Rotating convection and the solar differential rotation
β Scribed by Kwing L. Chan; Hans G. Mayr
- Publisher
- Springer
- Year
- 1994
- Tongue
- English
- Weight
- 471 KB
- Volume
- 152
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
In this paper we study the dependence on depth and latitude of the solar angular velocity produced by a meridian circulation in the convection zone, assuming that the main mechanism responsible for setting up and driving the circulation is the interaction of rotation with convection. We solve the fi
Areas of sunspots and their positions taken from the Greenwich Photoheliographic Results (1874-1976) and typical intensities of the umbrae and penumbrae are used to calculate daily values of the solar flux at a wavelength of about 500 nm. Using overlapping time series of 512 days each solar rotation