Radioseismology as a new method of investigations of meteor streams on the Moon and planets
Radioseismology is based on registration and interpretation of radio emission of seismic origin. Non-thermal radio emission of the Moon was detectedat 13 and 21 cm on July 30 - August 2, 1999. Strong oscillations of the non-thermal lunar radio flux at 25 mm were detected during the leonid meteor sho...
Main Authors: | , , , |
---|---|
Format: | Report |
Language: | unknown |
Published: |
arXiv
2001
|
Subjects: | |
Online Access: | https://dx.doi.org/10.48550/arxiv.astro-ph/0112498 https://arxiv.org/abs/astro-ph/0112498 |
id |
ftdatacite:10.48550/arxiv.astro-ph/0112498 |
---|---|
record_format |
openpolar |
spelling |
ftdatacite:10.48550/arxiv.astro-ph/0112498 2023-05-15T17:04:13+02:00 Radioseismology as a new method of investigations of meteor streams on the Moon and planets Berezhnoi, A. A. Bervalds, E. Khavroshkin, O. B. Ozolins, G. 2001 https://dx.doi.org/10.48550/arxiv.astro-ph/0112498 https://arxiv.org/abs/astro-ph/0112498 unknown arXiv Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph Geophysics physics.geo-ph FOS Physical sciences Preprint Article article CreativeWork 2001 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0112498 2022-04-01T16:49:48Z Radioseismology is based on registration and interpretation of radio emission of seismic origin. Non-thermal radio emission of the Moon was detectedat 13 and 21 cm on July 30 - August 2, 1999. Strong oscillations of the non-thermal lunar radio flux at 25 mm were detected during the leonid meteor shower on November 17-18, 2000. The time of maxima of oscillations does not contradict theoretical predictions about the existence of three maxima of the Leonid shower on the Moon. These results can be explained as the detection of lunar radio emission of seismic origin caused by meteoroid impacts. The implications of the radioseismic method for determination of the intensity of meteor streams on the Moon are described. : Proceeding of the Meteoroids 2001 conference, Kiruna, Sweden, August 6-10, 2001, in press Report Kiruna DataCite Metadata Store (German National Library of Science and Technology) Kiruna |
institution |
Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
unknown |
topic |
Astrophysics astro-ph Geophysics physics.geo-ph FOS Physical sciences |
spellingShingle |
Astrophysics astro-ph Geophysics physics.geo-ph FOS Physical sciences Berezhnoi, A. A. Bervalds, E. Khavroshkin, O. B. Ozolins, G. Radioseismology as a new method of investigations of meteor streams on the Moon and planets |
topic_facet |
Astrophysics astro-ph Geophysics physics.geo-ph FOS Physical sciences |
description |
Radioseismology is based on registration and interpretation of radio emission of seismic origin. Non-thermal radio emission of the Moon was detectedat 13 and 21 cm on July 30 - August 2, 1999. Strong oscillations of the non-thermal lunar radio flux at 25 mm were detected during the leonid meteor shower on November 17-18, 2000. The time of maxima of oscillations does not contradict theoretical predictions about the existence of three maxima of the Leonid shower on the Moon. These results can be explained as the detection of lunar radio emission of seismic origin caused by meteoroid impacts. The implications of the radioseismic method for determination of the intensity of meteor streams on the Moon are described. : Proceeding of the Meteoroids 2001 conference, Kiruna, Sweden, August 6-10, 2001, in press |
format |
Report |
author |
Berezhnoi, A. A. Bervalds, E. Khavroshkin, O. B. Ozolins, G. |
author_facet |
Berezhnoi, A. A. Bervalds, E. Khavroshkin, O. B. Ozolins, G. |
author_sort |
Berezhnoi, A. A. |
title |
Radioseismology as a new method of investigations of meteor streams on the Moon and planets |
title_short |
Radioseismology as a new method of investigations of meteor streams on the Moon and planets |
title_full |
Radioseismology as a new method of investigations of meteor streams on the Moon and planets |
title_fullStr |
Radioseismology as a new method of investigations of meteor streams on the Moon and planets |
title_full_unstemmed |
Radioseismology as a new method of investigations of meteor streams on the Moon and planets |
title_sort |
radioseismology as a new method of investigations of meteor streams on the moon and planets |
publisher |
arXiv |
publishDate |
2001 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0112498 https://arxiv.org/abs/astro-ph/0112498 |
geographic |
Kiruna |
geographic_facet |
Kiruna |
genre |
Kiruna |
genre_facet |
Kiruna |
op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
op_doi |
https://doi.org/10.48550/arxiv.astro-ph/0112498 |
_version_ |
1766058268800581632 |