
Das Gesenkformen I
R. Eschelbach
₹3,623

Proceedings of the First Issi Workshop 6-10 November 1995, Bern, Switzerland
by Rudolf Von Steiger, R. Lallement, M. a. Lee
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In summary, we can conclude that the contributions of the different ionization processes to the total ionization rate for the most abundant interstellar species are basically known. The ionization of the noble gases He and Ne is almost completely dominated by photoionization, whereas for H charge-exchange with the solar wind is most important. For other species, such as 0 and Ar, both processes contribute significantly.
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