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imported>BinChen ((A) Composite image of AR 11339 from SDO/AIA on 2011 November 5. (B) GOES SXR flux showing the M1.8 flare and its aftermath. The coronal jet occurred between 21:18-21:25 UT (dashed vertical lines). (C-D) VLA dynamic spectra in which type IIIdm bursts (the) |
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(A) Composite image of AR 11339 from SDO/AIA | Type III radio bursts observed by the VLA on 2011 November 5. (A) Composite image of AR 11339 from SDO/AIA. (B) GOES SXR flux showing the M1.8 flare and its aftermath. The coronal jet occurred between 21:18-21:25 UT (dashed vertical lines). (C-D) VLA dynamic spectra in which type IIIdm bursts (the bright vertical or nearly-vertical features) are present. (E) VLA radio (blue) and RHESSI 12-25 keV HXR (red) light curves during the radio bursts. The small and large boxes correspond to the time ranges of the dynamic spectra shown in (C) and (D). | ||
Revision as of 21:17, 26 January 2013
Type III radio bursts observed by the VLA on 2011 November 5. (A) Composite image of AR 11339 from SDO/AIA. (B) GOES SXR flux showing the M1.8 flare and its aftermath. The coronal jet occurred between 21:18-21:25 UT (dashed vertical lines). (C-D) VLA dynamic spectra in which type IIIdm bursts (the bright vertical or nearly-vertical features) are present. (E) VLA radio (blue) and RHESSI 12-25 keV HXR (red) light curves during the radio bursts. The small and large boxes correspond to the time ranges of the dynamic spectra shown in (C) and (D).
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