Hostname: page-component-cd9895bd7-jn8rn Total loading time: 0 Render date: 2024-12-12T09:45:47.009Z Has data issue: false hasContentIssue false
  • English
  • Français

Collaborative VLA and LASCO Observations of Nonthermal Energy Release in the Corona

Published online by Cambridge University Press:  13 May 2016

R. F. Willson
R. F. Willson*
Affiliation:
Department of Physics and Astronomy, Tufts University, Medford, MA 02155, USA

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.

We discuss recent collaborative observations of coronal mass ejections and related activity using the Very Large Array (VLA) and the Solar and Heliospheric Observatory (SOHO). VLA observations show the onset of intense 400 cm burst emission during an X1 GOES soft X-ray burst observed by the Yohkoh spacecraft and prior to a CME observed by the Large Angle Spectroscometric C2 Coronagraph (LASCO) on board SOHO. VLA snapshot maps show that the 400 cm burst site varied discontinuously throughout the course of the flare, possibly reflecting abrupt changes in the structure of the coronal magnetic fields along which the energetic particles traveled.

Type
Session V: Coronal Heating and Solar Wind Acceleration
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 520 - 522
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Willson, R.F., et al. ApJ(Letters) 504, 417.Google Scholar