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The determination of the velocity amplitude of the total photospheric motion field

โœ Scribed by N. N. Kondrashova; E. A. Gurtovenko

Publisher
Springer
Year
1974
Tongue
English
Weight
383 KB
Volume
34
Category
Article
ISSN
0038-0938

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A given motion field in a stellar atmosphere is usually observed through 'filters' defined by line shifts and -broadenings and conventionally called macroturbulence and microturbulence. These 'filters' can be defined and computed exactly, as a function of the wave number of the velocity field (Figu