КФУ. Карточка публикации. Comparison of the Structures of Meteor Streams of Cometary and Possible Asteroidal Origin

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

Форма представления

Статьи в зарубежных журналах и сборниках

Год публикации

2018

Язык

русский

Авторы, сотрудники КФУ

Сергиенко Мария Викторовна, автор

Соколова Марина Геннадьевна, автор

Библиографическое описание на языке оригинала

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.

Аннотация

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.

Ключевые слова

meteoroid, meteor, meteor stream, comet, asteroid

Название журнала

SOLAR SYST RES+

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https://repository.kpfu.ru/?p_id=191760

Полная запись метаданных

Поле DC	Значение	Язык
dc.contributor.author	Сергиенко Мария Викторовна	ru_RU
dc.contributor.author	Соколова Марина Геннадьевна	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/?p_id=191760	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	Статьи в зарубежных журналах и сборниках	ru_RU