Sporadic solar radio emission at decameter wavelengths

Sporadic solar radio emission at decameter wavelengths

Results of observations of the solar sporadic radio emission in decameter range are presented. These observations were carried out at UTR-2 radio telescope with 60-channel spectrometer and DSP (Digital Spectral Polarimeter) last years. Particular attention is devoted to such components of sporadic r...

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Збережено в:
Бібліографічні деталі
Дата:2005
Автори: Mel'nik, V.N., Konovalenko, A.A., Abranin, E.P., Dorovsky, V.V., Lisachenko, V.N., Stanislavsky, A.A., Rucker, H.O., Lecacheux, A.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2005
Назва видання:Кинематика и физика небесных тел
Теми:
MS1: Decameter Radioastronomy
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/79604
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Sporadic solar radio emission at decameter wavelengths / V.N. Mel'nik, A.A. Konovalenko, E.P. Abranin, V.V. Dorovsky, V.N. Lisachenko, A.A. Stanislavsky, H.O. Rucker, A. Lecacheux // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 61-66. — Бібліогр.: 6 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id irk-123456789-79604
record_format dspace
spelling irk-123456789-796042015-04-04T03:01:33Z Sporadic solar radio emission at decameter wavelengths Mel'nik, V.N. Konovalenko, A.A. Abranin, E.P. Dorovsky, V.V. Lisachenko, V.N. Stanislavsky, A.A. Rucker, H.O. Lecacheux, A. MS1: Decameter Radioastronomy Results of observations of the solar sporadic radio emission in decameter range are presented. These observations were carried out at UTR-2 radio telescope with 60-channel spectrometer and DSP (Digital Spectral Polarimeter) last years. Particular attention is devoted to such components of sporadic radio emission as Type III bursts, Type II bursts, “drift pair” bursts. New properties of these bursts, which distinguished for decameter band, are noted. They are as follows: – fine structure of Type III bursts unobserved before at other frequencies; – first discovered fine structure of Type II bursts in the form of small duration sub bursts with positive and negative frequency drift; – wavelike movement of Type II burst backbone with herringbone structure; – difference of frequency drift rates of “drift pair” bursts with positive and negative rates. 2005 Article Sporadic solar radio emission at decameter wavelengths / V.N. Mel'nik, A.A. Konovalenko, E.P. Abranin, V.V. Dorovsky, V.N. Lisachenko, A.A. Stanislavsky, H.O. Rucker, A. Lecacheux // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 61-66. — Бібліогр.: 6 назв. — англ. 0233-7665 http://dspace.nbuv.gov.ua/handle/123456789/79604 en Кинематика и физика небесных тел Головна астрономічна обсерваторія НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
topic MS1: Decameter Radioastronomy
MS1: Decameter Radioastronomy
spellingShingle MS1: Decameter Radioastronomy
MS1: Decameter Radioastronomy
Mel'nik, V.N.
Konovalenko, A.A.
Abranin, E.P.
Dorovsky, V.V.
Lisachenko, V.N.
Stanislavsky, A.A.
Rucker, H.O.
Lecacheux, A.
Sporadic solar radio emission at decameter wavelengths
Кинематика и физика небесных тел
description Results of observations of the solar sporadic radio emission in decameter range are presented. These observations were carried out at UTR-2 radio telescope with 60-channel spectrometer and DSP (Digital Spectral Polarimeter) last years. Particular attention is devoted to such components of sporadic radio emission as Type III bursts, Type II bursts, “drift pair” bursts. New properties of these bursts, which distinguished for decameter band, are noted. They are as follows: – fine structure of Type III bursts unobserved before at other frequencies; – first discovered fine structure of Type II bursts in the form of small duration sub bursts with positive and negative frequency drift; – wavelike movement of Type II burst backbone with herringbone structure; – difference of frequency drift rates of “drift pair” bursts with positive and negative rates.
format Article
author Mel'nik, V.N.
Konovalenko, A.A.
Abranin, E.P.
Dorovsky, V.V.
Lisachenko, V.N.
Stanislavsky, A.A.
Rucker, H.O.
Lecacheux, A.
author_facet Mel'nik, V.N.
Konovalenko, A.A.
Abranin, E.P.
Dorovsky, V.V.
Lisachenko, V.N.
Stanislavsky, A.A.
Rucker, H.O.
Lecacheux, A.
author_sort Mel'nik, V.N.
title Sporadic solar radio emission at decameter wavelengths
title_short Sporadic solar radio emission at decameter wavelengths
title_full Sporadic solar radio emission at decameter wavelengths
title_fullStr Sporadic solar radio emission at decameter wavelengths
title_full_unstemmed Sporadic solar radio emission at decameter wavelengths
title_sort sporadic solar radio emission at decameter wavelengths
publisher Головна астрономічна обсерваторія НАН України
publishDate 2005
topic_facet MS1: Decameter Radioastronomy
url http://dspace.nbuv.gov.ua/handle/123456789/79604
citation_txt Sporadic solar radio emission at decameter wavelengths / V.N. Mel'nik, A.A. Konovalenko, E.P. Abranin, V.V. Dorovsky, V.N. Lisachenko, A.A. Stanislavsky, H.O. Rucker, A. Lecacheux // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 61-66. — Бібліогр.: 6 назв. — англ.
series Кинематика и физика небесных тел
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first_indexed 2023-10-18T19:19:04Z
last_indexed 2023-10-18T19:19:04Z
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