scholarly journals RELATIONSHIP OF EUV IRRADIANCE CORONAL DIMMING SLOPE AND DEPTH TO CORONAL MASS EJECTION SPEED AND MASS

2016 ◽  
Vol 830 (1) ◽  
pp. 20 ◽  
Author(s):  
James Paul Mason ◽  
Thomas N. Woods ◽  
David F. Webb ◽  
Barbara J. Thompson ◽  
Robin C. Colaninno ◽  
...  
1990 ◽  
Vol 142 ◽  
pp. 450-451
Author(s):  
V K Verma

We present an analysis of the relationship between coronal mass ejection (CME) events with solar flares and coronal holes. Out of 79 CME events whose location and span are known, 10 CME event circles contain solar flares. On the other hand out of 71 CME events (selected for the study with coronal holes) 40 CME event circles contain coronal holes. We have examined the above associations by calculating the Yule's coefficients of association and found that the CME events and solar flares are statistically not associated while CME events and coronal holes are statistically associated. This does not necessarily indicate that CMEs come from coronal holes as claimed by Hewish and Bravo (1986).


Solar Physics ◽  
2004 ◽  
Vol 219 (2) ◽  
pp. 315-342 ◽  
Author(s):  
Timothy A. Howard ◽  
Richard A. Harrison

2008 ◽  
Vol 4 (T27A) ◽  
pp. 79-103
Author(s):  
James A. Klimchuk ◽  
Lidia van Driel-Gesztelyi ◽  
Carolus J. Schrijver ◽  
Donald B. Melrose ◽  
Lyndsay Fletcher ◽  
...  

Commission 10 deals with solar activity in all of its forms, ranging from the smallest nanoflares to the largest coronal mass ejections. This report reviews scientific progress over the roughly two-year period ending in the middle of 2008. This has been an exciting time in solar physics, highlighted by the launches of the Hinode and STEREO missions late in 2006. The report is reasonably comprehensive, though it is far from exhaustive. Limited space prevents the inclusion of many significant results. The report is divided into the following sections: Photosphere and chromosphere; Transition region; Corona and coronal heating; Coronal jets; flares; Coronal mass ejection initiation; Global coronal waves and shocks; Coronal dimming; The link between low coronal CME signatures and magnetic clouds; Coronal mass ejections in the heliosphere; and Coronal mass ejections and space weather. Primary authorship is indicated at the beginning of each section.


2007 ◽  
Vol 59 (sp3) ◽  
pp. S801-S806 ◽  
Author(s):  
Louise K. Harra ◽  
Hirohisa Hara ◽  
Shinsuke Imada ◽  
Peter R. Young ◽  
David R. Williams ◽  
...  

2008 ◽  
Vol 4 (S257) ◽  
pp. 191-200
Author(s):  
Richard Harrison

AbstractCoronal Mass Ejections (CMEs) have been addressed by a particularly active research community in recent years. With the advent of the International Heliophysical Year and the new STEREO and Hinode missions, in addition to the on-going SOHO mission, CME research has taken centre stage in a renewed international effort. This review aims to touch on some key observational areas, and their interpretation. First, we consider coronal dimming, which has become synonymous with CME onsets, and stress that recent advances have heralded a move from a perceived association between the two phenomena to a firm, well-defined physical link. What this means for our understanding of CME modeling is discussed. Second, with the new STEREO observations, and noting the on-going SMEI observations, it is important to review the opening field of CME studies in the heliosphere. Finally, we discuss some specific points with regard to EIT-waves and the flare-CME relationship. In the opinion of the author, these issues cover key hot topics which need consideration for significant progress in the field.


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