A coronal hole observed at 10.7 GHz with a large single dish-Reference-Cited by-同舟云学术

A coronal hole observed at 10.7 GHz with a large single dish

Published:1975-05 Issue:1 Volume:42 Page:157-161
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

F�rst E.,Hirth W.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00153292.pdf

Reference13 articles.

1. Burton, W. M. : 1968, in K. O. Kiepenheuer (ed.), ?Structure and Development of Solar Active Regions?, IAU Symp. 35, 393.

2. Chiuderi-Drago, F.: 1974, presented on the Conference on ATM Mission, Florence 1974.

3. Chiuderi, F., Fürst, E., Hirth, W., and Lantos, W.: 1974, to be published in Astronomy and Astrophysics.

4. Fürst, E., Hachenberg, O., Zinz, W., and Hirth, W.: 1973, Solar Phys. 32, 445.

5. Krieger, A. S., Timothy, A. F., and Roelof, E. C.: 1973, Solar Phys. 29, 505.

Cited by 20 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Coronal partings;Advances in Space Research;2016-02

2. Radio Observations of Coronal Phenomena and Solar Flares;Physics of Solar Planetary Environments: Proceedings of the International Symposium on Solar-Terrestrial Physics, June 7-18,1976 Boulder, Colorado, Volume I;2013-03-19

3. Specific features of radio emissions of coronal holes based on eclipse and noneclipse observations at a solar activity minimum;Geomagnetism and Aeronomy;2012-04

4. An Interpretation of the Coronal Holes’ Visibility in the Millimeter Wavelength Range;Solar Physics;2007-09-03

5. A multi-wavelength study of solar coronal-hole regions showing radio enhancements;Astronomy & Astrophysics;2001-11