Physical parameters of EUV explosive events

Details Physical parameters of EUV explosive events Physical parameters of EUV explosive events

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...360..331p&link_type=abstract

Astronomy and Astrophysics, Vol. 360, p.331-334

Astronomy and Astrophysics

Astrophysics

7

Sun: Atmosphere, Sun: Magnetic Fields, Sun: Particle Emission, Sun: Transition Region, Sun: Uv Radiation

Scientific paper

Previously published results of EUV explosive events and electron density enhancements in the solar transition region are revised. An attempt has been made to correlate both observational phenomena, and to associate the observed density enhancements to magnetic reconnection sites. The corresponding local magnetic field strength in these sites is estimated. These values are of the same order as previously measured in photospheric cancelling flux regions.

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