PPT-Solar flare distributions:

lognormal instead of power law SolarTerrestrial Centre of Excellence Cis Verbeeck Emil Kraaikamp Lena Podladchikova Royal Observatory of Belgium SDO Workshop Ghent Belgium October 29 . Magdalena Gryciuk. Astronomical Institute, University of . Wroclaw. Space . Research . Centre, Polish . Academy of Sciences. I SOLARNET SPRING SCHOOL, WROCŁAW, 28.03.2014 . SPHINX INSTRUMENT. SPHINX . RHESSI: a . statistical study. Jianxia. Cheng. . Jiong. . Qiu. , . Mingde. Ding, and . Haimin. Wang. outline. Introduction. Observations and data analysis. Properties of HXR spikes. summary. 1.Introduction. . 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. Ryan Payne. Advisor:. Dana . Longcope. Solar Flares. General. Solar flares are violent releases of matter and energy within active regions on the Sun.. Flares are identified by a sudden brightening in chromospheric and coronal emissions.. 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 . ?. 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. . Observed, estimated, and predicted daily geomagnetic . AFr. -indices (A-indices from Fredericksburg, VA), and daily AP-indices (planetary A-indices). . Ap. indices are estimated in near-real time using a network of up to 12 North American stations. . 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. Joel Allred (NASA GSFC) --Team 1. Phil Judge (HAO) & Lucia . Kleint. . (Original PI)-- Team 2 . Alexander . Kosovichev. (NJIT/Stanford) –Team 3. Chang Liu (NJIT)--Team 4. 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. Hugh S. Hudson (UC Berkeley and U of Glasgow). Bibliography. Bornmann. , P. L., “Limits to derived flare properties…”, . ApJ. 356, 733,. 1990.. Hudson, H.S., . Simoes. , J.A., Fletcher, L., Hayes, L. A., and Hannah, I.G.. Exoplanets. Kazunari. Shibata. . Kwasan. and . Hida. observatories, . Kyoto University. Hiroaki Isobe. Unit of Synergetic Studies for Space, Kyoto University. isobe@kwasan.kyoto. -. u.ac.jp. COSPAR2014, .