Difference between revisions of "EOVSA Data products"

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=Data Definition=
 
=Data Definition=
 
==Level 0==
 
==Level 0==
===Raw visibility data from the instrument===
+
Raw visibility data from the instrument
 
==Level 1==
 
==Level 1==
===Calibrated visibility data, which have all of the required content to produce Level 2 data products===
+
Calibrated visibility data, which have all of the required content to produce Level 2 data products
====CASA 1-min averaged ms====
+
===CASA 1-min averaged ms===
====CASA Event ms====
+
===CASA Event ms===
 
==Level 2==
 
==Level 2==
 
Images and spectrogram data in standard FITS format
 
Images and spectrogram data in standard FITS format
 
===All-day TP spectrum===
 
===All-day TP spectrum===
** All-day XP spectrum
+
===All-day XP spectrum===
** Synoptic 6-band Images
+
===Synoptic 6-band Images===
** 10-min 6-band Images
+
===10-min 6-band Images===
** Event images
+
===Event images===
  
  

Revision as of 14:52, 23 March 2020

Welcome to the EOVSA data products documentation. EOVSA observes the full disk of the Sun at all times when the Sun is >10 degrees above the local horizon, which is season dependent and ranges from 7-12 hours duration centered on 20 UT. During January, coverage will be 16-24 UT daily, 7 days/week. EOVSA will provide microwave spectra and imaging at up to 451 frequencies between 1 and 18 GHz. We deliver the radio interferometry data in level 0-2.

Pipeline flowchart.jpg

Data Definition

Level 0

Raw visibility data from the instrument

Level 1

Calibrated visibility data, which have all of the required content to produce Level 2 data products

CASA 1-min averaged ms

CASA Event ms

Level 2

Images and spectrogram data in standard FITS format

All-day TP spectrum

All-day XP spectrum

Synoptic 6-band Images

10-min 6-band Images

Event images

Full disk images at 6 selected frequency bands centered at 1.4, 3.0, 4.5, 6.8, 10.2, and 13.9 GHz will be provided once per day, calibrated in brightness temperature. Total power full-Sun-integrated spectrograms calibrated in solar flux units will be provided at 451 frequencies and 1 s time resolution. Similar cross-power spectrograms will also be provided, which have much better sensitivity to weak bursts. EOVSA will also provide quick look images and spatially-resolved microwave spectra of any bursts that are identified in the cross-power spectra. Such spatially-resolved spectra can be analyzed to provide quantitative diagnostics of the magnetic field, plasma, and particle energy parameters in the burst source.



All-day TP spectrum

The all-day TP spectrum provides a daily dynamic spectrum of the sun-integrated flux in the broad frequency range 1-18 GHz at up to 451 science frequency channels with a cadence of 1 s.

TPSP.jpeg

All-day XP spectrum

The all-day XP spectrum provides a daily dynamic spectrum of mean flux from baselines with "intermediate" lengths in the broad frequency range 1-18 GHz at up to 451 science frequency channels with a cadence of 1 s.

XPSP.jpeg

Synoptic 6-band Images

Full disk images at 6 selected frequency bands centered at 1.4, 3.0, 4.5, 6.8, 10.2, and 13.9 GHz will be provided once per day, calibrated in brightness temperature.
Synoptic image.jpg

All-day 1-min avg. visibility