VLA 20160219: Difference between revisions
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| '''Time''' || '''Feature''' || '''Event''' || ''' | | '''Time''' || '''Feature''' || '''Event''' || '''Movie''' || '''RHESSI''' || '''Quicklook Images''' || '''Comments''' | ||
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|18:42-18:44 ||Drifting pulsation structures || || | |18:42-18:44 ||Drifting pulsation structures || || [https://drive.google.com/open?id=1f5-MBgwHDHfWoMkifgxWgFxgJ2K8TAtu VLA movie] || [[:File:Feb19_Rhessi.png]] || [[:File:Feb19.png]] [[https://drive.google.com/open?id=161euS4JvUTRi8KEUC00Dsy3ITf15nKCZ 1843.png]] || Drifting pulsation structures in the dynamic spectrum that correspond to a peak in GOES derivative and RHESSI 6-12 keV light curve | ||
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Latest revision as of 22:16, 19 September 2018
Overview
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 NuSTAR. One C-class flares were covered: A C2.7 flare at the limb peaking at arounf 23:00 . File:20160219 sum.png
List of Events/Features
| Time | Feature | Event | Movie | RHESSI | Quicklook Images | Comments |
| 18:42-18:44 | Drifting pulsation structures | VLA movie | File:Feb19_Rhessi.png | File:Feb19.png [1843.png] | Drifting pulsation structures in the dynamic spectrum that correspond to a peak in GOES derivative and RHESSI 6-12 keV light curve |
