Hydromagnetic shocks in the solar wind
β Scribed by K. W. Ogilvie; L. F. Burlaga
- Publisher
- Springer
- Year
- 1969
- Tongue
- English
- Weight
- 618 KB
- Volume
- 8
- Category
- Article
- ISSN
- 0038-0938
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π SIMILAR VOLUMES
The evolutionary state of slow forward shock waves is examined with the use of two MHD numerical codes. Our study is intended to be exploratory rather than a detailed parametric one. The first code is one-dimensional (with three components of velocity and magnetic field) which is used to follow a sl
The effects of the large scale gradients generated by the solar wind expansion are taken into account to estimate the turbulent flux from nonlinear interactions among inward and outward propagating AlfvΓ©n waves. It is shown that even if all inward propagating waves are lost in the acceleration regio