PPT-Correlating Type II and III Radio Bursts with

Solar Energetic Particle Events L Winter S Huston K Ledbetter R Quinn AER Analysis of the WindWAVES radio burst and the GOES proton properties led to finding that radio properties eg type II and type III peak flux can be used to predict the peak proton flux level. 01 Date 20140221 Maintainer Jeff Binder Description An implementation of Jon Kleinbergs burst detection algorithm Uses an in64257 nite Markov model to detect periods of increased activity in a series of dis crete events with known times and provides Alexander . Kotov. , . ChengXiang. . Zhai. , Richard . Sproat. University of Illinois at Urbana-Champaign. Roadmap. Problem definition. Previous work. Approach. Experiments. Summary. Motivation. Web data is generated by a large number of textual streams (news, blogs, tweets, etc. fast radio bursts . Vikram. Ravi. University of Melbourne and CASS. With Ryan Shannon and Paul . Lasky. And . with particular . thanks to the Swinburne CAS staff and students. 1. Fast radio bursts (. HSTs continuing contribution to gamma-ray bursts. Andrew Levan. University of Warwick. Javier . Gorosabel. . Urkia. . 27 Oct 1969- 21 Apr 2015. A major contributor to the field of gamma-ray bursts from the first afterglows to today. Poonam Chandra. National Centre for Radio Astrophysics - Tata Institute of Fundamental Research. Collaborator: Dale Frail and many others. Radio Afterglows. . Late time follow up.. . Accurate energetics instead of “isotropic equivalent” energy .. Laura Chomiuk. Jansky. Fellow, Michigan State University. Supernova Types: I vs. II. Type I:. No Hydrogen. Thermonuclear WD explosions (. Ia. ) . and. . Core collapse of massive stars stripped of H envelopes (. © All rights reserved. Ji . Long (. 紀龍. ). in collaboration with . Zhang . Shu. , . Chen . YuPeng. , . Zhang . Shuang. -Nan, Diego . F. . Torres, . Peter Kretschmar, Masha . Chernyakova. , Li Jian, . w. eb . Ryan Shannon, . ICRAR-Curtin/. ATNF (. Vikram. Ravi, Swinburne . Pulsar . Group). Outline. Fast radio bursts (. FRBs) . Exciting times!. FRB 131104 . The . (improbable/real-time) . discovery of an FRB to the Carina dwarf spheroidal. Aim: How do we correlate rocks? . Geologists try to match similar rock strata in different locations to see if they formed at the same time. This process is called. Correlation. Lets learn about correlation. Edwin Kite (U. Chicago), John Armstrong (Weber State), . Robin Wordsworth (Harvard), Francois Forget (LMD) . c. an climate . models. h. elp distinguish. these scenarios?. h. abitable surface. s. terile surface. catch a burst and notify other observatoriesboth in space and on the ground of its approx-imate locationWithin minutes HETE-2 mayobtain a precise locationCurrent telescopestake much longer to notify o 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) . IIn. supernovae. Poonam Chandra. National Centre for Radio Astrophysics. Tata Institute of Fundamental Research. Collaborators: Roger Chevalier, Nikolai Chugai, . Claes. . Fransson. , A. . Soderberg. Sheared magnetic structures, inferred from photospheric magnetograms, have been thought to be indicative of imminent eruption (Ambastha et al., 1993). Combining vector magnetograms with the Yohkoh sof