dc.contributor.author |
Makarov, V. I |
|
dc.contributor.author |
Fatianov, M. P |
|
dc.contributor.author |
Sivaraman, K. R |
|
dc.date.accessioned |
2008-09-23T14:16:43Z |
|
dc.date.available |
2008-09-23T14:16:43Z |
|
dc.date.issued |
1983-06 |
|
dc.identifier.citation |
Solar Physics, Vol. 85, No. 2, pp. 215 - 226 |
en |
dc.identifier.issn |
0038-0938 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3833 |
|
dc.description.abstract |
Poleward migration of the magnetic neutral line on the sun has been calculated for the periods 1945-1950 and 1955-1981 using synoptic charts based on H-alpha observations. Epochs of sign reversal of the solar magnetic field at latitudes 50 to 90 deg have been determined for these periods. During the cycles 19 and 20 a threefold sign reversal took place in the northern hemisphere. During all the above cycles both the solar poles were of one polarity for a period ranging from 0.5 to 1 year. The poleward drift velocity of the magnetic neutral line varies from 6 to 29 m/s and seems to depend on the strength of the cycle. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Springer |
en |
dc.relation.uri |
http://www.springerlink.com/content/g615410654h26604/ |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1983SoPh...85..215M |
en |
dc.subject |
Lines of Force |
en |
dc.subject |
Magnetic Field Configurations |
en |
dc.subject |
Magnetic Poles |
en |
dc.subject |
Solar Magnetic Field |
en |
dc.subject |
Drift Rate |
en |
dc.subject |
Latitude |
en |
dc.subject |
Long Term Effects |
en |
dc.subject |
Northern Hemisphere |
en |
dc.subject |
Polarity |
en |
dc.subject |
Temporal Distribution |
en |
dc.title |
Poleward migration of the magnetic neutral line and the reversal of the polar fields on the sun. I - Period 1945-1981 |
en |
dc.type |
Article |
en |