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- 18:16, 2 December 2025 2025 December (hist | edit) [1,170 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) ||...")
- 15:46, 2 November 2025 2025 November (hist | edit) [7,405 bytes] Oweng (talk | contribs) (Created page with "== November 1 == Observer on duty: Owen Giersch {| class="wikitable" ! Start Time (UT) || Duration (min) || Antenna(s) || Comments/Reasons |- | 11:12 || 60 ||1, 3-8, 10-13 || Successful Reference calibration for all > 7. Analysis written to SQL @2025-10-31 11:16 UT. |- | 17:14 || 16 || 1, 3-8, 10-12 || Successful Phase calibration. Analysis written to SQL. |- | 00:52 (Nov 2) || 60 || 3,4,6,12 || Successful Phase calibration. Analysis written to SQL. |- |} ==== Outage...")
- 16:42, 2 October 2025 2025 October (hist | edit) [16,950 bytes] CaiusSelhorst (talk | contribs) (Created page with "== October 1 == Observer on duty: Caius Selhorst {| class="wikitable" ! Start Time (UT) || Duration (min) || Antenna(s) || Comments/Reasons |- | 12:53 || 79 || 1, 4-8, 10-13 || Successful Reference calibration for all bands. Analysis written to SQL @2025-10-01 13:18 UT. |- | 02:54 (Oct 02) || 60 || 1, 4-8, 10-13 || Successful Phase calibration. Analysis written to SQL. |- |} ==== Outages ==== {| class="wikitable" ! Start Time (UT) || End Time (UT) || Antenna(s) || Com...")
- 17:51, 26 September 2025 OVSA Science Highlight No. 6: Detection of Radio Gyroresonance Emission from a CME (hist | edit) [6,883 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 September 26, 2025. The space weather potential of a coronal mass ejection (CME) depends significantly on its magnetic field. Hence, considerable effort has been invested in developing various techniques to measure the CME magnetic field. Radio...")
- 16:55, 19 September 2025 OVSA Science Highlight No. 5: Is CME's Magnetic Flux Conserved? (hist | edit) [4,239 bytes] Bchen (talk | contribs) (Created page with "''Contributed by '''Xingyao Chen'''<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. Probably yes, if a magnetic flux rope truly comprises the “core” of the CME. However, we have not had direct proof heretofore. One of the main challenges is to measure the magnetic field of a CME itself, let alone track its evolution during the eruptio...")
- 12:14, 11 September 2025 OVSA Science Highlight No. 4: When the Sun Meets the Crab (hist | edit) [4,606 bytes] Bchen (talk | contribs) (Created page with "''Contributed by '''Peijin Zhang'''<sup>1, 2</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; <sup>2</sup>)Cooperative Programs for the Advancement of Earth System Science, University Corporation for Atmospheric Research, Boulder, CO, USA'' Being situated in the Zodiac constellation Taurus, the [https://en.wikipedia.org/wiki/Crab_Nebula Crab Nebula] (also known as...")