Type III Radio Bursts and Microflares

Details Type III Radio Bursts and Microflares Type III Radio Bursts and Microflares

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spd....34.1501c&link_type=abstract

American Astronomical Society, SPD meeting #34, #15.01; Bulletin of the American Astronomical Society, Vol. 35, p.830

Astronomy and Astrophysics

Astronomy

Scientific paper

We present recent observations of microflares observed simultaneously in EUV (TRACE), radio (Nancay, Phoenix-2), and X-rays (RHESSI). During a period of 15 min on 19 July 2002 14:23-14:35 UT, RHESSI observed microflares approximately every 2 minutes. Each microflare was accompagnied by a radio Type III burst. The largest flare (14:29:25 UT) was also accompagnied by a cluster of decimetric radio spikes in the frequency range 1 to 2 GHz. In addition, FeXII (195 Å) images provided by TRACE show two jets-like emissions originating from a complex double arche structure. The centroid of the jets were found to travel at apparent speeds of ˜ 100 km s-1, consistent with observations by Shimojo et al. (1996). X-ray images show non-thermal emission (9-30 keV) from the footpoints of the TRACE arches. Strong correlation in flux amplitude is found between emissions in the radio ( ˜1340 MHz) and non-thermal X-ray (9-30 keV integrated). The event is interpreted as an anemone-jet in the model by Shibata et al. (1994). This research is supported by NASA contract NAS 5-98033.

Affiliated with

Also associated with

No associations

Rating

Type III Radio Bursts and Microflares does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Type III Radio Bursts and Microflares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Type III Radio Bursts and Microflares will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-987291