Chromospheric fine structure revisited

Details Chromospheric fine structure revisited Chromospheric fine structure revisited

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...264..236g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 264, no. 1, p. 236-242.

Astronomy and Astrophysics

Astrophysics

22

Chromosphere, Solar Atmosphere, Solar Limb, Spicules, Stellar Structure, Doppler Effect, H Alpha Line, Velocity Distribution

Scientific paper

We obtained H-alpha spectra from both spicules at the limb and mottles at disk center. We compare our results with data obtained by other groups and derive two distributions of axial spicule velocity, one based on limb, the other on disk observations. The two distributions disagree. We conclude that our knowledge on the basic properties of the chromospheric fine structure has not much improved in the last two decades; it is still rather scanty.

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