Calculated Coronal Magnetic Fields and Their Comparison with the Coronal Structures as Observed during Five Solar Eclipses
1994 ◽
Vol 144
◽
pp. 559-564
Keyword(s):
AbstractWe were successful in observing the solar corona during five solar eclipses (1973-1991). For the eclipse days the coronal magnetic field was calculated by extrapolation from the photosphere. Comparison of the observed and calculated coronal structures is carried out and some peculiarities of this comparison, related to the different phases of the solar cycle, are presented.
Keyword(s):
1994 ◽
Vol 144
◽
pp. 21-28
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Keyword(s):
2003 ◽
Vol 10
(4/5)
◽
pp. 313-322
◽
2013 ◽
Vol 8
(S300)
◽
pp. 139-146
◽
1968 ◽
Vol 35
◽
pp. 379-384
◽
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Keyword(s):
1993 ◽
Vol 141
◽
pp. 302-305
◽
1994 ◽
Vol 144
◽
pp. 29-33
2015 ◽
Vol 11
(S320)
◽
pp. 167-174
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