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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Published in:Advances in Astronomy and Space Physics
Date:2012
Main Authors: Allawi, H., Pohjolainen, S.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2012
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/119190
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this: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.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Allawi, H.
Pohjolainen, S.
author_facet Allawi, H.
Pohjolainen, S.
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.
collection DSpace DC
container_title Advances in Astronomy and Space Physics
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.
first_indexed 2025-12-07T17:49:25Z
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institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
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language English
last_indexed 2025-12-07T17:49:25Z
publishDate 2012
publisher Головна астрономічна обсерваторія НАН України
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spelling Allawi, H.
Pohjolainen, S.
2017-06-04T19:39:25Z
2017-06-04T19:39:25Z
2012
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
https://nasplib.isofts.kiev.ua/handle/123456789/119190
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.
The data used in this work were obtained from the web archives of the LASCO CME Catalog (generated and maintained at the CDAW Data Center by NASA and The Catholic University of America in cooperation with the Naval Research Laboratory) and the Wind WAVES instrument website.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
The energy sources of CME acceleration
Article
published earlier
spellingShingle The energy sources of CME acceleration
Allawi, H.
Pohjolainen, S.
title 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_short The energy sources of CME acceleration
title_sort energy sources of cme acceleration
url https://nasplib.isofts.kiev.ua/handle/123456789/119190
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AT pohjolainens theenergysourcesofcmeacceleration
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