2024-09-10T00:28:03.761569Z http://sot.lmsal.com Mr. Sam Freeland Lockheed Martin Solar and Astrophysics Laboratory (LMSAL) http://www.lmsal.com Lockheed Martin ATC, 3251 Hanover St., Palo Alto, CA 94306 null null HINODE SOTSP Yasuda Y. Kato Shine 0 HOP 94 - Driving mechanism(s) of small scale transient brightenings in the solar atmosphere Disk Center Driving mechanism(s) of small scale transient brightenings in the solar atmosphere BP, DC 11 20090110_162043 145 170 178 11 32 400 2 1 1 0 2 22 2010 187 0.935 21.926 6.969 59.279 162.304 2009-01-10T16:20:43.000Z 2009-01-10T16:33:21.000Z 21.926 6.969 Driving mechanism(s) of small scale transient brightenings in the solar atmosphere Fast map, 60 arcsec FOV, 1-side CCD, no repeat 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.