Temperature and microturbulence in the outer regions of prominences

Details Temperature and microturbulence in the outer regions of prominences Temperature and microturbulence in the outer regions of prominences

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...51..103m&link_type=abstract

Solar Physics, vol. 51, Jan.-Feb. 1977, p. 103-111. In French.

Physics

9

Plasma Turbulence, Solar Prominences, Solar Temperature, Electron Energy, H Alpha Line, Solar Wind Velocity

Scientific paper

H alpha and K line profiles have been determined in all regions of a
quiescent prominence where these emissions are likley to originate in
optically thin layers. From this data, an electron temperature of 5700 K
and a microturbulent velocity of 6.7 km/s were obtained for the outer
parts of the prominence.

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