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(newest | oldest) View (newer 50 | older 50) (20 | 50 | 100 | 250 | 500)- 20:55, 21 October 2025 User account Mwieber talk contribs was created by Bchen talk contribs
- 17:52, 26 September 2025 Bchen talk contribs uploaded File:SMondal2025 fig3.jpg
- 17:52, 26 September 2025 Bchen talk contribs created page File:SMondal2025 fig3.jpg
- 17:51, 26 September 2025 Bchen talk contribs uploaded File:SMondal2025 fig2.jpg
- 17:51, 26 September 2025 Bchen talk contribs created page File:SMondal2025 fig2.jpg
- 17:51, 26 September 2025 Bchen talk contribs uploaded File:SMondal2025 fig1.jpg
- 17:51, 26 September 2025 Bchen talk contribs created page File:SMondal2025 fig1.jpg
- 17:51, 26 September 2025 Bchen talk contribs created page OVSA Science Highlight No. 6: Detection of Radio Gyroresonance Emission from a CME (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...")
- 17:32, 26 September 2025 Bchen talk contribs created page File:Cme 20240309.jpeg
- 17:32, 26 September 2025 Bchen talk contribs uploaded File:Cme 20240309.jpeg
- 16:58, 19 September 2025 Bchen talk contribs created page File:XChen2025 fig1.jpg
- 16:58, 19 September 2025 Bchen talk contribs uploaded File:XChen2025 fig1.jpg
- 16:55, 19 September 2025 Bchen talk contribs created page OVSA Science Highlight No. 5: Is CME's Magnetic Flux Conserved? (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...")
- 13:34, 19 September 2025 Bchen talk contribs created page File:Cme mfr.jpeg (From [https://iopscience.iop.org/article/10.3847/2041-8213/adfa71 X. Chen et al. 2025, ApJ])
- 13:34, 19 September 2025 Bchen talk contribs uploaded File:Cme mfr.jpeg (From [https://iopscience.iop.org/article/10.3847/2041-8213/adfa71 X. Chen et al. 2025, ApJ])
- 17:41, 11 September 2025 Bchen talk contribs moved page OVRO-LWA Data Products to OVRO-LWA Solar Data Products
- 12:15, 11 September 2025 Bchen talk contribs uploaded File:PZhang2025 fig2.jpg
- 12:15, 11 September 2025 Bchen talk contribs created page File:PZhang2025 fig2.jpg
- 12:15, 11 September 2025 Bchen talk contribs uploaded File:PZhang2025 fig1.jpg
- 12:15, 11 September 2025 Bchen talk contribs created page File:PZhang2025 fig1.jpg
- 12:14, 11 September 2025 Bchen talk contribs created page OVSA Science Highlight No. 4: When the Sun Meets the Crab (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...")
- 11:52, 11 September 2025 Bchen talk contribs uploaded File:Crab solar conjunction.jpeg (Generated by Google Gemini 2.5 pro, based on Fig. 6 of Hewish 1958 (https://ui.adsabs.harvard.edu/abs/1958MNRAS.118..534H).)
- 11:52, 11 September 2025 Bchen talk contribs created page File:Crab solar conjunction.jpeg (Generated by Google Gemini 2.5 pro, based on Fig. 6 of Hewish 1958 (https://ui.adsabs.harvard.edu/abs/1958MNRAS.118..534H).)
- 23:49, 3 September 2025 User account Mwickline talk contribs was created by Bchen talk contribs (New account for Mallory Wickline)
- 23:48, 3 September 2025 User account Lseyfritz talk contribs was created by Bchen talk contribs (New account for Louis Seyfritz)
- 23:45, 3 September 2025 User account Asingh talk contribs was created by Bchen talk contribs (New account for Anshika Singh)
- 19:19, 22 August 2025 Bchen talk contribs moved page EOVSA Data Policy to OVSA Data Policy
- 09:27, 22 August 2025 Bchen talk contribs uploaded a new version of File:OVRO-LWA data product flowchart.png
- 18:20, 21 August 2025 Bchen talk contribs uploaded a new version of File:OVRO-LWA data product flowchart.png
- 11:10, 20 August 2025 Bchen talk contribs created page File:Fleishman2025 fig2.jpg
- 11:10, 20 August 2025 Bchen talk contribs uploaded File:Fleishman2025 fig2.jpg
- 11:09, 20 August 2025 Bchen talk contribs created page File:Fleishman2025 fig1.jpg
- 11:09, 20 August 2025 Bchen talk contribs uploaded File:Fleishman2025 fig1.jpg
- 11:09, 20 August 2025 Bchen talk contribs created page OVSA Science Highlight No. 3: The First EOVSA "Cold" Solar Flare (Created page with "''Contributed by '''Gregory Fleishman'''<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>Institut für Sonnenphysik (KIS), Georges-Köhler-Allee 401 A, D-79110 Freiburg, Germany)'' File:Fleishman2025_fig1.jpg|thumb|Fig. 1: A subset of inferred flare parameters and their evolution. Top row: magnetic field strength. Bottom row: nonthermal elec...")
