2024-09-24T22:21:33.000Z 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 Yasuda Y. Kato Shine 0 HOP 94 disk center, Quiet Sun HOP 94 DC 1 20090110_140042 187 210 223 1 13 1024 2 1 1 2 0 22 2010 511 0.998046875 1.83 6.906 161.987 162.304 2009-01-10T14:00:42.000Z 2009-01-10T14:33:04.000Z 1.83 6.906 HOP 94 Fast map 164x164", Q65, 1 side NaI 5896 FGIV magnetograms - 1/min H-alpha 6563/SOT - 1/min The aim of this study is to determine the driving mechanism(s) behind these events as well as to study their coronal responses. For this, it is crucial to obtain the plasma parameters of these events and their magnetic topology. From EIS data, we can derive the densities, temperatures and Doppler shifts of the associated plasma. Highly coordinated observations such as magnetograms and Halpha images from SOT along with XRT will give a clue on the unification of classified transients for instance like blinkers and spicules/macro-spicules/jets along with CDS/SoHO, the later of which is necessary in the identification of the already known blinkers.;;Driving mechanisms of small scale transient brightenings in the solar atmosphere. HOP 94 (MDI 13:42-16:55) 2009/01/10 11:24:00 - 2009/01/10 17:00:00 pointing: (-25,0) tracking FG03 (0x02b4) Na IVDG 61x164", 2x2, for HOP 94 SP11 (0x0091) Fast map, 60 arcsec FOV, 1-side CCD, no repeat SP01 (0x00bb) Fast map 164x164", Q65, 1 side SP11 (0x0091) Fast map, 60 arcsec FOV, 1-side CCD, no repeat ivo://sot.lmsal.com/VOEvent#2009-01-10T14:00:00Z