Computer Science
Scientific paper
Oct 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006kfnt...22..346t&link_type=abstract
Kinematika i Fizika Nebesnykh Tel, vol. 22, no. 5, p.346-362
Computer Science
1
Scientific paper
The evolution and structure of the active region NOAA 0139 on the basis of radio observations obtained at RATAN-600, SSRT, and RT-22 are investigated. By means of a wavelet analysis as well as images obtained at the space orbital stations SOHO and TRACE, it is shown that observed dynamics of the S-component of microwave emission may be caused by the change of number and power of elementary flare events. The strong depression of emission revealed at short wavelengths in the course of evolution of active region is explained by the decrease of fluxes of accelerated electrons, which are responsible for the high temperature of the transition region and upper chromosphere of the Sun. The results obtained show evidence for an essential contribution of elementary flare events to the heating of the coronal plasma.
Agalakov B. V.
Borisevich T. P.
Peterova Natalia G.
Tsap Yu. T.
Tsvetkov L. I.
No associations
LandOfFree
The heating of the upper solar atmosphere and variations of microwave emission from the active region NOAA 0139 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The heating of the upper solar atmosphere and variations of microwave emission from the active region NOAA 0139, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The heating of the upper solar atmosphere and variations of microwave emission from the active region NOAA 0139 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-908491