Velocity field in a small solar flare

Details Velocity field in a small solar flare Velocity field in a small solar flare

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..439k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 439-440

Physics

Scientific paper

The temporal variations of the line-of-sight velocities have been revealed in a small flare during its main phase. The measurements were made in 34 Fraunhofer lines formed in different photospheric layers. The downflow was observed in the photosphere 4 min after the chromospheric flare peak with the maximum velocity followed 12 min later. The largest velocity variations (up to 1.6 km/s) occurred in the layer 180-220 km. An enhancement of 5-min velocity oscillations was found.

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