PPT-Building a comet

Whats a Comet Made of dirty snowball model Composed of Ices water CO 2 and others Gases water CO 2 CO O 2 and some simple organics Tiny dust particles organic and inorganic. ISON . OBSERVING . CAMPAIGN . (=CIOC) SBAG Update Jan – Jul 2013 . CIOC . Team. established Jan 2013 at SBAG-8. . Team has a mix of experiences, skillsets, and research specialties. . Abundant contributions from early- and mid. European Space Agency (ESA). Launched 10 years ago, 5 Earth flybys to save fuel and weight. Rosetta Explores a Comet. Comet 67P or . Churyumov-Gerasimenko. (after who found it). 4x4.5 km – here with Los Angeles for scale. 67P/. Churyumov-Gerasimenko. : . Needs for SWMF Modeling. K.C. Hansen. Zhenguang. Huang. University of Michigan. SWMF User Meeting, October 13-14, 2014. Comet Modeling at UM. ICES Tools. Andre . Bieler. Andrew Cheng . (JHU/APL; andrew.cheng@jhuapl.edu). Steve Arnold . (. JHU/APL). Pietro. . Bernasconi. . (JHU/APL). Karl . Hibbitts. . (JHU/APL). Eliot . Young. . (. SwRI. ). Tibor. . Kremic. . (GRC). COMET. μ-e conversion search from . muonic. . aluminium. J-PARC pulsed proton beam to produce pulsed . muon. beam. Forbidden in the Standard Model .  clue to the new physics beyond the Standard Model. . Shahzeb Siddiqui - sms5713@psu.edu. Software Systems Engineer. Office: 222A Computer Building. Institute of . CyberScience. . May . x. th. . 2015 . System Overview. Comet is one of the XSEDE cluster designed by Dell and SDSC that delivers 2.0 PFLOPS of performance. . muon. particle physics . programmes. at J-PARC. Mu_01. Satoshi MIHARA. IPNS, KEK. FKPPL-FJPPL workshop, . Yonesei. Univ.. Outline. Introduction. Physics motivation. J-PARC facility. France-Japan collaboration in the COMET experiment at J-PARC. Could . Comets have Delivered the Ingredients for Life? . Dr. Erika . Gibb. Dept. of Physics & Astronomy. April 9, 2016. A. B. C. D. 50,000 AU. 500 AU. Test the possibility for exogenous delivery to early Earth –>. Beam line. Experiment area. SC magnet. Pion production target. Construction of. high-p/COMET beam lines. Steel-septum (. Lambertson. ) magnet,. Current-septum magnets x2. Beamline. magnets. Dx7, Qx8. dust tail. - A long, wide tail buffeted by photons emitted from the Sun, but it curves slightly due to the comet's motion.. hydrogen envelope. - Hydrogen gas that surrounds the coma of the comet and trails along for millions of miles (it is usually between the ion tail and the dust tail). The hydrogen envelope is about 10 million km across at the nucleus of the comet and about 100 million km long.. Migrating Execution Transparently. OSDI'12. Mark Gordon, Anoushe Jamshidi,. Scott Mahlke, Z. Morley Mao, and Xu Chen. University of Michigan, AT&T Labs - Research. Mark Gordon. 2. Overview. Introduction. . Shahzeb Siddiqui - sms5713@psu.edu. Software Systems Engineer. Office: 222A Computer Building. Institute of . CyberScience. . May . x. th. . 2015 . System Overview. Comet is one of the XSEDE cluster designed by Dell and SDSC that delivers 2.0 PFLOPS of performance. . Akiva Bar-Nun and Diana Laufer . Dept. of Geosciences, Tel Aviv University. Thanks to the OSIRIS team. 1. The comet is chaotic since it was formed by agglomeration of fluffy ice balls at low speeds, followed by violent gas release events on the comet.. November 12, 2014:. First-Ever Soft Landing on a Comet. (Comet 67P/. Churyumov-Gerasimenko. ). The Rosetta Mission. Launched in 2004: 10 Years in the Making. Graphic: . Time. Magazine, Nov. 17, 2014.