Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...201..339a&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 201, no. 2, Aug. 1988, p. 339-349.
Astronomy and Astrophysics
Astrophysics
24
Chromosphere, Mass Flow Rate, Photosphere, Solar Atmosphere, Solar Corona, Sunspots, Solar Magnetic Field, Solar Maximum Mission, Ultraviolet Spectrometers, Velocity Distribution
Scientific paper
The authors have studied the height dependence of the characteristics of the Evershed flow in the photosphere, chromosphere and chromosphere-corona transition region. The Multichannel Subtractive Double Pass Spectrograph was used to obtain line of sight velocity maps in Hα, the Meudon magnetograph for mapping the photospheric velocity and magnetic field and the Ultraviolet Spectrometer and Polarimeter on the Solar Maximum Mission spacecraft for line-of-sight velocities in C IV, in sunspot regions. The observations are practically simultaneous in the three atmospheric levels and cover three consecutive days (Sep 28, 29 and 30, 1980). The emphasis was on the large scale, quasi-stationary characteristics of the flow.
Alissandrakis Constantine E.
Dialetis D.
Mein Pierre
Schmieder Brigitte
Simon Gabor
No associations
LandOfFree
The Evershed flow in the solar photosphere, chromosphere and chromosphere-corona transition region does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Evershed flow in the solar photosphere, chromosphere and chromosphere-corona transition region, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Evershed flow in the solar photosphere, chromosphere and chromosphere-corona transition region will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1692886