dc.contributor.author |
Das, T. K |
|
dc.contributor.author |
Nag, T. K |
|
dc.contributor.author |
Dutta, A. K |
|
dc.date.accessioned |
2008-09-04T16:52:44Z |
|
dc.date.available |
2008-09-04T16:52:44Z |
|
dc.date.issued |
1998 |
|
dc.identifier.citation |
BASI, Vol. 26, p. 311 - 315 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/3370 |
|
dc.description.abstract |
A study has been made about the solar proton events observed by NOAA satellite during the period 1976-1993 by considering their association with Hα-flares. The proton flux has been found to depend linearly upon the estimated flare energy output per day. The proton flux varies with the rise time also in a linear way. Study about the visual features of the proton - associated Hα-flares reveals that the proton events are connected with those kinds of flares which have multiple instabilities in the associated active regions |
en |
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1998BASI...26..311D |
en |
dc.subject |
Solar proton |
en |
dc.subject |
H-alpha flares |
en |
dc.title |
Solar proton events in relation to H-alpha flares |
en |
dc.type |
Article |
en |