Expanded Owens Valley Solar Array: Difference between revisions

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** [https://github.com/Gelu-Nita/GSFIT GSFIT] A IDL-widget(GUI)-based spectral fitting package called gsfit, which provides a user-friendly display of EOVSA image cubes and an interface to fast fitting codes (via platform-dependent shared-object libraries).  
** [https://github.com/Gelu-Nita/GSFIT GSFIT] A IDL-widget(GUI)-based spectral fitting package called gsfit, which provides a user-friendly display of EOVSA image cubes and an interface to fast fitting codes (via platform-dependent shared-object libraries).  
** [[Spectrogram Software]]
** [[Spectrogram Software]]
** [[Mapping Software]]
* <big>Data Analysis Guides</big>
* <big>Data Analysis Guides</big>
** <big>[[EOVSA Data Analysis Tutorial]]</big> at [http://rhessi18.umn.edu/ RHESSI XVIII Workshop]
** <big>[[EOVSA Data Analysis Tutorial]]</big> at [http://rhessi18.umn.edu/ RHESSI XVIII Workshop]

Revision as of 01:06, 10 June 2020

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EOVSA (Expanded Owens Valley Solar Array) is a new solar-dedicated radio interferometer operated by the New Jersey Institute of Technology. This wiki serves as the site for EOVSA documentation.

EOVSA Documentation

Using EOVSA Data

System Software

Observing Log

2016 November; December

2017 January; February; March; April; May; June; July; August; September; October; November; December

2018 January; February; March; April; May; June; July; August; September; October; November; December

2019 January; February; March; April; May; June; July; August; September; October; November; December

2020 January; February; March; April; May; June; July; August; September; October; November; December

Tohbans

Trouble Shooting Guide

Tohban Records

Owen's Notes

EOVSA Flare List

See this link for a list of EOVSA flares as a Google Spreadsheet.

Another link available at the EOVSA website.


EOVSA Publications

Here is a (partial) list of publications that utilize EOVSA data.

2020
Yu et al. (2020), ApJ, in preparation (check back later for link) Magnetic Reconnection During the Post Impulsive Phase of the X8.2 Solar Flare: Bi-Directional Outflows as a Cause of Microwave and X-ray Bursts
Chen et al. (2020b), submitted Measurement of magnetic field and relativistic electrons along a solar flare current sheet
Chen et al. (2020a), ApJL, in press Microwave Spectral Imaging of an Erupting Magnetic Flux Rope: Implications for the Standard Solar Flare Model in Three Dimensions
Kuroda et al. (2020), Frontiers, in press Evolution of Flare-accelerated Electrons Quantified by Spatially Resolved Analysis
Glesener et al. (2020), ApJL, 891, 34 Accelerated Electrons Observed Down to <7 keV in a NuSTAR Solar Microflare
Karlicky at al. (2020), ApJ, 889, 72 Drifting Pulsation Structure at the Very Beginning of the 2017 September 10 Limb Flare
Fleishman et al. (2020), Science, 367, 278 Decay of the coronal magnetic field can release sufficient energy to power a solar flare
Gary et al. (2020) AAS iPoster A new view of the solar atmosphere: daily full-disk multifrequency radio images from EOVSA
2018
Polito et al. (2018), ApJ, 864, 63 Broad Non-Gaussian Fe XXIV Line Profiles in the Impulsive Phase of the 2017 September 10 X8.3-class Flare Observed by Hinode/EIS
Gary et al. (2018), ApJ, 863, 83 Microwave and Hard X-Ray Observations of the 2017 September 10 Solar Limb Flare
Kuroda et al. (2018), ApJ, 852, 32 Three-dimensional Forward-fit Modeling of the Hard X-ray and the Microwave Emissions of the 2015 June 22 M6.5 flare
2016
Nita et al. (2016), J. Astron. Instr., 5, 1641009-7366 EOVSA Implementation of a Spectral Kurtosis Correlator for Transient Detection and Classification

VLA Flare List

See this link for a list of VLA flare observations.