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 Arikawa Kano Shine 94 HOP 94 disk center Driving mechanism(s) of small scale transient brightenings in the solar atmosphere DC 11 20090113_172306 145 170 178 11 32 400 2 1 1 2 0 22 2010 192 0.96 31.045 7.172 60.864 162.304 2009-01-13T17:23:06.000Z 2009-01-13T17:35:43.000Z 31.045 7.172 Driving mechanism(s) of small scale transient brightenings in the solar atmosphere Fast map, 60 arcsec FOV, 1-side CCD, no repeat 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. We will also review the coronal response of the features named blinkers, by using simultaneous CDS and EIS observations. Request to SOT HOP Number 0094 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. We will also review the coronal response of the features named blinkers, by using simultaneous CDS and EIS observations. Request to SOT HOP Number 0094 NaI 5896 FGIV magnetograms - 1/min H-alpha 6563/SOT - 1/min ivo://sot.lmsal.com/VOEvent#2009-01-13T17:23:00Z