КФУ. Карточка публикации. The δ-Cancrids Meteor Complex

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THE δ-CANCRIDS METEOR COMPLEX

Форма представления

Статьи в зарубежных журналах и сборниках

Год публикации

2022

Язык

английский

Авторы, сотрудники КФУ

Соколова Марина Геннадьевна, автор

Усанин Владимир Сергеевич, автор

Библиографическое описание на языке оригинала

Sokolova M.G, Usanin V.S., The δ-Cancrids Meteor Complex//Solar System Research. - 2022. - Vol.56, Is.1. - P.54-61.

Аннотация

In studying the connections of the δ-Cancrids (DCA) meteor stream, consisting of the northern (NCC) and southern (SCC) branches, with the comet–asteroid complex, the structure of the shower was studied using visual and television observations. According to visual observations, it was found that for meteors with a minimum recorded stellar magnitude of +3m and brighter, the maximum of activity ZHR = 8.6 +/- 1.8 is observed at the Sun's longitude 298.5 degrees +/- 1.2 degrees, while the parameter r of the luminosity function during the period of the shower activity varies in the range of 1.5–2.0. For meteors weaker than +3m, the moment of maximum occurs 1.4 degrees later than for brighter meteors. For the orbits of meteors of the NCC and SCC branches, obtained from television observations, the dependence of the values of the semimajor axes and eccentricities on the mass of meteoroids was also revealed. The orbit separation time for the δ-Cancrid meteors in the meteor magnitude range from 0m to +3m due to the nongravitational Poynting–Robertson effect is 22–26 thousand years for the southern branch SCC, and 24–29 thousand years for the northern branch NCC.

Ключевые слова

meteoroid, meteor, meteor shower, comet

Название журнала

Solar System Research

URL

https://link.springer.com/article/10.1134/S0038094622010063

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https://repository.kpfu.ru/?p_id=264295

Полная запись метаданных

Поле DC	Значение	Язык
dc.contributor.author	Соколова Марина Геннадьевна	ru_RU
dc.contributor.author	Усанин Владимир Сергеевич	ru_RU
dc.date.accessioned	2022-01-01T00:00:00Z	ru_RU
dc.date.available	2022-01-01T00:00:00Z	ru_RU
dc.date.issued	2022	ru_RU
dc.identifier.citation	Sokolova M.G, Usanin V.S., The δ-Cancrids Meteor Complex//Solar System Research. - 2022. - Vol.56, Is.1. - P.54-61.	ru_RU
dc.identifier.uri	https://repository.kpfu.ru/?p_id=264295	ru_RU
dc.description.abstract	Solar System Research	ru_RU
dc.description.abstract	In studying the connections of the δ-Cancrids (DCA) meteor stream, consisting of the northern (NCC) and southern (SCC) branches, with the comet–asteroid complex, the structure of the shower was studied using visual and television observations. According to visual observations, it was found that for meteors with a minimum recorded stellar magnitude of +3m and brighter, the maximum of activity ZHR = 8.6 +/- 1.8 is observed at the Sun's longitude 298.5 degrees +/- 1.2 degrees, while the parameter r of the luminosity function during the period of the shower activity varies in the range of 1.5–2.0. For meteors weaker than +3m, the moment of maximum occurs 1.4 degrees later than for brighter meteors. For the orbits of meteors of the NCC and SCC branches, obtained from television observations, the dependence of the values of the semimajor axes and eccentricities on the mass of meteoroids was also revealed. The orbit separation time for the δ-Cancrid meteors in the meteor magnitude range from 0m to +3m due to the nongravitational Poynting–Robertson effect is 22–26 thousand years for the southern branch SCC, and 24–29 thousand years for the northern branch NCC.	ru_RU
dc.language.iso	ru	ru_RU
dc.subject	meteoroid	ru_RU
dc.subject	meteor	ru_RU
dc.subject	meteor shower	ru_RU
dc.subject	comet	ru_RU
dc.title	The δ-Cancrids Meteor Complex	ru_RU
dc.type	Статьи в зарубежных журналах и сборниках	ru_RU