Published December 1974
| Version v1
Report
Absolute photometry and coronal structure during solar eclipse June 30, 1973
Creators
Description
The white corona was microphotometrically measured; the result of the measurement is a table of the absolute intensity of the corona for the individual position angles by 5deg and a height above the Sun's edge by 0.1 - 0.2 between 1.1 and 2.9 diameters of the solar disk. A detailed description of the corona is given. The eastern edge reminds of the corona at minimal solar activity, the western edge has a rich structure and many coronal rays. (Oy)
Additional details
Additional titles
- Original title (Slovak)
- Absolutna fotometria a struktura korony zo zatmenia slnka 30. juna 1973
Publishing Information
- Imprint Title
- Solar corona and its relation to interplanetary space and to geoactivity
- Imprint Pagination
- p. 31-57.
- Report number
- INIS-mf--3390
Conference
- Title
- National solar seminar.
- Dates
- 26 Sep 1974.
- Place
- Horny Smokovec, Czechoslovakia.
INIS
- Country of Publication
- Serbia and Montenegro
- Country of Input or Organization
- Serbia and Montenegro
- INIS RN
- 8308698
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- DENSITOMETERS; ECLIPSE; PHOTOMETRY; SOLAR CORONA; SUN; TABLES
- Descriptors DEC
- INFORMATION; MEASURING INSTRUMENTS; PHOTOMETERS; STARS
Optional Information
- Notes
- Imprint:Slnecna korona a jej vztah k medziplanetarnemu prostoru a geoaktivite.;Zbornik referatov z celostatneho slnecneho seminara.