PPT-Team Report Flare Dynamics in the Lower Solar Atmosphere

Joel Allred NASA GSFC Team 1 Phil Judge HAO amp Lucia Kleint Original PI Team 2 Alexander Kosovichev NJITStanford Team 3 Chang Liu NJITTeam 4. the Earth on solar EUV observations from LEO satellites . V. Slemzin. 1. , A. Ulyanov. 1. , S. Kuzin. 1. , K. Gaikovitch. 2. , D. Berghmans. 3. , M. Dominique. 3. , B. Nicula. 3. , F. Hourrier. . on Solar type Stars and Their Impacts on Habitability of . Exoplanets. Kazunari. Shibata. . Kwasan. and . Hida. observatories, . Kyoto University. Hiroaki Isobe. Unit of Synergetic Studies for Space, Kyoto University. Ch 27. Questions??. What are some theories about how our solar system began?. The Nebular Hypothesis. solar nebular. a rotating cloud of gas and dust from which the sun and planets formed. In 1796, French mathematician . Individual . AR example: 8910. The only selection criterion imposed in this study is that the AR must be within 30 degrees of disk center. to minimize projection errors. See right for description of . Stars, solar systems form within giant molecular clouds. Requires . high density. , . dust, and low temperatures. to initiate gravitational . collapse. Most material is hydrogen and helium; only a few percent is other elements. ?. Implications from observations of solar-type stars . and historical records. Hiroaki Isobe. Graduate School of Integrated Advanced Studies . in Human Survivability, Kyoto University. Aknowledgements. Hugh Hudson. SSL, UC Berkeley and U. Of Glasgow. . 1. The Sun and its corona/wind. Solar . flares and . CMEs. Extreme events: new facts. “. Nanoflares. ”. The Sun itself. 2. It is not obvious from this sketch, but the very thin . Viacheslav Sadykov. , Alexander Kosovichev, Gelu Nita. (Department of Physics, NJIT). Rishabh Gupta, Vincent Oria. (Department of Computer Sciences, NJIT). Alexander Frolov . (High-school student). Introduction. on Solar-Type Stars: The Curious . Case of EK . Draconis. Tom . Ayres (. CASA. ) . SDO photosphere . to corona. . Time-resolved . HST. /COS G160M. . TS*12. . Oct . ‘15. BACKGROUND. 2010. . HST/. in this class.. You will be compensated $$$ for your note-taking.. To . apply to be a note-taker please visit. http://sds.umbc.edu/becoming-a-note-taker/. Composition and Structure of the Atmosphere. CSP Industry Panel. Stage Gate Process. Solar Dynamics LLC. 2. 4 Work Categories in Each Stage. Market/customer assessment. Research, development, demonstration . activities ($$$). Competitive technology/detailed . HMI Observations of Solar Flares in Solar Cycle . 24. . Todd Hoeksema, Monica . Bobra. , . Sebastien. . Couvidat. , . and . Xudong. Sun. . Stanford University. SHARP Parameter Table. HMI Data Series: hmi.sharp_720s. lognormal instead of power law?. Solar-Terrestrial Centre of Excellence. Cis . Verbeeck. , Emil . Kraaikamp. , Lena . Podladchikova. Royal Observatory of Belgium. SDO Workshop, Ghent, Belgium. , October 29, . M. . Prijatelj. Carnegie Mellon University. Advisors: B. Chen, P. . Jibben. (SAO). Overview. Motivations. Standard Flare Model. Flux rope eruption. Magnetic reconnection. Flare emissions. Type III Radio Bursts.