Published September 1987
| Version v1
Journal article
On the characteristics of the solar corona above the coronal hole
Description
It is shown that more fast than radial divergence of the magnetic field lines results in more strong cooling influence of the plasma flow on the solar corona regime. This explains the lower values of the plasma density and temperature and the higher flow velocity typical for coronal holes
Additional details
Additional titles
- Original title (Russian)
- О характеристиках солнечной короны над коронльной дырой
Publishing Information
- Journal Title
- Pis'ma Astron. Zh.
- Journal Volume
- 13
- Journal Issue
- 9
- Series
- Pis'ma Astron. Zh.
- Journal Page Range
- 797-802
- ISSN
- 0320-0108
- CODEN
- PAZHD
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 19020262
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ALFVEN WAVES; MAGNETIC FIELDS; MAGNETOACOUSTIC WAVES; PLASMA; PLASMA DENSITY; PLASMA HEATING; SOLAR CORONA; SOLAR WIND
- Descriptors DEC
- ATMOSPHERES; HEATING; HYDROMAGNETIC WAVES; SOLAR ACTIVITY; SOLAR ATMOSPHERE; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR CORONAE; STELLAR WINDS