VLA 20160218: Difference between revisions
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| '''Time''' || '''Feature''' || '''Event''' || '''Location''' || '''RHESSI''' || '''Quicklook Images''' || '''Comments''' | | '''Time''' || '''Feature''' || '''Event''' || '''Location''' || '''RHESSI''' || '''Quicklook Images''' || '''Comments''' | ||
|- | |- | ||
|19:43-19:44 || | |19:43-19:44 || small spikes || Maybe A6.4Microflare@19:43 || Near solar disk center || No || || Few stripes at lower frequency, maybe amicroflare. | ||
|- | |- | ||
|20:08-20:10 || Type III, Broadband GS || C1.2@19:59 || ? || No || || Type III like features at lower frequency (which frequency range?) and broadband gyrosynchrotron emission across entire 1-2 GHz band | |20:08-20:10 || Type III, Broadband GS || C1.2@19:59 || ? || No || || Type III like features at lower frequency (which frequency range?) and broadband gyrosynchrotron emission across entire 1-2 GHz band |
Revision as of 20:00, 15 November 2017
Overview
(write a brief summary of the observation) This observation was made in C configuration (max baseline length 3 km) with the full array (27 antennas) in L band (1-2 GHz), with 2 MHz frequency resolution and 50 ms time resolution. The observation was coordinated with Hinode and IRIS (HOP 297). Two C-class flares were covered: A C1.2 eruptive flare at the limb N11W88 starting at 19:59 and a C1.4 flare from AR 2501 near the disk center N03E23. RHESSI data is available for the impulsive phase of the C1.4 flare. File:20160218 sum.png
- link to VLA overview movie: this should have ~10 s cadence at several frequencies (perhaps one for each spw, so 8), zoomed in to the flare site.
- link to AIA movie: find one from HEK events or make your own
List of Events/Features
Time | Feature | Event | Location | RHESSI | Quicklook Images | Comments |
19:43-19:44 | small spikes | Maybe A6.4Microflare@19:43 | Near solar disk center | No | Few stripes at lower frequency, maybe amicroflare. | |
20:08-20:10 | Type III, Broadband GS | C1.2@19:59 | ? | No | Type III like features at lower frequency (which frequency range?) and broadband gyrosynchrotron emission across entire 1-2 GHz band | |
21:09-21:12 | Pulsations | C1.8@21:08 | Ar2501 near solar disk center | Yes | File:2110.png | Quasi-periodic pulsations in impulsive phase. Highest RHESSI response @ 25keV. Radio source located near a footpoint. |