Solar Partial N-burst

Details Solar Partial N-burst Solar Partial N-burst

Aug 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003chjaa...3..381n&link_type=abstract

Chinese Journal of Astronomy & Astrophysics, Vol. 3, p. 381-390

Astronomy and Astrophysics

Astrophysics

4

Sun: Radio Radiation, Sun: Magnetic Fields

Scientific paper

We present a new sub-class of type III solar radio burst at the high frequencies around 6.0 GHz. In addition to a descending and an ascending branch on the dynamic spectrum, it has an inverted morphology different from the simple type U-burst. We call it ``partial N-burst'' because it is interpreted as the known N-burst minus its first branch. The partial N-burst presented here was detected among a reverse slope type III (RS-III) burst group prior to the type V solar radio continuum and was simultaneously recorded by two spectrometers at the National Astronomical Observatories, Chinese Academy of Sciences (NAOC, 5.20-7.60 GHz) and at Purple Mountain Observatory (PMO, 4.50-7.50 GHz) on 1999 August 25. After the N-burst and M-burst, the partial N-burst is a third piece of evidence for a magnetic mirror effect in solar radio observation, when the same electron is reflected at a pinched foot of a flare loop.

Affiliated with

Also associated with

No associations

Rating

Solar Partial N-burst 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 Solar Partial N-burst, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Partial N-burst will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1667482