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On H. alfvén's theory of the effect of magnetic storms on cosmic ray intensity

✍ Scribed by W.F.G. Swann


Publisher
Elsevier Science
Year
1954
Tongue
English
Weight
54 KB
Volume
257
Category
Article
ISSN
0016-0032

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On H. Alfvén's theory of the effect of m
✍ W.F.G. Swann 📂 Article 📅 1954 🏛 Elsevier Science 🌐 English ⚖ 518 KB

H. Alfv~n's theory envisages a stream of gas shot out from a place on the sun where there is a large magnetic field. The gas, supposed highly conducting, carries the magnetic field H with it, and the field is supposed to be perpendicular to the velocity v. A stationary observer observes an electric