Conjugate Ground-Spacecraft Observations of VLF Chorus Elements
We present results of simultaneous observations of VLF chorus elements at the ground-based station Kannuslehto in Northern Finland and on board Van Allen Probe A. Visual inspection and correlation analysis of the data reveal one-to-one correspondence of several (at least 12) chorus elements followin...
Published in: | Geophysical Research Letters |
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Online Access: | https://doi.org/10.1002/2017GL076139 http://hdl.handle.net/11104/0282366 |
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ftczacademyscien:oai:asep.lib.cas.cz:CavUnEpca/0487718 2024-09-09T19:59:19+00:00 Conjugate Ground-Spacecraft Observations of VLF Chorus Elements Demekhov, A. G. Manninen, J. Santolík, O. (Ondřej) Titova, E. E. 2017 https://doi.org/10.1002/2017GL076139 http://hdl.handle.net/11104/0282366 eng eng doi:10.1002/2017GL076139 urn:pissn: 0094-8276 urn:eissn: 1944-8007 http://hdl.handle.net/11104/0282366 VAN ALLEN PROBES WHISTLER-MODE WAVES MAGNETOSPHERIC CHORUS PROPAGATION EMISSIONS BAND FREQUENCY AMPLITUDE MASER GUIDE info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 2017 ftczacademyscien https://doi.org/10.1002/2017GL076139 2024-08-19T05:33:01Z We present results of simultaneous observations of VLF chorus elements at the ground-based station Kannuslehto in Northern Finland and on board Van Allen Probe A. Visual inspection and correlation analysis of the data reveal one-to-one correspondence of several (at least 12) chorus elements following each other in a sequence. Poynting flux calculated from electromagnetic fields measured by the Electric and Magnetic Field Instrument Suite and Integrated Science instrument on board Van Allen Probe A shows that the waves propagate at small angles to the geomagnetic field and oppositely to its direction, that is, from northern to southern geographic hemisphere. The spacecraft was located at L similar or equal to 4.1 at a geomagnetic latitude of -12.4 degrees close to the plasmapause and inside a localized density inhomogeneity with about 30% density increase and a transverse size of about 600 km. The time delay between the waves detected on the ground and on the spacecraft is about 1.3 s, with ground-based detection leading spacecraft detection. The measured time delay is consistent with the wave travel time of quasi-parallel whistler-mode waves for a realistic profile of the plasma density distribution along the field line. The results suggest that chorus discrete elements can preserve their spectral shape during a hop from the generation region to the ground followed by reflection from the ionosphere and return to the near-equatorial region. Article in Journal/Newspaper Northern Finland The Czech Academy of Sciences: Publication Activity (ASEP) Geophysical Research Letters 44 23 11,735 11,744 |
institution |
Open Polar |
collection |
The Czech Academy of Sciences: Publication Activity (ASEP) |
op_collection_id |
ftczacademyscien |
language |
English |
topic |
VAN ALLEN PROBES WHISTLER-MODE WAVES MAGNETOSPHERIC CHORUS PROPAGATION EMISSIONS BAND FREQUENCY AMPLITUDE MASER GUIDE |
spellingShingle |
VAN ALLEN PROBES WHISTLER-MODE WAVES MAGNETOSPHERIC CHORUS PROPAGATION EMISSIONS BAND FREQUENCY AMPLITUDE MASER GUIDE Demekhov, A. G. Manninen, J. Santolík, O. (Ondřej) Titova, E. E. Conjugate Ground-Spacecraft Observations of VLF Chorus Elements |
topic_facet |
VAN ALLEN PROBES WHISTLER-MODE WAVES MAGNETOSPHERIC CHORUS PROPAGATION EMISSIONS BAND FREQUENCY AMPLITUDE MASER GUIDE |
description |
We present results of simultaneous observations of VLF chorus elements at the ground-based station Kannuslehto in Northern Finland and on board Van Allen Probe A. Visual inspection and correlation analysis of the data reveal one-to-one correspondence of several (at least 12) chorus elements following each other in a sequence. Poynting flux calculated from electromagnetic fields measured by the Electric and Magnetic Field Instrument Suite and Integrated Science instrument on board Van Allen Probe A shows that the waves propagate at small angles to the geomagnetic field and oppositely to its direction, that is, from northern to southern geographic hemisphere. The spacecraft was located at L similar or equal to 4.1 at a geomagnetic latitude of -12.4 degrees close to the plasmapause and inside a localized density inhomogeneity with about 30% density increase and a transverse size of about 600 km. The time delay between the waves detected on the ground and on the spacecraft is about 1.3 s, with ground-based detection leading spacecraft detection. The measured time delay is consistent with the wave travel time of quasi-parallel whistler-mode waves for a realistic profile of the plasma density distribution along the field line. The results suggest that chorus discrete elements can preserve their spectral shape during a hop from the generation region to the ground followed by reflection from the ionosphere and return to the near-equatorial region. |
format |
Article in Journal/Newspaper |
author |
Demekhov, A. G. Manninen, J. Santolík, O. (Ondřej) Titova, E. E. |
author_facet |
Demekhov, A. G. Manninen, J. Santolík, O. (Ondřej) Titova, E. E. |
author_sort |
Demekhov, A. G. |
title |
Conjugate Ground-Spacecraft Observations of VLF Chorus Elements |
title_short |
Conjugate Ground-Spacecraft Observations of VLF Chorus Elements |
title_full |
Conjugate Ground-Spacecraft Observations of VLF Chorus Elements |
title_fullStr |
Conjugate Ground-Spacecraft Observations of VLF Chorus Elements |
title_full_unstemmed |
Conjugate Ground-Spacecraft Observations of VLF Chorus Elements |
title_sort |
conjugate ground-spacecraft observations of vlf chorus elements |
publishDate |
2017 |
url |
https://doi.org/10.1002/2017GL076139 http://hdl.handle.net/11104/0282366 |
genre |
Northern Finland |
genre_facet |
Northern Finland |
op_relation |
doi:10.1002/2017GL076139 urn:pissn: 0094-8276 urn:eissn: 1944-8007 http://hdl.handle.net/11104/0282366 |
op_doi |
https://doi.org/10.1002/2017GL076139 |
container_title |
Geophysical Research Letters |
container_volume |
44 |
container_issue |
23 |
container_start_page |
11,735 |
op_container_end_page |
11,744 |
_version_ |
1809930452043038720 |