Fe II lines in the problem of the diagnostic of solar photospheric shocks

Details Fe II lines in the problem of the diagnostic of solar photospheric shocks Fe II lines in the problem of the diagnostic of solar photospheric shocks

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnt...16..130g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 16, no. 2, p. 130-137

Computer Science

4

Scientific paper

We propose to use Fe II lines observed near the solar limb for the
detection of photospheric shocks at granule edges. Their theoretical
spectral scans synthesized with 2-D models provide a more clear evidence
for photospheric shocks as compared to spectral lines of neutral
elements.

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