-9200-9878 ; 0000-0001-8811-8836</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttps://insu.hal.science/insu-01897671$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Záhlava, J.</creatorcontrib><creatorcontrib>Němec, F.</creatorcontrib><creatorcontrib>Santolík, O.</creatorcontrib><creatorcontrib>Kolmašova, I.</creatorcontrib><creatorcontrib>Hospodarsky, G. B.</creatorcontrib><creatorcontrib>Parrot, M.</creatorcontrib><creatorcontrib>Kurth, W. S.</creatorcontrib><creatorcontrib>Bortnik, J.</creatorcontrib><creatorcontrib>Kletzing, C.</creatorcontrib><title>Longitudinal Dependence of Whistler Mode Electromagnetic Waves in the Earth's Inner Magnetosphere</title><title>Journal of geophysical research. Space physics</title><description>We use the measurements performed by the DEMETER (2004–010) and the Van Allen Probes (2012–016, still operating) spacecraft to investigate the longitudinal dependence of the intensity of whistler mode waves in the Earth's inner magnetosphere. We show that a significant longitudinal dependence is observed inside the plasmasphere on the nightside, primarily in the frequency range 400 Hz to 2 kHz. On the other hand, almost no longitudinal dependence is observed on the dayside. The obtained results are compared to the lightning occurrence rate provided by the Optical Transient Detector/Lightning Imaging Sensor mission normalized by a factor accounting for the ionospheric attenuation. The agreement between the two dependencies indicates that lightning‐generated electromagnetic waves may be responsible for of the observed effect, thus substantially affecting the overall wave intensity in the given frequency range. Finally, we show that the longitudinal dependence is most pronounced for waves with oblique wave of normal angles.
Key Points
Longitudinal dependence of whistler mode waves in the inner magnetosphere is investigated
Significant longitudinal dependence at frequencies between about 0.4 and 2 kHz is found inside the plasmasphere
The dependence is primarily observed on the nightside and is likely related to lightning activity</description><subject>Attenuation</subject><subject>DEMETER</subject><subject>Dependence</subject><subject>Earth magnetosphere</subject><subject>Earth Sciences</subject><subject>Electromagnetic radiation</subject><subject>Geophysics</subject><subject>Lightning</subject><subject>Magnetism</subject><subject>Magnetosphere</subject><subject>Physics</subject><subject>Plasmasphere</subject><subject>Sciences of the Universe</subject><subject>Space Physics</subject><subject>Spacecraft</subject><subject>Van Allen Probes</subject><subject>whistler waves</subject><issn>2169-9380</issn><issn>2169-9402</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNp9kE1LAzEQhoMoWGpv_oCAB0FcTbLZZHMstfaDiiBKjyHdZLsp26Qm20r_vVur4sm5zDDz8DI8AFxidIcREfcE4XzaRyQjOT0BHYKZSARF5PRnTnN0DnoxrlBbebvCWQeomXdL22y1daqGD2ZjnDauMNCXcF7Z2NQmwCevDRzWpmiCX6ulM40t4FztTITWwaZqjyo01XWEE-cO_Bfj46YywVyAs1LV0fS-exe8PQ5fB-Nk9jyaDPqzpKCU8aTUQrNskXEiNEoJprkqlSgyzVLOKdM5IwuGRUZzQQmnhnFFikWqGaU81VykXXBzzK1ULTfBrlXYS6-sHPdn0rq4la0gwRnHO9zCV0d4E_z71sRGrvw2tAqiJBgTjjlpY7vg9kgVwccYTPmbi5E8SJd_pbd4esQ_bG32_7JyOnrpZ_Tw-yc9jYCK</recordid><startdate>201808</startdate><enddate>201808</enddate><creator>Záhlava, J.</creator><creator>Němec, F.</creator><creator>Santolík, O.</creator><creator>Kolmašova, I.</creator><creator>Hospodarsky, G. 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B. ; Parrot, M. ; Kurth, W. 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B.</creatorcontrib><creatorcontrib>Parrot, M.</creatorcontrib><creatorcontrib>Kurth, W. S.</creatorcontrib><creatorcontrib>Bortnik, J.</creatorcontrib><creatorcontrib>Kletzing, C.</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><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Journal of geophysical research. Space physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Záhlava, J.</au><au>Němec, F.</au><au>Santolík, O.</au><au>Kolmašova, I.</au><au>Hospodarsky, G. B.</au><au>Parrot, M.</au><au>Kurth, W. S.</au><au>Bortnik, J.</au><au>Kletzing, C.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Longitudinal Dependence of Whistler Mode Electromagnetic Waves in the Earth's Inner Magnetosphere</atitle><jtitle>Journal of geophysical research. Space physics</jtitle><date>2018-08</date><risdate>2018</risdate><volume>123</volume><issue>8</issue><spage>6562</spage><epage>6575</epage><pages>6562-6575</pages><issn>2169-9380</issn><eissn>2169-9402</eissn><abstract>We use the measurements performed by the DEMETER (2004–010) and the Van Allen Probes (2012–016, still operating) spacecraft to investigate the longitudinal dependence of the intensity of whistler mode waves in the Earth's inner magnetosphere. We show that a significant longitudinal dependence is observed inside the plasmasphere on the nightside, primarily in the frequency range 400 Hz to 2 kHz. On the other hand, almost no longitudinal dependence is observed on the dayside. The obtained results are compared to the lightning occurrence rate provided by the Optical Transient Detector/Lightning Imaging Sensor mission normalized by a factor accounting for the ionospheric attenuation. The agreement between the two dependencies indicates that lightning‐generated electromagnetic waves may be responsible for of the observed effect, thus substantially affecting the overall wave intensity in the given frequency range. Finally, we show that the longitudinal dependence is most pronounced for waves with oblique wave of normal angles.
Key Points
Longitudinal dependence of whistler mode waves in the inner magnetosphere is investigated
Significant longitudinal dependence at frequencies between about 0.4 and 2 kHz is found inside the plasmasphere
The dependence is primarily observed on the nightside and is likely related to lightning activity</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2018JA025284</doi><tpages>14</tpages><orcidid>https://orcid.org/0000-0002-3233-2718</orcidid><orcidid>https://orcid.org/0000-0003-0905-5721</orcidid><orcidid>https://orcid.org/0000-0002-5471-6202</orcidid><orcidid>https://orcid.org/0000-0002-4891-9273</orcidid><orcidid>https://orcid.org/0000-0002-2334-9331</orcidid><orcidid>https://orcid.org/0000-0002-1704-3846</orcidid><orcidid>https://orcid.org/0000-0002-4136-3348</orcidid><orcidid>https://orcid.org/0000-0001-9200-9878</orcidid><orcidid>https://orcid.org/0000-0001-8811-8836</orcidid><oa>free_for_read</oa></addata></record> |
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source | Wiley |
subjects | Attenuation DEMETER Dependence Earth magnetosphere Earth Sciences Electromagnetic radiation Geophysics Lightning Magnetism Magnetosphere Physics Plasmasphere Sciences of the Universe Space Physics Spacecraft Van Allen Probes whistler waves |
title | Longitudinal Dependence of Whistler Mode Electromagnetic Waves in the Earth's Inner Magnetosphere |
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