Hostname: page-component-857557d7f7-ktsnh Total loading time: 0 Render date: 2025-11-24T07:05:21.981Z Has data issue: false hasContentIssue false
  • English
  • Français

On Coronal Instability and Moving Radio Features Associated with a Flare Spray

Published online by Cambridge University Press:  14 August 2015

G. Daigne
G. Daigne*
Affiliation:
Meudon-Nançay Observatory, France

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A solar radio outburst with its different parts well seen on metric wavelengths is described. A stable source shows successively two kinds of emission before the flash-phase of the event, and a moving type IV burst (V ≃ 1000 km/s), initiated 1/4 solar radius high, is directly associated with a spray-type prominence. Parameters of this radiating source are discussed.

A type II burst seen on lower frequencies with a spectrograph (V ≃ 3200 km/s) seems to start after the flash phase. Two possible cases are considered for the generation of the shock-wave responsible for type II burst.

Information

Type
Part IV: Observations of Magnetic Fields Associated with Flares and Other TransitoryPhenomena
Information
Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 367 - 375
Copyright
Copyright © Reidel 1971 

References

Boischot, A. and Clavelier, B.: 1968, Ann. Astrophys. 31, 445.Google Scholar
Bruzek, A.: 1968, COSPAR Symp. Tokyo , 61.Google Scholar
Kai, K.: 1970 Solar Phys. 11, 310.CrossRefGoogle Scholar
Newkirk, G. A.: 1967, Ann. Rev. Astron. Astrophys. 5, 213.CrossRefGoogle Scholar
Orrall, F. Q. and Smith, H. J.: 1961, Sky Telesc. 22, 330.Google Scholar
Pneuman, G. W.: 1967, Solar Phys. 2, 462.CrossRefGoogle Scholar
Ramaty, R. and Lingenfelter, R. E.: 1968, Solar Phys. 5, 531.CrossRefGoogle Scholar
Riddle, A. C.: 1970, Solar Phys. 13, 448.CrossRefGoogle Scholar
Sagdeev, R. Z.: 1966, Rev. Plasma Phys. 4, 23.Google Scholar
Stewart, R. T. and Sheridan, K. V.: 1970, Solar Phys. 12, 229.CrossRefGoogle Scholar
Vinokur, M.: 1968, Ann. Astrophys. 31, 457.Google Scholar
Warwick, J. W.: 1957, Astrophys. J. 125, 811.CrossRefGoogle Scholar
Wild, J. P.: 1968, Proc. ASA 1 (4), 137.Google Scholar
Wild, J. P.: 1969, Solar Phys. 9, 260.CrossRefGoogle Scholar
Wild, J. P.: 1970, Proc. ASA (to be published) Google Scholar
Wild, J. P., Smerd, S. F. and Weiss, A. A.: 1963, Ann. Rev. Astron. Astrophys. 1, 291.CrossRefGoogle Scholar
Wild, J. P., Sheridan, K. V. and Kai, K.: 1968, Nature 218, 536.CrossRefGoogle Scholar
Zaitsev, V. V.: 1969, Soviet Astron. 12, 610.Google Scholar