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On three-dimensional information pictures of chromospheric spicules

✍ Scribed by S. G. Mamedov; E. Sh. Orudzhev

Publisher
Springer
Year
1969
Tongue
English
Weight
173 KB
Volume
6
Category
Article
ISSN
0038-0938

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✦ Synopsis

Almost all observations of the sun, including all kinds of spectropliotometry, magnetic field and radial velocity measurements, and also spectroheliographic researches supply us with only two-dimensional (flat) information about the object. We obtain data on the distribution of a physical parameter in two-space dimensions (in some cases one of these dimensions is the wavelength in the spectrum) or in space-time dimensions. Only when we take a cinema-film (MAMEDOV, 1966) of the spectral changes over the disk with a slowly moving image of the sun on the slit, we have a real possibility of obtaining three-dimensional information: two space dimensions

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