- 10:59, 20 August 2025 Bchen talk contribs uploaded a new version of File:Cold flare.jpeg (Smaller size)
- 10:57, 20 August 2025 Bchen talk contribs created page File:Cold flare.jpeg (Illustration generated by Google Gemini 2.5pro)
- 10:57, 20 August 2025 Bchen talk contribs uploaded File:Cold flare.jpeg (Illustration generated by Google Gemini 2.5pro)
- 15:31, 19 August 2025 Bchen talk contribs created page File:SEP illustration gemini.jpeg (This is an illustration of a solar energetic particle event generated by Google Gemini 2.5 pro.)
- 15:31, 19 August 2025 Bchen talk contribs uploaded File:SEP illustration gemini.jpeg (This is an illustration of a solar energetic particle event generated by Google Gemini 2.5 pro.)
- 15:17, 19 August 2025 Bchen talk contribs created page File:Wang2025 fig3.jpg
- 15:17, 19 August 2025 Bchen talk contribs uploaded File:Wang2025 fig3.jpg
- 15:17, 19 August 2025 Bchen talk contribs uploaded File:Wang2025 fig2.jpg
- 15:17, 19 August 2025 Bchen talk contribs created page File:Wang2025 fig2.jpg
- 15:15, 19 August 2025 Bchen talk contribs uploaded File:Wang2025 fig1.jpg
- 15:15, 19 August 2025 Bchen talk contribs created page File:Wang2025 fig1.jpg
- 15:14, 19 August 2025 Bchen talk contribs created page OVSA Science Highlight No. 2: Two Phases of Impulsive SEP Acceleration (Created page with "''Contributed by '''Meiqi Wang''' (Center for Solar-Terrestrial Research, New Jersey Institute of Technology, 323 Martin Luther King Jr Blvd., Newark, NJ 07102-1982, USA)'' File:Wang2025_fig1.jpg|thumb|Time history of the 2021 July 3 event. (a) Electron count rate observed by PSP/ISOIS. (b) GOES 1–8 Å soft X-ray light curve. The X1.5 flare at 14:29 UT is the focus of this study. (c) EOVSA microwave dynamic spectrum of the X1.5 flare. (d) HXR light curves observed...")
- 19:04, 2 August 2025 Bchen talk contribs deleted page OVSA Science Highlight (content was: "== #1: Microwave Precursor of a Major Solar Eruption == ''Contributed by '''Yuankun Kou'''<sup>1,2,3</sup> (<sup>1</sup> School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China; <sup>2</sup> Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, China; <sup>3</sup> School of Physics and Astronomy, Un...", and the only contributor was "Bchen" (talk))
- 19:03, 2 August 2025 Bchen talk contribs deleted page No. 1: Microwave Precursor of a Major Solar Eruption (content was: " ''Contributed by '''Yuankun Kou'''<sup>1,2,3</sup> (<sup>1</sup> School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China; <sup>2</sup> Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, China; <sup>3</sup> School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK)'' File:kou...", and the only contributor was "Bchen" (talk))
- 19:00, 2 August 2025 Bchen talk contribs created page OVSA Science Highlight No. 1: Microwave Precursor of a Major Solar Eruption (Created page with "''Contributed by '''Yuankun Kou'''<sup>1,2,3</sup> (<sup>1</sup> School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China; <sup>2</sup> Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, China; <sup>3</sup> School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK)'' File:kou2025_fig1.jpg|thumb|Microwave sources overlaying on SDO/AIA 131 Å images during the precur...")
- 18:59, 2 August 2025 Bchen talk contribs created page No. 1: Microwave Precursor of a Major Solar Eruption (Created page with "== OVSA Science Highlight No. 1: Microwave Precursor of a Major Solar Eruption == ''Contributed by '''Yuankun Kou'''<sup>1,2,3</sup> (<sup>1</sup> School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China; <sup>2</sup> Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, China; <sup>3</sup> School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK)'' File:kou2025_fig...")
