The energy sources of CME acceleration

We investigate the possibility that during the fast acceleration phase of a coronal mass ejection (CME), a freely propagating shock wave could be launched. We test this hypothesis by calculating the speeds of blast waves by using the Taylor-Sedov equation in changing density solar atmosphere, and co...

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Збережено в:
Бібліографічні деталі
Дата:2012
Автори: Allawi, H., Pohjolainen, S.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2012
Назва видання:Advances in Astronomy and Space Physics
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/119190
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:The energy sources of CME acceleration / H. Allawi, S. Pohjolainen // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 157-160. — Бібліогр.: 14 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
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spelling irk-123456789-1191902017-06-05T03:04:00Z The energy sources of CME acceleration Allawi, H. Pohjolainen, S. We investigate the possibility that during the fast acceleration phase of a coronal mass ejection (CME), a freely propagating shock wave could be launched. We test this hypothesis by calculating the speeds of blast waves by using the Taylor-Sedov equation in changing density solar atmosphere, and compare these speeds with the radio type II burst speeds during the CME event on 17 February 2000. The matching speeds and the realistic value of the blast wave energy, 10²⁴ J, lead us to suggest that the CME acceleration phase may involve shocks separating from the initial CME driver. 2012 Article The energy sources of CME acceleration / H. Allawi, S. Pohjolainen // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 157-160. — Бібліогр.: 14 назв. — англ. 2227-1481 http://dspace.nbuv.gov.ua/handle/123456789/119190 en Advances in Astronomy and Space Physics Головна астрономічна обсерваторія НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
description We investigate the possibility that during the fast acceleration phase of a coronal mass ejection (CME), a freely propagating shock wave could be launched. We test this hypothesis by calculating the speeds of blast waves by using the Taylor-Sedov equation in changing density solar atmosphere, and compare these speeds with the radio type II burst speeds during the CME event on 17 February 2000. The matching speeds and the realistic value of the blast wave energy, 10²⁴ J, lead us to suggest that the CME acceleration phase may involve shocks separating from the initial CME driver.
format Article
author Allawi, H.
Pohjolainen, S.
spellingShingle Allawi, H.
Pohjolainen, S.
The energy sources of CME acceleration
Advances in Astronomy and Space Physics
author_facet Allawi, H.
Pohjolainen, S.
author_sort Allawi, H.
title The energy sources of CME acceleration
title_short The energy sources of CME acceleration
title_full The energy sources of CME acceleration
title_fullStr The energy sources of CME acceleration
title_full_unstemmed The energy sources of CME acceleration
title_sort energy sources of cme acceleration
publisher Головна астрономічна обсерваторія НАН України
publishDate 2012
url http://dspace.nbuv.gov.ua/handle/123456789/119190
citation_txt The energy sources of CME acceleration / H. Allawi, S. Pohjolainen // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 157-160. — Бібліогр.: 14 назв. — англ.
series Advances in Astronomy and Space Physics
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first_indexed 2023-10-18T20:33:58Z
last_indexed 2023-10-18T20:33:58Z
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