Other
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..265s&link_type=abstract
In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 265-2
Other
Magnetic Field Reconnection, Solar Corona, Solar Limb, Solar Prominences, Stellar Mass Ejection, Thermal Emission, Magnetic Fields, Solar Flares, Solar X-Rays, Space Plasmas, Ultraviolet Radiation
Scientific paper
Observations of a limb prominence which became activated following two small x-ray flares on 13 Aug. 1980 are presented. For the second event the structure was clearly visible in soft x-rays for over 30 minutes. The prominence was also emitting strongly at other wavelengths, and in particular the UV O V emission was seen from what appeared to be precisely the same structure as the x-rays. The brightest point in both the UV and x-rays appeared first at the opposite end of the prominence to the chromospheric flare. The highest temperature plasma was in excess of 107 K. The energization of the prominence is discussed and it is suggested that energy deposition by energetic particles could be important. It is further suggested that the particles are accelerated by reconnecting coronal magnetic fields associated with a coronal mass ejection which was in progress throughout this period.
No associations
LandOfFree
Multi-thermal emission associated with a limb prominence following two subflares and a coronal mass ejection 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 Multi-thermal emission associated with a limb prominence following two subflares and a coronal mass ejection, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multi-thermal emission associated with a limb prominence following two subflares and a coronal mass ejection will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1552345