A new method for the analysis of the solar photospheric spectrum
β Scribed by P. Persi
- Publisher
- Springer
- Year
- 1975
- Tongue
- English
- Weight
- 345 KB
- Volume
- 43
- Category
- Article
- ISSN
- 0038-0938
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π SIMILAR VOLUMES
Some weak unidentified solar photospheric lines in the wavelength range: (3400-3465) ~ may be due to PH lines of the (0, 0) band of the PH(A3//~ -X 3 Z-) system. These faint PH molecular lines have resulted an excitation temperature of the order of 4500 K. Using experimental lifetime data for PH in
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
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