scholarly journals The solar origin of the January 1997 coronal mass ejection, magnetic cloud and geomagnetic storm

1998 ◽  
Vol 25 (14) ◽  
pp. 2469-2472 ◽  
Author(s):  
D. F. Webb ◽  
E. W. Cliver ◽  
N. Gopalswamy ◽  
H. S. Hudson ◽  
O. C. St. Cyr
1996 ◽  
Vol 154 ◽  
pp. 187-193
Author(s):  
Rainer Schwenn

AbstractIn the field of solar-terrestrial relations a clear and unique terminology is needed in order to abolish and avoid unnecessary confusion between the scientists from several involved disciplines. For example, the widely used abbreviation CME (for coronal mass ejection) has turned out to be somewhat misleading. Early on it had been known that other than coronal material is often involved in such events. The discoverers observed transient events of mass ejections from the sun, which could be observed in the corona owing to the newly available coronagraphs. This article is meant to clarify the terminology, with emphasis on giving credit to the original discoverers and the terms they introduced. With this aim in mind I suggest some minor modifications of the terminology.


2018 ◽  
Vol 10 (2) ◽  
pp. 133-144
Author(s):  
S. Bhardwaj ◽  
P. A. Khan ◽  
R. Atulkar ◽  
P. K. Purohit

 The fluctuations in the Interplanetary Magnetic Field significantly affect the state of geomagnetic field particularly during the Coronal Mass Ejection (CME) events. In the present investigation we have studied the influence of Interplanetary Magnetic Field changes on the geomagnetic field components at high, low and mid latitudes. To carry out this investigation we have selected three stations viz. Alibag (18.6°N, 72.7°E), Beijing MT (40.3°N, 116.2°E) and Casey (66.2°S, 110.5°E) one each in the low, mid and high latitude regions. Then we selected geomagnetic storm events of three types namely weak (-50≤Dst≤-20), moderate (100≤Dst≤-50) and intense (Dst≤-100nT). In each storm category 10 events were considered. From our study we conclude that geomagnetic field components are significantly affected by the changes in the IMF at all the three latitudinal regions during all the storm events. At the same time we also found that the magnitude of change in geomagnetic field components is highest at the high latitudes during all types of storm events while at low and mid latitude stations the magnitude of effect is approximately the same.


Solar Physics ◽  
2014 ◽  
Vol 289 (11) ◽  
pp. 4173-4208 ◽  
Author(s):  
D. F. Webb ◽  
M. M. Bisi ◽  
C. A. de Koning ◽  
C. J. Farrugia ◽  
B. V. Jackson ◽  
...  

1982 ◽  
Vol 9 (12) ◽  
pp. 1317-1320 ◽  
Author(s):  
L. F. Burlaga ◽  
L. Klein ◽  
N. R. Sheeley ◽  
D. J. Michels ◽  
R. A. Howard ◽  
...  

1999 ◽  
Vol 104 (A11) ◽  
pp. 24885-24894 ◽  
Author(s):  
S. G. Kanekal ◽  
D. N. Baker ◽  
J. B. Blake ◽  
B. Klecker ◽  
R. A. Mewaldt ◽  
...  

Space Weather ◽  
2014 ◽  
Vol 12 (4) ◽  
pp. 246-256 ◽  
Author(s):  
R.‐S. Kim ◽  
Y.‐J. Moon ◽  
N. Gopalswamy ◽  
Y.‐D. Park ◽  
Y.‐H. Kim

2010 ◽  
Vol 115 (A8) ◽  
pp. n/a-n/a ◽  
Author(s):  
Susan McKenna-Lawlor ◽  
Lu Li ◽  
Iannis Dandouras ◽  
Pontus C. Brandt ◽  
Yihua Zheng ◽  
...  

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