A method for arc-second determination of solar burst emission centers with high time resolution and sensitivity at 48 GHz-Reference-Cited by-同舟云学术

A method for arc-second determination of solar burst emission centers with high time resolution and sensitivity at 48 GHz

Published:1995-06 Issue:1 Volume:159 Page:157-171
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Costa J. E. R.,Correia E.,Kaufmann P.,Magun A.,Herrmann R.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00733039.pdf

Reference21 articles.

1. Altenhoff, W. J., Baars, J. W. M., Downes, T., and Wink, J. E.: 1987,Astron. Astrophys. 184, 381.

2. Bastian, T. S., Nitta, N., Kiplinger, A. L., and Dulk, G. A.: 1994, in S. Enome and T. Hirayama (eds.),Proc. of Kofu Symposium on New Look at the Sun with Emphasis on Advanced Observations of Coronal Dynamics and Flares, September 6?10, 1993, Kofu, Japan, NRO Report No. 360, p. 199.

3. Correia, E. and Kaufmann, P.: 1987,Solar Phys. 111, 143.

4. Costa, J. E. R., Homor, J. L., and Kaufmann, P.: 1986, in E. Tandberg-Hanssen and H. S. Hudson (eds.), ?Solar Flares and Coronal Physics Using P/OF as a Research Tool?,NASA Conf. Publ. 2421, p. 201.

5. Costa, J. E. R., Gary, D., Bastian, T., and Kaufmann, P.: 1995, in preparation.

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