Non-equilibrium ionization effects during flares in coronal loops

Details Non-equilibrium ionization effects during flares in coronal loops Non-equilibrium ionization effects during flares in coronal loops

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.505..517o&link_type=abstract

In: SOLMAG 2002. Proceedings of the Magnetic Coupling of the Solar Atmosphere Euroconference and IAU Colloquium 188, 11 - 15 Jun

Astronomy and Astrophysics

Astrophysics

Sun: Corona, X-Ray Spectroscopy

Scientific paper

We present preliminary results of hydrodynamic modeling of flares occurring in plasma magnetically confined in coronal loops, using the adaptive-mesh astrophysical hydrodynamic code FLASH. We also investigate the deviations from ionization equilibrium on the population fractions of the most abundant elements in astrophysical plasmas and the relevant consequences on observed spectra.

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