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International Letters of Chemistry, Physics and Astronomy
Volume 33

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The Propagation of an Impulsive Coronal Mass Ejections (CMEs) due to the High Solar Flares and Moreton Waves

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Abstract:

This paper provides a short review of some of the basic concepts related to the origin of Coronal Mass Ejections (CMEs). The numerous ideas which have been put forward to elucidate the initiation of CMEs are categorized in terms of whether this event is a gradual CME or impulsive CME. In this case, an earth-directed Coronal Mass Ejection (CME) was observed on April 2, 2014 by the Large Angle Spectrometric Coronagraph (LASCO) C2. This recent observations obtained a large impulsive CMEs. The CME, originating from the active region AR2027. The speed of CMEs is 1600 kms-1. A halo CME, a bright expanding ring at the North- West region is exploded beginning at about 14:36 UT, and the process of departing, expansion and propagation are highlighted. We discuss the correspondence of this event with the structure of the CME in the LASCO data. It is believed that the high solar flare and a Moreton waves initiate this kind of CMEs

Info:

Periodical:
International Letters of Chemistry, Physics and Astronomy (Volume 33)
Pages:
118-126
Citation:
Z. S. Hamidi and N.N.M. Shariff, "The Propagation of an Impulsive Coronal Mass Ejections (CMEs) due to the High Solar Flares and Moreton Waves", International Letters of Chemistry, Physics and Astronomy, Vol. 33, pp. 118-126, 2014
Online since:
May 2014
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Cited By:

[1] M. Batubara, T. Manik, R. Suryana, M. Lathif, P. Sitompul, M. Zamzam, F. Mumtahana, "Solar Radio Burst Data Processing of CALLISTO and Frequency Drift Rate Determination of Solar Radio Burst Detected by CALLISTO Network in Indonesia", IOP Conference Series: Materials Science and Engineering, Vol. 180, p. 012049, 2017

DOI: https://doi.org/10.1088/1757-899X/180/1/012049