Resonance electromagnetic effect of the Kamchatka meteoroid
A large meteoroid entered the terrestrial atmosphere and exploded at an altitude of 26 km between the Kamchatka Peninsula and Alaska (geographic coordinates 56.9 degrees N, 172.4 degrees E) over the Bering Sea at 23:48:20 UT on December 18, 2018. The meteoroid has been named the Kamchatka (or Bering...
Published in: | Kinematics and Physics of Celestial Bodies |
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ftunivgent:oai:archive.ugent.be:01HR68YQ5M5FE2XZSFPQ103SNF 2024-04-28T08:14:39+00:00 Resonance electromagnetic effect of the Kamchatka meteoroid Luo, Yiyang Chernogor, L. F. 2023 application/pdf https://biblio.ugent.be/publication/01HR68YQ5M5FE2XZSFPQ103SNF http://hdl.handle.net/1854/LU-01HR68YQ5M5FE2XZSFPQ103SNF https://doi.org/10.3103/S0884591323010051 https://biblio.ugent.be/publication/01HR68YQ5M5FE2XZSFPQ103SNF/file/01HT29K11RATK4NWBVWMBKVR03 eng eng https://biblio.ugent.be/publication/01HR68YQ5M5FE2XZSFPQ103SNF http://hdl.handle.net/1854/LU-01HR68YQ5M5FE2XZSFPQ103SNF http://doi.org/10.3103/S0884591323010051 https://biblio.ugent.be/publication/01HR68YQ5M5FE2XZSFPQ103SNF/file/01HT29K11RATK4NWBVWMBKVR03 No license (in copyright) info:eu-repo/semantics/restrictedAccess KINEMATICS AND PHYSICS OF CELESTIAL BODIES ISSN: 0884-5913 ISSN: 1934-8401 Physics and Astronomy Kamchatka meteoroid resonance effect electromagnetic effect mechanism explosive impact oscillation of magnetic field line CHELYABINSK AIRBURST journalArticle info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 2023 ftunivgent https://doi.org/10.3103/S0884591323010051 2024-04-09T23:31:17Z A large meteoroid entered the terrestrial atmosphere and exploded at an altitude of 26 km between the Kamchatka Peninsula and Alaska (geographic coordinates 56.9 degrees N, 172.4 degrees E) over the Bering Sea at 23:48:20 UT on December 18, 2018. The meteoroid has been named the Kamchatka (or Bering Sea) meteoroid. Its basic parameters are as follows: calculated total impact energy 173 kt of TNT, total optical radiated energy 1.3 x 10(14) J, mass 1.41 kt, speed 32 km/s, size 9.4 m, and the trajectory directed at an angle of 68.6 degrees with respect to the horizon. The entry of the Kamchatka meteoroid into the atmosphere was accompanied by the generation of a transient resonance electromagnetic signal in the 25-35 mHz band observable in the vicinity of the meteoroid explosion and in the magnetically conjugate region. Oscillations with amplitudes of 0.2-0.8 nT were observed over a 7-min interval. This study is aimed at analyzing the observations of the resonance electromagnetic effect from the Kamchatka meteoroid and discussing a mechanism for this effect. The resonance effect in the Earth's magnetic field is analyzed using data with a time resolution of 1 s and an amplitude resolution of 1 nT from the database collected by the Intermagnet magnetometer network of magnetic observatories. The distance between the site of the meteoroid explosion and the magnetic observatories ranges from 1000 to 5000 km in the Northern Hemisphere and from 9010 to 12 425 km in the Southern Hemisphere. It is established that the only feasible mechanism is associated with the magnetic field displacement in the magnetosphere by the explosive impact of the celestial body, whereas only a negligibly small part of the meteoroid's energy is spent on the generation of magnetic field perturbations. The meteoroid's energy losses are similar to the losses in the reactive components of the radio frequency circuits, i.e., they return into the system. The oscillations cease after the meteoroid flies by, and the system returns into the initial ... Article in Journal/Newspaper Bering Sea Kamchatka Kamchatka Peninsula Alaska Ghent University Academic Bibliography Kinematics and Physics of Celestial Bodies 39 1 1 9 |
institution |
Open Polar |
collection |
Ghent University Academic Bibliography |
op_collection_id |
ftunivgent |
language |
English |
topic |
Physics and Astronomy Kamchatka meteoroid resonance effect electromagnetic effect mechanism explosive impact oscillation of magnetic field line CHELYABINSK AIRBURST |
spellingShingle |
