Expanded Owens Valley Solar Array: Difference between revisions
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; 2018 | ; 2018 | ||
: [https://ui.adsabs.harvard.edu/#abs/2018ApJ...864...63P/abstract Polito et al. (2018) 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) | : [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:// | : [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 |
Revision as of 12:43, 1 December 2018
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
- General
- Computer-Network
- Control System
- Hardware
- Calibration
Using EOVSA Data
- Software Basics
- EOVSA Data Analysis Guide
- EOVSA Modeling Guide
System Software
- LabVIEW software
- Python code Github repository
Observing Log
Tohbans
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