Investigation on the formation of herringbone structure in type II solar radio bursts
We report detailed observation of the ``herringbone'' of a Type II solar radio burst that occurred on 2010 November 3rd. Data from the Space Weather Prediction Center, National Oceanic and Atmospheric Administration, e-CALLISTO, and Nancay RadioHeliograph are analyzed. We determine the bri...
محفوظ في:
| المؤلفون الرئيسيون: | , , , |
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| التنسيق: | مقال |
| منشور في: |
Natl Astronomical Observatories, Chin Acad Sciences
2023
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| الموضوعات: | |
| الوصول للمادة أونلاين: | http://eprints.um.edu.my/38256/ |
| الوسوم: |
إضافة وسم
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| الملخص: | We report detailed observation of the ``herringbone'' of a Type II solar radio burst that occurred on 2010 November 3rd. Data from the Space Weather Prediction Center, National Oceanic and Atmospheric Administration, e-CALLISTO, and Nancay RadioHeliograph are analyzed. We determine the brightness temperature and degree of circular polarization of the ``herringbone'' burst. Correlations between the physical parameters and the ``herringbone'' are examined. Based on the relationship, this is the first study that suggested this ``herringbone'' was generated through fundamental plasma. |
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