The Amplitude of Sunspot Minimum as a Favorable Precursor for the Prediction of the Amplitude of the Next Solar Maximum and the Limit of the Waldmeier Effect

Solar Physics ◽  
2011 ◽  
Vol 276 (1-2) ◽  
pp. 395-406 ◽  
Author(s):  
K. B. Ramesh ◽  
N. Bhagya Lakshmi
Keyword(s):  
Solar Maximum ◽  
Sunspot Minimum

Coronal Mass Ejections and Solar Filament Disappearances at Solar Maximum

1994 ◽  
Vol 144 ◽  
pp. 127-129
Author(s):  
S. Dinulescu ◽  
G. Maris
Keyword(s):  
Coronal Mass Ejections ◽  
Solar Maximum ◽  
Solar Filament

AbstractOccurrence of CMEs as a result of solar filament disappearance is discussed over the cycle 22.

Correction [to “Solar wind and location of shock front and magnetopause at the 1969 Solar Maximum”]

1971 ◽  
Vol 76 (13) ◽  
pp. 3178-3178
Author(s):  
A. Egidi ◽  
V. Formisiano ◽  
F. Palmiotto ◽  
P. Saraceno ◽  
G. Moreno
Keyword(s):  
Solar Wind ◽  
Shock Front ◽  
Solar Maximum

Flux and Energy Spectrum of Cosmic-RayαParticles during Solar Maximum

1959 ◽  
Vol 114 (1) ◽  
pp. 365-373 ◽  
Author(s):  
P. S. Freier ◽  
E. P. Ney ◽  
C. J. Waddington
Keyword(s):  
Energy Spectrum ◽  
Solar Maximum

Solar wind and coronal structure near sunspot minimum: Pioneer and SMM observations from 1985–1987

1990 ◽  
Vol 95 (A6) ◽  
pp. 8231 ◽  
Author(s):  
J. D. Mihalov ◽  
A. Barnes ◽  
A. J. Hundhausen ◽  
E. J. Smith
Keyword(s):  
Solar Wind ◽  
Coronal Structure ◽  
Sunspot Minimum
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