Intermediate degree p-mode frequency splittings near solar maximum

Solar Physics ◽  
1994 ◽  
Vol 149 (1) ◽  
pp. 1-21 ◽  
Author(s):  
R. S. Ronan ◽  
B. J. Labonte
Keyword(s):  
Solar Maximum ◽  
Mode Frequency ◽  
Intermediate Degree

Confirmation of solar cycle-dependent intermediate-degree p-mode frequency shifts

1993 ◽  
Vol 406 ◽  
pp. 714 ◽  
Author(s):  
Edward J., Jr. Rhodes ◽  
Alessandro Cacciani ◽  
Sylvain G. Korzennik ◽  
Roger K. Ulrich
Keyword(s):  
Solar Cycle ◽  
Mode Frequency ◽  
Frequency Shifts ◽  
Intermediate Degree ◽  
Cycle Dependent

Observation of Hysteresis between Solar Activity Indicators and p-mode Frequency Shifts for Solar Cycle 22

2000 ◽  
Vol 179 ◽  
pp. 357-360
Author(s):  
S. C. Tripathy ◽  
Brajesh Kumar ◽  
Kiran Jain ◽  
A. Bhatnagar
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
Magnetic Activity ◽  
Mode Frequency ◽  
Hysteresis Phenomenon ◽  
Data Sets ◽  
Frequency Data ◽  
Frequency Shifts ◽  
Intermediate Degree

AbstractUsing intermediate degreep-mode frequency data sets for solar cycle 22, we find that the frequency shifts and magnetic activity indicators show a “hysteresis” phenomenon. It is observed that the magnetic indices follow different paths for the ascending and descending phases of the solar cycle while for radiative indices, the separation between the paths are well within the error limits.

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.

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