2026-10-01T18:36:43.000Z http://sot.lmsal.com Mr. Sam Freeland Lockheed Martin Solar and Astrophysics Laboratory (LMSAL) http://www.lmsal.com Lockheed Martin Advanced Tech Center, 3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA 94304 null null HINODE SOTSP Arai Arai Tiwari(RCO) 528 HOP 528, AR obs. Active Region AR AR 13 20260919_124905 373 401 402 13 70 1024 2 1 1 2 0 21 2023 509 0.994141 352.436 -328.97 161.353 162.304 2026-09-19T12:49:05.000Z 2026-09-19T13:21:27.000Z 352.436 -328.97 Dynamics of the bright points in the corona and in the low atmosphere Fast map, 164x164", 1-side, Q65, no repeat SSC Point of Contact: General: Adam Kobelski, Jessie Duncan (NASA/MSFC) / Tetsuya Watanabe (NAOJ) / Bart De Pontieu (LMSAL), SOT -- Marc DeRosa/Dick Shine (LMSAL), XRT -- Katharine Reeves/Paola Testa (SAO), EIS -- Sarah Matthews/Len Culhane (UCL/MSSL) Main Objective: The objective is to measure the Dopplershifts at different altitudes (temperatures) using a range of emission lines. Scientific Justification: Bright points are ubiquitous: in EMF, in decaying AR, in CHs. With THEMIS we measured large Dopplershifts in Halpha (Karki et al 2025). We would like to study the Dopplershifts in hotter lines with IRIS and EIS, and determine the magnetic configuration with SOT. ivo://sot.lmsal.com/VOEvent#2026-09-19T12:49:00Z