VLA 20160219

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

• link to VLA overview movie:

• AIA movie:http://www.lmsal.com/hek/hcr?cmd=view-event&event-id=ivo%3A%2F%2Fsot.lmsal.com%2FVOEvent%23VOEvent_SSW_cutout_20160219T2244-20160219T2333_AIA_131-193-171_S23E87_ssw_cutout_20160219_224411_aia_171_S23E872016-02-19T22%3A44%3A00.000.xml AIA movie on the limb C2.7flare http://www.lmsal.com/hek/hcr?cmd=view-event&event-id=ivo%3A%2F%2Fsot.lmsal.com%2FVOEvent%23VOEvent_ssw_cutout_20160219_180006_aia_4500_2016-02-19T17%3A53%3A10.000.xml AIA movie on the limb at 18:00

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 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

Migrated from MediaWiki page VLA 20160219, latest revision 2637 (2018-09-19T22:16:56Z).