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Show new changes starting from 22:33, 1 February 2026
   
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30 January 2026

N    19:14  OVSA Science Highlight No. 8: Megaelectronvolt electrons in a coronal source of a solar flare‎‎ 6 changes history +3,480 [Bchen‎ (6×)]
     
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16:44 (cur | prev) +3,098 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...")
     19:07  (Upload log) [Bchen‎ (2×)]
     
19:07 Bchen talk contribs uploaded File:OVSA SH 7 Mondal title.jpeg(The Sun's middle corona as generated by Gemini 3 pro's nano banana model.)
     
16:37 Bchen talk contribs uploaded File:OVSA SH 8 fleishman title.jpeg(Generated by Google Gemini 3.0 pro with nano banana pro.)
N    18:50  OVSA Science Highlight No. 7: Are Nonthermal Electrons Ubiquitously Present in the Quiet Middle Corona?‎‎ 4 changes history +3,794 [Bchen‎ (4×)]
     
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18:21 (cur | prev) +2,364 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...")