On frequency and strength of shock waves in the solar atmosphere
β Scribed by Peter Ulmschneider
- Publisher
- Springer
- Year
- 1970
- Tongue
- English
- Weight
- 554 KB
- Volume
- 12
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
β¦ Synopsis
Comparison of computed radiative energy losses of several new empirical chromospheric models with heating by shock wave dissipation gives information on the frequency and strength of shock waves in the solar chromosphere. A mechanical flux of around 2.5 β’ 10 ~ erg/cm e sec is found for the base of the chromosphere. The shocks are weak and the wave period is around 10 sec.
π SIMILAR VOLUMES
A consistent account of plasma turbulence in magnetohydrodynamics equation s describing transport processes across the magnetic field is presented. The structure of the perpendicular shock wave generated in the solar atmosphere, as a result of either local disturbance of the magnetic field or dense