ON THE OPTICAL THICKNESS OF RADIATING, COOLING, AND EXPANDING HYDROGEN CLOUD FOR RADIO FREQUENCIES. (in Russian)
Journal Article
·
· Izv. Krym. Astrofiz. Observ., 38: 205-7(1967)(Publ. 1968).
OSTI ID:4823231
- Research Organization:
- Originating Research Org. not identified
- NSA Number:
- NSA-23-006827
- OSTI ID:
- 4823231
- Journal Information:
- Izv. Krym. Astrofiz. Observ., 38: 205-7(1967)(Publ. 1968)., Other Information: Orig. Receipt Date: 31-DEC-69
- Country of Publication:
- Country unknown/Code not available
- Language:
- Russian
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Related Subjects
N32130* -Physics-Astrophysics-Quasi-stellar
Radio & X- Ray Sources
ATMOSPHERE
COOLING
EXPANSION
HYDROGEN
RADIATIONS
RADIO WAVES
STARS
THICKNESS
WAVE PROPAGATION
RADIO WAVES/propagation through radiating, cooling, and expanding hydrogen clouds, (T)
HYDROGEN/optical thickness of radiating, cooling, and expanding clouds of, radio-frequency, (T)
STARS/optical thickness of hydrogen clouds associated with
radio-frequency
(T)
Radio & X- Ray Sources
ATMOSPHERE
COOLING
EXPANSION
HYDROGEN
RADIATIONS
RADIO WAVES
STARS
THICKNESS
WAVE PROPAGATION
RADIO WAVES/propagation through radiating, cooling, and expanding hydrogen clouds, (T)
HYDROGEN/optical thickness of radiating, cooling, and expanding clouds of, radio-frequency, (T)
STARS/optical thickness of hydrogen clouds associated with
radio-frequency
(T)