Mass flow velocity distribution in the solar chromosphere

Details Mass flow velocity distribution in the solar chromosphere Mass flow velocity distribution in the solar chromosphere

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981wsco.rept.....t&link_type=abstract

Final Report, 1 Jan. 1980 - 31 Sep. 1981 Weber State Coll., Ogden, UT. Dept. of Physics.

Physics

Chromosphere, Flow Velocity, Mass Flow, Velocity Distribution, High Resolution, Silicon, Solar Atmosphere, Spectrographs, Spectrum Analysis, Telescopes

Scientific paper

A study of chromospheric lines (those of Si-II and Si-III) was made using the data from high resolution telescope and spectrograph (HRTS). The optically thick line profiles such as lambda 1206 due to Si-III and lambda 1265 and lambda 1533 due to Si-II were to be investigated in detail using the techniques of spectrum synthesis in an attempt to model the mass flow velocity distribution in the region of the solar atmosphere.

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