Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..424...37g&link_type=abstract
Proceedings of the 9th International Conference of the Hellenic Astronomical Society, proceedings of a conference held 20-24 Sep
Astronomy and Astrophysics
Astronomy
Scientific paper
The main properties of the coronal mass ejections observed by the Solar and Heliospheric Observatory (SOHO) mission’s Large Angle and Spectrometric Coronagraph (LASCO) from January 1996 until December 2008 are studied. For this the extended database of the solar proton enhancements with proton flux >0.1pfu at energy >10MeV measured at the Earth’s orbit (Belov et al. 2005) as well as the solar flare flux measurements provided by the Geostationary Operational Environmental Satellites (GOES) during this time period are used. Coronal mass ejections data were corrected taking into account the gaps of SOHO during the last solar cycle and were separated according to their linear speed, their width and their kinetic energy. Additionally, a correlative analysis of these properties of coronal mass ejections in connection with the associated solar proton enhancements gives useful results.
Asvestari E.
Belov Aleksander A.
Gerontidou Maria
Kurt Veli
Mavromichalaki Helen
No associations
LandOfFree
Fluctuations of CMEs Characteristics During the Declining Phase of the Last Solar Cycle 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 Fluctuations of CMEs Characteristics During the Declining Phase of the Last Solar Cycle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fluctuations of CMEs Characteristics During the Declining Phase of the Last Solar Cycle will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-953797