Magnetic Cloud and Its Interplanetary Shock Sheath as a Modulator of the Cosmic Ray Intensity

Forbush Decreases (FDs) are representative events of abrupt decrease in galactic cosmic ray intensity. They are known to be strongly associated with solar wind events such as interplanetary shock (IP shock) and magnetic cloud (MC). In order to examine effectiveness of the MC on FDs, I studied the 44...

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Main Author: Su Yeon Oh
Format: Article
Language:English
Published: The Korean Space Science Society 2008-06-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2008/v25n2/OJOOBS_2008_v25n2_149.pdf
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author Su Yeon Oh
author_facet Su Yeon Oh
author_sort Su Yeon Oh
collection DOAJ
description Forbush Decreases (FDs) are representative events of abrupt decrease in galactic cosmic ray intensity. They are known to be strongly associated with solar wind events such as interplanetary shock (IP shock) and magnetic cloud (MC). In order to examine effectiveness of the MC on FDs, I studied the 44 MCs that occurred during the 2 years from 1998 to 1999 and investigated the properties of interplanetary magnetic field (IMF) and solar wind. As a result, I found that 11 out of 44 MCs are associated with the FDs. In particularly, it is noted that the FDs are driven by the IP shock sheaths which are associated with over 13 nT of IMF magnitude, 3 nT of IMF turbulence, and 550 km/s of solar wind speed. This result indicates that magnetic cloud and its interplanetary shock sheath work as a modulator of the cosmic ray intensity.
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spelling doaj.art-b473f58848964a31be50281b545c53bd2024-01-02T05:05:40ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092008-06-0125214915610.5140/JASS.2008.25.2.149Magnetic Cloud and Its Interplanetary Shock Sheath as a Modulator of the Cosmic Ray IntensitySu Yeon Oh0Dept. of Astronomy and Space Science, Chungnam University, Daejeon 305-764, Korea Forbush Decreases (FDs) are representative events of abrupt decrease in galactic cosmic ray intensity. They are known to be strongly associated with solar wind events such as interplanetary shock (IP shock) and magnetic cloud (MC). In order to examine effectiveness of the MC on FDs, I studied the 44 MCs that occurred during the 2 years from 1998 to 1999 and investigated the properties of interplanetary magnetic field (IMF) and solar wind. As a result, I found that 11 out of 44 MCs are associated with the FDs. In particularly, it is noted that the FDs are driven by the IP shock sheaths which are associated with over 13 nT of IMF magnitude, 3 nT of IMF turbulence, and 550 km/s of solar wind speed. This result indicates that magnetic cloud and its interplanetary shock sheath work as a modulator of the cosmic ray intensity.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2008/v25n2/OJOOBS_2008_v25n2_149.pdfForbush DecreaseCosmic rayMagnetic cloudInterplanetary shock
spellingShingle Su Yeon Oh
Magnetic Cloud and Its Interplanetary Shock Sheath as a Modulator of the Cosmic Ray Intensity
Journal of Astronomy and Space Sciences
Forbush Decrease
Cosmic ray
Magnetic cloud
Interplanetary shock
title Magnetic Cloud and Its Interplanetary Shock Sheath as a Modulator of the Cosmic Ray Intensity
title_full Magnetic Cloud and Its Interplanetary Shock Sheath as a Modulator of the Cosmic Ray Intensity
title_fullStr Magnetic Cloud and Its Interplanetary Shock Sheath as a Modulator of the Cosmic Ray Intensity
title_full_unstemmed Magnetic Cloud and Its Interplanetary Shock Sheath as a Modulator of the Cosmic Ray Intensity
title_short Magnetic Cloud and Its Interplanetary Shock Sheath as a Modulator of the Cosmic Ray Intensity
title_sort magnetic cloud and its interplanetary shock sheath as a modulator of the cosmic ray intensity
topic Forbush Decrease
Cosmic ray
Magnetic cloud
Interplanetary shock
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2008/v25n2/OJOOBS_2008_v25n2_149.pdf
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