Difference between revisions of "Expanded Owens Valley Solar Array"

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(Observing Log)
(EOVSA Publications)
 
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**[[Total Power Calibration]]
 
**[[Total Power Calibration]]
 
**[[System Gain Calibration]]
 
**[[System Gain Calibration]]
 +
**[[Antenna Position]] (Baseline Calibration)
 
**[[Reference Gain Calibration]]
 
**[[Reference Gain Calibration]]
 
**[[Daily Gain Calibration]]
 
**[[Daily Gain Calibration]]
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**[[Bandpass Calibration]]
 
**[[Bandpass Calibration]]
 
**[[Polarization Calibration]]
 
**[[Polarization Calibration]]
**[[Antenna Position]]
 
 
**[[Calibrator Survey]]
 
**[[Calibrator Survey]]
  
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** [[Imaging]]
 
** [[Imaging]]
 
**[[Flare Imaging]]
 
**[[Flare Imaging]]
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**[https://sites.google.com/site/fgscodes/ Fast Gyrosynchrotron Codes (Alexey Kuznetsov's website)]
  
 
* <big>EOVSA Modeling Guide</big>
 
* <big>EOVSA Modeling Guide</big>
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[[Tohban Records]]
 
[[Tohban Records]]
  
== Flare List ==
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== EOVSA Flare List ==
  
See [http://ovsa.njit.edu/jay/rd_db.php this link] for a more updated version of EOVSA flare list.  
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See [https://docs.google.com/spreadsheets/d/1P8jHuDRF93dMflU6RMQcsJqVepD9vFkPkofV8Imj4xA/edit?usp=sharing this link] for a list of EOVSA flares as a Google Spreadsheet.
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 +
[http://ovsa.njit.edu/jay/rd_db.php Another link] available at the EOVSA website.  
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| January 25, 2017 || 21:27:14 || [http://hessi.ssl.berkeley.edu/hessidata/metadata/2017/01/25/hsi_20170125_204400_corrected_rate.png Lightcurve] || [http://ovsa.njit.edu/flaremon/XSP20170125200011.png XSP] || Yes || 12 - 25 || 21:26:57 || || B8.5 || [[:File:UDB20170125200025.png | Plot]]
 
| January 25, 2017 || 21:27:14 || [http://hessi.ssl.berkeley.edu/hessidata/metadata/2017/01/25/hsi_20170125_204400_corrected_rate.png Lightcurve] || [http://ovsa.njit.edu/flaremon/XSP20170125200011.png XSP] || Yes || 12 - 25 || 21:26:57 || || B8.5 || [[:File:UDB20170125200025.png | Plot]]
 
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== EOVSA Publications ==
 
== EOVSA Publications ==
 +
Here is a list of publications that utilizes EOVSA data.
  
This is the list of links to the publications (including posters) related to EOVSA.
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; 2018
 
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: [https://ui.adsabs.harvard.edu/#abs/2018ApJ...864...63P/abstract 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
[https://drive.google.com/open?id=14pg4PvsPdVMki8LpZUoNRQVxkysEl1Rt Kuroda et al. (2018): “Three-dimensional Forward-fit Modeling of the Hard X-ray and the Microwave Emissions of the 2015 June 22 M6.5 flare”, ApJ, 852, 32]
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: [https://ui.adsabs.harvard.edu/#abs/2018ApJ...863...83G/abstract Gary et al. (2018), ApJ, 863, 83] Microwave and Hard X-Ray Observations of the 2017 September 10 Solar Limb Flare
 +
: [https://ui.adsabs.harvard.edu/#abs/2018ApJ...852...32K/abstract 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

Latest revision as of 12:43, 1 December 2018

Eovsa1.png

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

2016 December

2017 January

2017 February

2017 March

2017 April

2017 May

2017 June

2017 July

2017 August

2017 September

2017 October

2017 November

2017 December

2018 January

2018 February

2018 March

2018 April

2018 July

Tohbans

Trouble Shooting Guide

Tohban Records

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 list of publications that utilizes EOVSA data.

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