Investigation of Type III Radio Bursts in Different Phases of Solar Flares
碩士 === 國立中央大學 === 太空科學研究所 === 107 === The purpose of this study is to investigate the difference of the characteristics of type III solar radio bursts in different phases of solar flares. We use the dynamic spectrum observed by Solar Broadband Radio Spectrometer (SBRS) in the frequency range of 2.6-...
Main Authors: | Shao-Fu Hsieh, 謝劭甫 |
---|---|
Other Authors: | Ya-Hui Yang |
Format: | Others |
Language: | zh-TW |
Published: |
2019
|
Online Access: | http://ndltd.ncl.edu.tw/handle/76wz7h |
Similar Items
-
Magnetic reconnection of solar flare detected by solar radio burst type III
by: Amran, N.A, et al.
Published: (2014) -
Magnetic Reconnection of Solar Flare Detected by Solar Radio Burst Type III
by: Amran, NA, et al. -
A model of so-called "Zebra" emissions in solar flare radio burst continua
by: R. A. Treumann, et al.
Published: (2011-09-01) -
Observations of Solar Type III radio bursts by Cassini/RPWS experiment
by: M. Y. Boudjada, et al.
Published: (2020-12-01) -
Statistical Analysis of Solar Radio Burst Type III and Type IV with Relation to Solar Activities
by: Hamidi, Z.S, et al.
Published: (2019)