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Combined display of all available logs of EOVSA Wiki. You can narrow down the view by selecting a log type, the username (case-sensitive), or the affected page (also case-sensitive).
(newest | oldest) View (newer 50 | older 50) (20 | 50 | 100 | 250 | 500)- 10:23, 30 April 2026 Bchen talk contribs created page File:OVSA SH 9 Kaltman title.jpeg
- 10:23, 30 April 2026 Bchen talk contribs uploaded File:OVSA SH 9 Kaltman title.jpeg
- 10:14, 30 April 2026 Bchen talk contribs created page File:OVSA HL9 Kaltman fig2.jpg
- 10:14, 30 April 2026 Bchen talk contribs uploaded File:OVSA HL9 Kaltman fig2.jpg
- 10:14, 30 April 2026 Bchen talk contribs created page File:OVSA HL9 Kaltman fig1.jpg
- 10:14, 30 April 2026 Bchen talk contribs uploaded File:OVSA HL9 Kaltman fig1.jpg
- 10:12, 30 April 2026 Bchen talk contribs created page OVSA Science Highlight No. 9: Inferring Alfvén Speed and Plasma Beta in 3D (Created page with "''Contributed by '''Tatyana Kaltman'''<sup>1</sup> (<sup>1</sup>1Institut für Sonnenphysik (KIS), Georges-Köhler-Allee 401 A, D-79110 Freiburg, Germany); Edited by S. Yu. Posted on April 30, 2026. Measurements of the magnetic field in solar flares remain one of the major challenges in solar physics. Microwave imaging spectroscopy with the Expanded Owens Valley Solar Array (EOVSA) offers a unique way to diagnose the coronal magnetic field through gyrosynchrotron emissi...")
- 02:54, 30 April 2026 Asingh talk contribs created page File:FlareID FL 20260425170400 20260425T170458 3-10GHz.png
- 02:54, 30 April 2026 Asingh talk contribs uploaded File:FlareID FL 20260425170400 20260425T170458 3-10GHz.png
- 02:46, 30 April 2026 Asingh talk contribs created page File:Eovsa.spec xp.flare id 202604251704.png
- 02:46, 30 April 2026 Asingh talk contribs uploaded File:Eovsa.spec xp.flare id 202604251704.png