The Solar Origin of Corotating Interaction Regions and their Formation in the Inner Heliosphere-Reference-Cited by-同舟云学术

The Solar Origin of Corotating Interaction Regions and their Formation in the Inner Heliosphere

Published:1999 Issue: Volume: Page:141-178
ISSN:1385-7525
Container-title:Space Sciences Series of ISSI
language:
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Author:

Balogh A.,Bothmer V.,Crooker N. U.,Forsyth R. J.,Gloeckler G.,Hewish A.,Hilchenbach M.,Kallenbach R.,Klecker B.,Linker J. A.,Lucek E.,Mann G.,Marsch E.,Posner A.,Richardson I. G.,Schmidt J. M.,Scholer M.,Wang Y.-M.,Wimmer-Schweingruber R. F.,Aellig M. R.,Bochsler P.,Hefti S.,Mikić Z.

Publisher

Springer Netherlands

Link

http://link.springer.com/content/pdf/10.1007/978-94-017-1179-1_11

Reference73 articles.

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2. Aellig, M. R., Grünwaldt, H., Bochsler, P., Wurz, P., Hefti, S., Kallenbach, R., Ipavich, F. M., and the CELIAS team: 1998, `Iron Freeze-in Temperatures Measured by SOHO/CELIAS/CTOF’, J. Geophys. Res. 103, 17,215–17, 222.

3. Altschuler, M. D., and Newkirk, G.: 1969, `Magnetic Fields and the Structure of the Corona’, Sol. Phys. 9, 131–141.

4. Arnaud, M., and Rothenflug, R.: 1985, An Updated Evaluation of Recombination and Ionization Rates’, Astron. Astrophys. Suppl. See 60, 425–457.

5. Billings, D. E.: 1966, A Guide to the Solar Corona,Academic Press.

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