dc.contributor.author |
Kundu, M. R |
|
dc.contributor.author |
Shevgaonkar, R. K |
|
dc.date.accessioned |
2010-09-02T10:45:58Z |
|
dc.date.available |
2010-09-02T10:45:58Z |
|
dc.date.issued |
1985-04 |
|
dc.identifier.citation |
The Astrophysical Journal, Vol. 291, pp. 860-864 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/5241 |
|
dc.description.abstract |
A preflare active region was studied using the Very Large Array at 2, 6, and 20 cm. At 2 cm the region is composed of two components located in regions of opposite polarity. Both components are preheated prior to the impulsive onset of a flare. However, one component develops new structures during preburst phase, and the burst occurs in this location. It is believed that the new structures represent emerging flux regions which interact with an overlying loop to produce a neutral sheet, which ultimately is responsible for triggering the flare. |
en |
dc.language.iso |
en |
en |
dc.publisher |
The University of Chicago Press |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1985ApJ...291..860K |
en |
dc.rights |
© The American Astronomical Society |
en |
dc.subject |
Solar activity |
en |
dc.subject |
Solar flares |
en |
dc.subject |
Solar radio bursts |
en |
dc.subject |
Astronomical maps |
en |
dc.subject |
Interferometry |
en |
dc.subject |
Magnetic flux |
en |
dc.subject |
Radiant flux density |
en |
dc.subject |
Very large array (Vla) |
en |
dc.title |
Multiwavelength observations of a preflare solar active region using the VLA |
en |
dc.type |
Article |
en |