Published May 1980
| Version v1
Journal article
Possibility of observations of recombination lines in the solar radiation
- 1. AN SSSR, Leningrad. Fiziko-Tekhnicheskij Inst.
- 2. AN SSSR, Astrofizicheskaya Observatoriya
Description
The intensity of the HI recombination emission nα with quantum numbers n=24-36 are estimated for the quiet Sun. It is shown that relative line intensities are within the interval 10-2-10-4. It means that such lines can be observed by existing radio-receiving equipment. It is concluded that observation of recombination lines is the base for a new method of investigation of solar low chromosphere
Additional details
Additional titles
- Original title (Russian)
- Возможность наблюдений рекомбинационных линий в излучении Солнца
Publishing Information
- Journal Title
- Astron. Zh.
- Journal Volume
- 57
- Journal Issue
- 3
- Series
- Astron. Zh.
- Journal Page Range
- 621-623
- ISSN
- 0004-6299
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 11567467
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- CHROMOSPHERE; FAR INFRARED RADIATION; HYDROGEN; MICROWAVE RADIATION; RECOMBINATION; SOLAR RADIATION; THEORETICAL DATA
- Descriptors DEC
- ATMOSPHERES; DATA; ELECTROMAGNETIC RADIATION; ELEMENTS; INFORMATION; INFRARED RADIATION; NONMETALS; NUMERICAL DATA; RADIATIONS; SOLAR ATMOSPHERE; STELLAR RADIATION
Optional Information
- Notes
- For English translation see the journal Soviet Astronomy - AJ (USA).