Physics and Astronomy Kamchatka meteoroid resonance effect electromagnetic effect mechanism explosive impact oscillation of magnetic field line CHELYABINSK AIRBURST Luo, Yiyang Chernogor, L. F. Resonance electromagnetic effect of the Kamchatka meteoroid |
topic_facet |
Physics and Astronomy Kamchatka meteoroid resonance effect electromagnetic effect mechanism explosive impact oscillation of magnetic field line CHELYABINSK AIRBURST |
description |
A large meteoroid entered the terrestrial atmosphere and exploded at an altitude of 26 km between the Kamchatka Peninsula and Alaska (geographic coordinates 56.9 degrees N, 172.4 degrees E) over the Bering Sea at 23:48:20 UT on December 18, 2018. The meteoroid has been named the Kamchatka (or Bering Sea) meteoroid. Its basic parameters are as follows: calculated total impact energy 173 kt of TNT, total optical radiated energy 1.3 x 10(14) J, mass 1.41 kt, speed 32 km/s, size 9.4 m, and the trajectory directed at an angle of 68.6 degrees with respect to the horizon. The entry of the Kamchatka meteoroid into the atmosphere was accompanied by the generation of a transient resonance electromagnetic signal in the 25-35 mHz band observable in the vicinity of the meteoroid explosion and in the magnetically conjugate region. Oscillations with amplitudes of 0.2-0.8 nT were observed over a 7-min interval. This study is aimed at analyzing the observations of the resonance electromagnetic effect from the Kamchatka meteoroid and discussing a mechanism for this effect. The resonance effect in the Earth's magnetic field is analyzed using data with a time resolution of 1 s and an amplitude resolution of 1 nT from the database collected by the Intermagnet magnetometer network of magnetic observatories. The distance between the site of the meteoroid explosion and the magnetic observatories ranges from 1000 to 5000 km in the Northern Hemisphere and from 9010 to 12 425 km in the Southern Hemisphere. It is established that the only feasible mechanism is associated with the magnetic field displacement in the magnetosphere by the explosive impact of the celestial body, whereas only a negligibly small part of the meteoroid's energy is spent on the generation of magnetic field perturbations. The meteoroid's energy losses are similar to the losses in the reactive components of the radio frequency circuits, i.e., they return into the system. The oscillations cease after the meteoroid flies by, and the system returns into the initial ... |
format |
Article in Journal/Newspaper |
author |
Luo, Yiyang Chernogor, L. F. |
author_facet |
Luo, Yiyang Chernogor, L. F. |
author_sort |
Luo, Yiyang |
title |
Resonance electromagnetic effect of the Kamchatka meteoroid |
title_short |
Resonance electromagnetic effect of the Kamchatka meteoroid |
title_full |
Resonance electromagnetic effect of the Kamchatka meteoroid |
title_fullStr |
Resonance electromagnetic effect of the Kamchatka meteoroid |
title_full_unstemmed |
Resonance electromagnetic effect of the Kamchatka meteoroid |
title_sort |
resonance electromagnetic effect of the kamchatka meteoroid |
publishDate |
2023 |
url |
https://biblio.ugent.be/publication/01HR68YQ5M5FE2XZSFPQ103SNF http://hdl.handle.net/1854/LU-01HR68YQ5M5FE2XZSFPQ103SNF https://doi.org/10.3103/S0884591323010051 https://biblio.ugent.be/publication/01HR68YQ5M5FE2XZSFPQ103SNF/file/01HT29K11RATK4NWBVWMBKVR03 |
genre |
Bering Sea Kamchatka Kamchatka Peninsula Alaska |
genre_facet |
Bering Sea Kamchatka Kamchatka Peninsula Alaska |
op_source |
KINEMATICS AND PHYSICS OF CELESTIAL BODIES ISSN: 0884-5913 ISSN: 1934-8401 |
op_relation |
https://biblio.ugent.be/publication/01HR68YQ5M5FE2XZSFPQ103SNF http://hdl.handle.net/1854/LU-01HR68YQ5M5FE2XZSFPQ103SNF http://doi.org/10.3103/S0884591323010051 https://biblio.ugent.be/publication/01HR68YQ5M5FE2XZSFPQ103SNF/file/01HT29K11RATK4NWBVWMBKVR03 |
op_rights |
No license (in copyright) info:eu-repo/semantics/restrictedAccess |
op_doi |
https://doi.org/10.3103/S0884591323010051 |
container_title |
Kinematics and Physics of Celestial Bodies |
container_volume |
39 |
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1 |
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1 |
op_container_end_page |
9 |
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1797580622055604224 |