Time-Latitudinal Dynamics of Magnetic Fields and the Green Corona Over Three Solar Cycles

[1]  J. Pasachoff,et al.  The April 8, 2005, Eclipse White-Light Corona , 2006 .

[2]  R. Altrock.  The Temperature of the Low Corona During Solar Cycles 21–23 , 2004 .

[3]  E. Cliver,et al.  Reexamination of the coronal index of solar activity before the year 1965 , 2003 .

[4]  L. Gizon,et al.  A New Component of Solar Dynamics: North-South Diverging Flows Migrating toward the Equator with an 11 Year Period , 2002 .

[5]  V. Rušin,et al.  The Green Corona and Magnetic Fields , 2002 .

[6]  J. T. Hoeksema,et al.  Polar Plume Anatomy: Results of a Coordinated Observation , 1997 .

[7]  R. Altrock.  AN ‘EXTENDED SOLAR CYCLE’ AS OBSERVED IN Fe XIV , 1997 .

[8]  D. Hathaway.  Doppler Measurements of the Suns Meridional Flow , 1996 .

[9]  V. Makarov,et al.  New results concerning the global solar cycle , 1989 .

[10]  P. R. Wilson,et al.  The extended solar activity cycle , 1988, Nature.

[11]  V. I. Makarov,et al.  Poleward migration of the magnetic neutral line and the reversal of the polar fields on the Sun , 1983 .

[12]  R. Howard,et al.  Evidence for a poleward meridional flow on the sun , 1982 .

[13]  R. Howard,et al.  Solar rotation measurements at Mount Wilson , 1981 .

[14]  M. Waldmeier.  Cyclic variations of the polar coronal hole , 1981 .

[15]  B. Labonte,et al.  The sun is observed to be a torsional oscillator with a period of 11 years , 1980 .

[16]  V. Rušin,et al.  Prominences and the Green Corona Over the Solar Activity Cycle , 1998 .

[17]  S. P. Padilla,et al.  Solar rotation measurements at Mount Wilson , 1988 .