Major solar flares without coronal mass ejections

Details Major solar flares without coronal mass ejections Major solar flares without coronal mass ejections

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..257..283g&link_type=abstract

Universal Heliophysical Processes, Proceedings of the International Astronomical Union, IAU Symposium, Volume 257, p. 283-286

Astronomy and Astrophysics

Astronomy

5

Coronal Mass Ejections (Cmes), Flares, Particle Emission, Radio Radiation

Scientific paper

We examine the source properties of X-class soft X-ray flares that were not associated with coronal mass ejections (CMEs). All the flares were associated with intense microwave bursts implying the production of high energy electrons. However, most (85%) of the flares were not associated with metric type III bursts, even though open field lines existed in all but two of the active regions. The X-class flares seem to be truly confined because there was no material ejection (thermal or nonthermal) away from the flaring region into space.

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