Difference between revisions of "Expanded Owens Valley Solar Array"

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== Using EOVSA Data  ==
 
== Using EOVSA Data  ==
 
* <big>[[EOVSA Data products]]</big>
 
* <big>[[EOVSA Data products]]</big>
** [http://www.ovsa.njit.edu/wiki/index.php/EOVSA_Data_products#All-day_TP_spectrum All-day TP spectrum]
 
** [http://www.ovsa.njit.edu/wiki/index.php/EOVSA_Data_products#All-day_XP_spectrum All-day XP spectrum]
 
** [http://www.ovsa.njit.edu/wiki/index.php/EOVSA_Data_products#Synoptic_7-band_Images Synoptic 7-band Images]
 
** [http://www.ovsa.njit.edu/wiki/index.php/EOVSA_Data_products#All-day_1-min_avg._visibility All-day 1-min avg. visibility]
 
 
* <big>Analysis Software</big>
 
* <big>Analysis Software</big>
 
** [https://github.com/suncasa/suncasa SunCASA] A wrapper around [https://casa.nrao.edu/ CASA (the Common Astronomy Software Applications package)] for synthesis imaging and visualizing solar spectral imaging data. CASA is one of the leading software tool for "supporting the data post-processing needs of the next generation of radio astronomical telescopes such as ALMA and VLA", an international effort led by the [https://public.nrao.edu/ National Radio Astronomy Observatory]. The current version of CASA uses Python (2.7) interface. More information about CASA can be found on [https://casa.nrao.edu/ NRAO's CASA website ]. Note, CASA is available ONLY on UNIX-BASED PLATFORMS (and therefore, so is SunCASA).  
 
** [https://github.com/suncasa/suncasa SunCASA] A wrapper around [https://casa.nrao.edu/ CASA (the Common Astronomy Software Applications package)] for synthesis imaging and visualizing solar spectral imaging data. CASA is one of the leading software tool for "supporting the data post-processing needs of the next generation of radio astronomical telescopes such as ALMA and VLA", an international effort led by the [https://public.nrao.edu/ National Radio Astronomy Observatory]. The current version of CASA uses Python (2.7) interface. More information about CASA can be found on [https://casa.nrao.edu/ NRAO's CASA website ]. Note, CASA is available ONLY on UNIX-BASED PLATFORMS (and therefore, so is SunCASA).  
 
** [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]
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== EOVSA Publications ==
 
== EOVSA Publications ==
Here is a (partial) list of publications that utilizes EOVSA data.
+
Here is a (partial) list of publications that utilize EOVSA data.
  
 +
; 2020
 +
: [https://ui.adsabs.harvard.edu/abs/2020arXiv200710443Y/abstract Yu et al. (2020), ApJ, in press] ''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''
 +
: [https://ui.adsabs.harvard.edu/abs/2020arXiv200512757C/abstract Chen et al. (2020b), Nature Astronomy, Jul 27, 2397] ''Measurement of magnetic field and relativistic electrons along a solar flare current sheet''
 +
: [https://ui.adsabs.harvard.edu/abs/2020ApJ...895L..50C/abstract Chen et al. (2020a), ApJL, 895, 50] ''Microwave Spectral Imaging of an Erupting Magnetic Flux Rope: Implications for the Standard Solar Flare Model in Three Dimensions''
 +
: [https://ui.adsabs.harvard.edu/abs/2020arXiv200413155K/abstract Kuroda et al. (2020), Frontiers, 7, 22] ''Evolution of Flare-accelerated Electrons Quantified by Spatially Resolved Analysis''
 +
: [https://ui.adsabs.harvard.edu/abs/2020ApJ...891L..34G/abstract Glesener et al. (2020), ApJL, 891, 34] ''Accelerated Electrons Observed Down to <7 keV in a NuSTAR Solar Microflare''
 +
: [https://ui.adsabs.harvard.edu/abs/2020ApJ...889...72K/abstract Karlicky at al. (2020), ApJ, 889, 72] ''Drifting Pulsation Structure at the Very Beginning of the 2017 September 10 Limb Flare''
 +
: [https://ui.adsabs.harvard.edu/abs/2020Sci...367..278F/abstract Fleishman et al. (2020), Science, 367, 278] ''Decay of the coronal magnetic field can release sufficient energy to power a solar flare''
 +
: [https://aas235-aas.ipostersessions.com/default.aspx?s=97-69-9E-4B-34-19-68-53-1B-C6-21-0C-16-1C-5C-82&guestview=true Gary et al. (2020) AAS iPoster] ''A new view of the solar atmosphere: daily full-disk multifrequency radio images from EOVSA''
 
; 2018
 
; 2018
: [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://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://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...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
+
: [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''
 +
; 2016
 +
: [https://ui.adsabs.harvard.edu/abs/2016JAI.....541009N/abstract 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 ==
 
== VLA Flare List ==
 
See [http://www.ovsa.njit.edu/wiki/index.php/VLA_Data_Survey#List_of_Jansky_VLA_Solar_Observations this link] for a list of VLA flare observations.
 
See [http://www.ovsa.njit.edu/wiki/index.php/VLA_Data_Survey#List_of_Jansky_VLA_Solar_Observations this link] for a list of VLA flare observations.

Latest revision as of 18:05, 21 August 2020

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; 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 press 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), Nature Astronomy, Jul 27, 2397 Measurement of magnetic field and relativistic electrons along a solar flare current sheet
Chen et al. (2020a), ApJL, 895, 50 Microwave Spectral Imaging of an Erupting Magnetic Flux Rope: Implications for the Standard Solar Flare Model in Three Dimensions
Kuroda et al. (2020), Frontiers, 7, 22 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.