PPT-Radiative processes during GRB prompt emission

Based on works by Asaf Peer ITC Harvard University in collaboration with Peter Meszaros PSU Martin Rees IoA Christoffer Lundman Felix Ryde Stockholm. . . . . . Maria . Giovanna Dainotti. Stanford . University, USA, Fulbright Scholar, . now . JSPS Fellow . at . Riken, Tokyo, . Bethany Elisa Cobb. The George Washington University. IAU. Symposium 279. March 13, 2012. (. Fynbo. et al. 2000). GRB-SNe Connection. Energy considerations. Long-duration GRBs associated with star-forming host galaxies . tropical cyclones. Robert Fovell and . Yizhe. Peggy Bu. University of California, Los Angeles. rfovell@ucla.edu. 1. Thanks to. : . Greg . Thompson, NCAR/. DTC; Ligia . Bernardet. and Mrinal . Biswas. Corrections. Peter Schnatz. Stony Brook University. Radiative. Events. In scattering experiments, a photon may be emitted by a charged particle due to . Bremsstrahlung. radiation.. This type of radiation is due to the deceleration of a charged particle as it approaches the . Useful reviews:. Waxman astro-ph/0103186. Ghisellini astro-ph/0111584. Piran astro-ph/0405503. Meszaros astro-ph/0605208. Useful links. http://www-astro.physics.ox.ac.uk/~garret/teaching/. http://www.cv.nrao.edu/course/astr534/. . Sanshiro. Shibata (Konan Univ.). Collaborator: . Nozomu. . Tominaga. (Konan Univ., IPMU). Introduction. Models for the prompt emission. Internal shock model. A standard scenario for a long time.. In astronomy, the main source of information about celestial bodies and other objects is the visible light or more generally electromagnetic radiation.. From Wikipedia.. It also is important for the atmosphere of Earth, so you’ll meet it if you are going into Earth atmosphere science…. imbalance . 1985-2012. Richard P. Allan. , . Chunlei. . Liu (University of Reading/NCAS Climate); Norman Loeb (NASA Langley); Matt Palmer (Met Office). r.p.allan@reading.ac.uk. @. rpallanuk. GEWEX 7. DYNAMO/CINDY. 2011. C.-H. . Sui, . Yi-An Chen, . Shu-Yu . Hou. National Taiwan University. NSA. SSA. (73.1E,0.7S). (. 72E,-7.3N. ). (73.5E,4.2N). (. 79E,6.9N. ). (. 80.5E,0.07N. ). (. 80.5E,-8N. ). Male. Judy Racusin. Penn State University. 2008 Nanjing GRB Workshop, Nanjing, China, June 23-27. Broadband Observations of the Extraordinary . Naked-Eye GRB 080319B. . J. L. . Racusin. , S.V. . Karpov. , M. . General information and WP.29 highlights. Participants/Address list. A provisional address list has been prepared: please check your . contact data (especially . the email-address) and correct them, if . National Centre for Radio Astrophysics. Tata Institute of Fundamental Research. Poonam Chandra. What are Gamma Ray bursts (GRBs)?. Most energetic events in the universe. Long duration GRBs (t>2s) . Xiaoming Hu. 1. , Sergio A. Sejas. 2. , Ming Cai. 3. , . Zhenning. Li. 4. and Song Yang. 1. 1. School of Atmospheric Sciences, Sun . Yat-sen. University, Guangzhou, China. 2. NASA Langley Research Center, Climate Science Branch, Hampton, Virginia, USA. Kerry Emanuel. Massachusetts Institute of Technology. Several Possibly Inter-related Enigmas of the Tropical Atmosphere. Why does moist convection often cluster?. What determines the number of tropical cyclones on the planet?.