| dc.creator |
Fernandes F.C.R. |
|
| dc.creator |
Sawant H.S. |
|
| dc.creator |
Cecatto J.R. |
|
| dc.creator |
Krishan V. |
|
| dc.creator |
Karlický M. |
|
| dc.creator |
Rosa R.R. |
|
| dc.date |
2003 |
|
| dc.date.accessioned |
2013-06-01T09:58:27Z |
|
| dc.date.available |
2013-06-01T09:58:27Z |
|
| dc.date.issued |
2013-06-01 |
|
| dc.identifier |
http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332003000100009 |
|
| dc.identifier |
http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2003&volume=33&issue=1&spage=109 |
|
| dc.identifier.uri |
http://koha.mediu.edu.my:8181/jspui/handle/123456789/8009 |
|
| dc.description |
The solar radio emissions in the decimetric frequency range (above 1000 MHz) are very rich in temporal and/or spectral fine structures. The Brazilian Solar Spectroscope (BSS) at INPE started operating in 1998. Since then, various types of fine structures, in the frequency range of (1000-2500) MHz, with high time and frequency resolutions have been recorded. The observed bursts include dot-like emissions and chains of dots, lace bursts exhibiting intensity variations as a function of frequency and zebra pattern emissions. It is suggested that they can be generated by a plasma resonance instability mechanism. This model can explain many features of the observed fine structures. |
|
| dc.publisher |
Sociedade Brasileira de Física |
|
| dc.source |
Brazilian Journal of Physics |
|
| dc.title |
Evidence of plasma resonance instability from observations of solar decimetric fine structures |
|