Published September 1986
| Version v1
Journal article
Decameter astrospectroscopy
Creators
Description
Possibilities of the method for investigation of rarefied cold cosmic bodies by the carbon lines in the decameter range are considered in the popular form. In 1978 the spectral lines in the decameter waves were detected for the first time by the UTR-2 radiotelescope. One succeeded in recording the line with quantum numbers n=603-732. The recombination lines were observed for the first time during absorption. The recombination lines determined in the decameter waves demonstrate brightly the effect of line broadening caused by inelastic particle collisions. The results are mainly obtained for interstellar clouds being in the direction of the Cassiopeia A radiosource
Additional details
Additional titles
- Original title (Russian)
- Декаметровая астроспектроскопия
Publishing Information
- Journal Title
- Zemlya Vselennaya
- Journal Issue
- no.5
- Series
- Zemlya Vselennaya.
- ISSN
- 0044-3948
- CODEN
- ZEVSA
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 18067279
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ABSORPTION; CARBON IONS; COSMIC GASES; COSMIC RADIATION; ENERGY LEVELS; IMAGES; INTERSTELLAR SPACE; LINE WIDTHS; MHZ RANGE 01-100; RADIOWAVE RADIATION; RECOMBINATION
- Descriptors DEC
- ATOMIC IONS; CHARGED PARTICLES; ELECTROMAGNETIC RADIATION; FLUIDS; FREQUENCY RANGE; GASES; IONIZING RADIATIONS; IONS; MHZ RANGE; RADIATIONS; SPACE