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- 18:21, 30 January 2026 OVSA Science Highlight No. 7: Are Nonthermal Electrons Ubiquitously Present in the Quiet Middle Corona? (hist | edit) [3,794 bytes] Bchen (talk | contribs) (Created page with "''Contributed by '''Surajit Mondal'''<sup>1</sup> (<sup>1</sup>Center for Solar-Terrestrial Research, New Jersey Institute of Technology, 323 Martin Luther King Jr Blvd., Newark, NJ 07102-1982, USA); Edited by B. Chen. Posted on January 30, 2026. The answer is probably yes. However, we did not yet have direct evidence. While radio observations are very sensitive to the presence of nonthermal electrons compared to most other wavebands, detecting the emission from relativ...")
- 16:44, 30 January 2026 OVSA Science Highlight No. 8: Megaelectronvolt electrons in a coronal source of a solar flare (hist | edit) [3,480 bytes] Bchen (talk | contribs) (Created page with "''Contributed by '''Gregory Fleishman'''<sup>1</sup> (<sup>1</sup>Center for Solar-Terrestrial Research, New Jersey Institute of Technology, 323 Martin Luther King Jr Blvd., Newark, NJ 07102-1982, USA); Edited by B. Chen. Posted on January 30, 2026. Analysis of γ-rays in solar flares (blue spectral component in Fig. 1a) has suggested a distinct continuum component dominating at MeV energies (blue curve in Fig. 1b), which differs from the well-studied X-ray continuum (r...")
- 16:13, 7 January 2026 2026 (hist | edit) [12,208 bytes] Bchen (talk | contribs) (Created page with "== List of EOVSA Flares with Spectrogram Data == ===January=== {| class="wikitable" ! Date || Time (UT) || GOES Class || Position || TP Spectrogram || XP Spectrogram || STIX Coverage || AIA Movie || EOVSA Images || Comments |- | [http://ovsa.njit.edu/browser/?suntoday_date=2025-01-01 2025-01-01] || 18:11 || M1.2 || [https://www.lmsal.com/solarsoft/latest_events_archive/events_summary/2025/01/01/gev_20250101_1805/index.html N13W86] || File:eovsa.spec_tp.flare_id_2...")
- 20:19, 2 January 2026 2026 January (hist | edit) [13,683 bytes] Oweng (talk | contribs) (Created page with "== January 1 == Observer on duty: Owen Giersch {| class="wikitable" ! Start Time (UT) || Duration (min) || Antenna(s) || Comments/Reasons |- | 14:52 || 79 || 1, 3-8, 10-13 || Successful Reference calibration for bands < 45. Analysis written to SQL @2026-01-01 15:13 UT. |- | 17:22 || 16 || 1, 3-8, 10-13 || Successful Phase calibration. Analysis written to SQL. |- | 22:14 || 16 || 1, 3-8, 10-13 || Successful Phase calibration. Analysis written to SQL. |- | 00:06 (Jan 02)...")
- 18:16, 2 December 2025 2025 December (hist | edit) [17,471 bytes] CaiusSelhorst (talk | contribs) (Created page with "== December 1 == Observer on duty: Caius Selhorst {| class="wikitable" ! Start Time (UT) || Duration (min) || Antenna(s) || Comments/Reasons |- | 23:57 || 60 ||1, 3-8, 10-13 || Successful Reference calibration for between 7 and 42. Analysis written to SQL @2025-12-01 13:00 UT. |- | 17:14 || 16 || 1, 3-8, 10-11, 13 || Successful Phase calibration. Analysis written to SQL. |- |} ==== Outages ==== {| class="wikitable" ! Start Time (UT) || End Time (UT) || Antenna(s) ||...")