KFU. Card publication. Comparison of the Structures of Meteor Streams of Cometary and Possible Asteroidal Origin

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FEDERAL UNIVERSITY

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COMPARISON OF THE STRUCTURES OF METEOR STREAMS OF COMETARY AND POSSIBLE ASTEROIDAL ORIGIN

Form of presentation

Articles in international journals and collections

Year of publication

2018

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Authors, employees of KFU

Sergienko Mariya Viktorovna, author

Sokolova Marina Gennadevna, author

Bibliographic description in the original language

Sokolova M. G. Comparison of the Structures of Meteor Streams of Cometary and Possible Asteroidal Origin / M. G. Sokolova, M. V. Sergienko // Solar System Research, 2016, Vol. 50, No. 6, pp. 379–389.

Annotation

The structures of the meteor streams of cometary origin—Draconids, Ursids, Perseids, and Lyrids— and the streams presumably connected with asteroids—Taurids and α-Capricornids—are compared. The comparative analysis was performed by the mass distribution of meteoroids in the stream and the activity profile for the meteors with the maximum recorded stellar magnitude +3m and brighter. Visual observations of 1987–2008 from the database of the International Meteor Organization (IMO) and earlier sources were considered. It has been shown that the structures of the meteor streams of cometary and, presumably, asteroidal origin differ somewhat by the activity profile and the mass distribution of meteoroids in the cross-section of a stream along the Earth's orbit.

Keywords

meteoroid, meteor, meteor stream, comet, asteroid

The name of the journal

SOLAR SYST RES+

Please use this ID to quote from or refer to the card

https://repository.kpfu.ru/eng/?p_id=191760&p_lang=2

Full metadata record

Field DC	Value	Language
dc.contributor.author	Sergienko Mariya Viktorovna	ru_RU
dc.contributor.author	Sokolova Marina Gennadevna	ru_RU
dc.date.accessioned	2018-01-01T00:00:00Z	ru_RU
dc.date.available	2018-01-01T00:00:00Z	ru_RU
dc.date.issued	2018	ru_RU
dc.identifier.citation	Sokolova M. G. Comparison of the Structures of Meteor Streams of Cometary and Possible Asteroidal Origin / M. G. Sokolova, M. V. Sergienko // Solar System Research, 2016, Vol. 50, No. 6, pp. 379–389.	ru_RU
dc.identifier.uri	https://repository.kpfu.ru/eng/?p_id=191760&p_lang=2	ru_RU
dc.description.abstract	SOLAR SYST RES+	ru_RU
dc.description.abstract	The structures of the meteor streams of cometary origin—Draconids, Ursids, Perseids, and Lyrids— and the streams presumably connected with asteroids—Taurids and α-Capricornids—are compared. The comparative analysis was performed by the mass distribution of meteoroids in the stream and the activity profile for the meteors with the maximum recorded stellar magnitude +3m and brighter. Visual observations of 1987–2008 from the database of the International Meteor Organization (IMO) and earlier sources were considered. It has been shown that the structures of the meteor streams of cometary and, presumably, asteroidal origin differ somewhat by the activity profile and the mass distribution of meteoroids in the cross-section of a stream along the Earth's orbit.	ru_RU
dc.language.iso	ru	ru_RU
dc.subject	meteoroid	ru_RU
dc.subject	meteor	ru_RU
dc.subject	meteor stream	ru_RU
dc.subject	comet	ru_RU
dc.subject	asteroid	ru_RU
dc.title	Comparison of the Structures of Meteor Streams of Cometary and Possible Asteroidal Origin	ru_RU
dc.type	Articles in international journals and collections	ru_RU