Swedish Institute of Space Physics Uppsala. Lecture ... F = q (E v x B) m g. For charged particles, gravity can usually be neglected (calculate yourself! ...
High-energy Emission from Pulsar Magnetospheres. Kouichi HIROTANI. TIARA, Taiwan. Osaka ... For example, the Crab pulsar shows very soft g-ray spectrum. ...
Earth, Mercury, and the gas-giant planets all have magnetospheres ... Table of the planet's mean temperatures and their respective predictions. Planet. Albedo ...
Magnetically-Dominated Accretion Flows Around Black Holes (MDAFs) ... But MDAFs can be 10 times larger than magnetospheres discussed generally heretofore ...
Determine the response of terrestrial and planetary magnetospheres and ... 4) South Africa: 1 site location. Contact will be made with staff at Hermanus Observatory. ...
Anomalous resistivity and the non-linear evolution of the ion-acoustic instability Panagiota Petkaki British Antarctic Survey, Cambridge Magnetic Reconnection Theory
Niels Bohr CompSchool Compact Objects Neutron Star Observables, Masses, Radii and Magnetic Fields Feryal Ozel University of Arizona Lecture 1: Surfaces of Neutron Stars
Magnetars: SGRs and AXPs Magnetars in the Galaxy ~7 SGRs, ~12 AXPs, plus candidates, plus radio pulsars with high magnetic fields (about them see arXiv: 1010.4592)
Title: Neutron star masses: dwarfs, giants and neighbors Author: PKSternberg Last modified by: sternberg pk Created Date: 11/26/2005 8:18:07 AM Document presentation ...
Title: PowerPoint Presentation Author: Sumanas Last modified by: Varada vaidya Created Date: 12/24/2002 1:08:46 AM Document presentation format: On-screen Show
Magnetars: SGRs and AXPs Magnetars in the Galaxy ~11 SGRs, ~12 AXPs, plus candidates, plus radio pulsars with high magnetic fields (about them see arXiv: 1010.4592)
Plasma = and charged particles (ions, electrons) and neutral particles ... Encloses the magnetosphere 'shielding' it from the SW. Geocentric distance ~10 RE. ...
... the Moon Europa also causes a neutral gas torus to form. ... At IO, this speed is much faster than the orbital speed of IO and the plasma torus passes by IO...
When Cassini reached Saturn it found ion cyclotron waves essentially every where ... The wave forms of ICWs at Saturn are similar to ICWs in the Earth's ...
Title: Slide 1 Author: Simon Brown Last modified by: sz Document presentation format: On-screen Show (4:3) Other titles: Arial Times New Roman Wingdings Comic Sans MS ...
At Jupiter, most of the aurora is driven by internal ... Michel Blanc, Philippe Louarn (CESR, Toulouse, F) Andrew Coates, Geraint H. Jones (UCL-MSSL, UK) ...
Space Science MO&DA Programs - June 2000 - Page 1. SS ... Space Science MO&DA Programs - June 2000 - Page 3. SS. POLAR's new 'weather map aurora' display ...
Albedo/reflectivity of the surface. Absorption (0) or reflection (1) Greenhouse gases ... Albedo of surface features. Parable of the Daiseyworld (cont) ...
The Bimodal Solar Wind-Magnetosphere-Ionosphere System George Siscoe Center for Space Physics Boston University Vasyliunas Dichotomization Momentum transfer via ...
Why is the best month to see Jupiter different from one year to the next? ... the chemical composition of Jupiter's atmosphere imply about the planet's origin? ...
X ray bright points. Solar active regions. G,K & M dwarfs. T Tauri stars. Convective. envelope ... CR: Cosmic ray. PI: Pickup ions. SW: Solar wind. TS: ...
High: LHW, E//, Centrifugal Acceleration, ES Shocks, Holzer ... Centrifugal Acceleration. Destiny of polar wind outflows. Gradual energy increase in polar cap ...
Titan's exosphere interaction with Saturn's ... of shocked solar wind with exosphere ... solar wind magnetosphere - exosphere - surface interactions ...
F2B: Quantify Particle Acceleration for Key Regions of Exploration ... Dipper mission, Earth analog to dynamics and variability of the lower thermosphere ...
... the second largest planet in the Solar ... own thing taking 550 days to orbit the planet. ... a magnetic field that shields the planet, its rings, and moons ...
However, at Uranus it is tipped 60o to the axis of rotation AND it is displaced ... However, Pluto and Neptune obit this Sun in a resonance configuration which ...
Known radio pulsars appear to emit short pulses of radio radiation with pulse ... ( From the Handbook of Pulsar Astronomy, by Lorimer and Kramer) 46. Pulsar population ...
describe general physical properties of ... describe the effect of tides on the Earth-Moon system. ... An album by Pink Floyd is titled 'Dark Side of the Moon. ...
There is plenty of evidence for the presence of particle acceleration in compact objects: ... In the vicinity of a compact object, the strong gravitational ...
Title: Star formation - the accretion (luminosity) problem Author: Lee Hartmann Last modified by: Lee Hartmann Created Date: 6/6/1999 2:12:30 PM Document presentation ...
A. Balogh (ICL, London) ... Precursor part Composition Composition Feature-8: magnetospheric condition Feature-9 : ground conj. Indications from data ...
Earth s Atmosphere with focus on the upper atmosphere above 100km (Thermosphere and Ionosphere) Gang Lu High Latitude Observatory National Center for ...
Mona Kessel, NASA HQ Contributions by Jacob Bortnik, Seth Claudepierre, Nicola Fox, Shri Kanekal, Kris Kersten, Craig Kletzing, Lou Lanzerotti, Tony Lui, Barry Mauk ...
The Earth s Magnetosphere & Solar Wind Tim Froehlig & Bevan Gerber ... also varies SoHO Solar and Heliospheric Observatory Joint ESA/NASA project Launched Dec ...
Solar Wind-Magnetosphere Interactions via Low Energy Neutral Atom Imaging T E Moore[1], M R Collier[1], M-C Fok[1], S A Fuselier[2], D. G. Simpson[1], G. R. Wilson[3 ...
Solar Wind-Magnetosphere Interaction for Northward Interplanetary Magnetic Field Paul Song Center for Atmospheric Research University of Massachusetts Lowell