'Radiation belt' diaporamas de présentation

1.5k views • 131 slides

Observation of radiation belt losses into the ionosphere

Observation of radiation belt losses into the ionosphere. Craig J. Rodger Department of Physics University of Otago Dunedin NEW ZEALAND. REPW 2007 2:45pm Wednesday, 8 August 2007. Energetic electrons, the Radiation Belts, and Geomagnetic Storms.

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Space Environment

Space Environment. Please type in your questions and raise your hand so we can answer it during class. SSE-120. Space Environment. Space Environmental Effects. 2. SSE-120. Space Environment. Consider some things in the environment. 3. SSE-120. Space Environment.

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Radiation Belt Precipitation due to Manmade VLF Transmissions: Satellite Observations

Radiation Belt Precipitation due to Manmade VLF Transmissions: Satellite Observations. Rory J Gamble 1 , Craig J Rodger 1 , Mark A Clilverd 2 , Neil R Thomson 1 , Simon L Stewart 1 , Robert J McCormick 1 , Michel Parrot 3 , Jean-André Sauvaud 4 , Jean-Jacques Berthelier 5.

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Ground-based transmitter signals observed from space: ducted or nonducted?

Ground-based transmitter signals observed from space: ducted or nonducted?. Mark A. Clilverd 1 , Craig J. Rodger 2 , Rory J. Gamble 2 , Nigel P. Meredith 1 , Michel Parrot 3 , Jean-Jacques Berthelier 4 , and Neil R. Thomson 2.

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429 views • 31 slides

Current challenges and opportunities in radiation belt and wave research

Current challenges and opportunities in radiation belt and wave research. Jacob Bortnik, UCLA. Contents. New GEM FG: Radiation Belt and Waves Modeling (RBWM) Radiation Belt Storm Probes (RBSP) mission Challenges & opportunities. We shall not cease from exploration

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Radiation Belt Storm Probe Electric Field and Waves Instrument (EFW) PI: Prof. John Wygant, UMN

Radiation Belt Storm Probe Electric Field and Waves Instrument (EFW) PI: Prof. John Wygant, UMN jwygant@comcast.net , (612) 626-8921 PM: Dave Curtis, UCB dwc@ssl.berkeley.edu , 510-642-5998. Org Chart. Major Subcontracts. UMN will subcontract to UCB and LASP to develop the EFW instrument

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Galactic Cosmic Rays

The Radiation Belts and Killer Electrons. Terry Onsager, NOAA Space Environment Center. Solar Energetic Particles. Trapped Electrons and Protons. Galactic Cosmic Rays. AF-Geospace, Courtesy of Greg Ginet, AFRL. Magnetospheric Specification Model, Rice University.

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Time Domain Astronomy

Time Domain Astronomy. ATUC Science Day Sydney, 24 Oct 2011 Ron Ekers CSIRO, Australia. Why me?. No erudite overview of the field I have observed all the classes of variables listed And a few more I will make various personal observations and anecdotes based on my experience.

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Once Upon a Time in the Electron Radiation Belts

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LT RBR :

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Space Radiation Climatology: A New Paradigm for Inner Magnetosphere Simulation and Data Analysis

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Energetic Electron Bursts in the Magnetotail

Energetic Electron Bursts in the Magnetotail. J. B. Blake Space Sciences Department The Aerospace Corporation. Electron Bursts - Cluster/RAPID. Electron bursts routinely seen in magnetotail Global size cannot be determined by Cluster constellation

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Waves and Particles in the Radiation Belt

Waves and Particles in the Radiation Belt. Kaiti Wang PSSC/NCKU March 17, 2009. Opportunity for Collaboration on ERG and SCOPE Missions & Community Input. An Important Question to Answer. Can chorus be a source for plasmaspheric hiss ?.

241 views • 13 slides

Galilean Moons

Galilean Moons. By Matt Francis. Facts. The Galilean Moons are 4 moons that orbit Jupiter and can be seen by any telescope. They are called Europa, Io, Callisto, and Ganymede. All the moons keep one face towards Jupiter in a phase called tidal locking. Europa.

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Van Allen Probes Extended Mission Science Themes (1 of 3)

Van Allen Probes Extended Mission Science Themes (1 of 3). S patial and temporal structures of injections and other transient phenomena and their effects on the radiation belts and ring current New Opportunities : Modified orbit configurations

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Nonlinear electric field structures in the inner magnetosphere

Nonlinear electric field structures in the inner magnetosphere D. M. Malaspina 1 , L. Andersson 1 , R. E. Ergun 1 , J. R. Wygant 2 , J. W. Bonnell 3 , C. Kletzing 4 , G. D. Reeves 5 , R. M. Skoug 5 , and B. A. Larsen 5 [1] U. Colorado / LASP [2] U. Minnesota [3] U.C. Berkeley

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Sputnik

Sputnik.

189 views • 2 slides