Ronald C. Kirkpatrick and Irvin R. Lindemuth- Magnetic Compression/Magnetized Target Fusion (MAGO/MTF), An Update
Nova engine powerpoint
The Solar Corona B. C. Low High Altitude Observatory National Center for Atmospheric Research The National Center for Atmospheric Research is operated.
Software Sustainability Institute SSI in one slide.
The Radio Jets of AGN Denise Gabuzda University College Cork Recent results considered in framework of the hypothesis that (many or even all) jets have.
Physics of Dust Pickup in the Solar Wind: Contributions by STEREO C.T. Russell, L.K. Jian, J.G. Luhmann, D.R. Weimer STEREO Science Team Meeting February.
Which describes a variation of wave frequency ω(t) in a geometric-optic approximation [4]. Here n(ω) is the refractive index of the medium, is the vector.
Science with SKA:. The SKA will provide continuous frequency coverage from 50 MHz to 14 GHz in the first two phases of its construction. A third phase.
Plasma Unbound: New Insights into Heating the Solar Atmosphere and Accelerating the Solar Wind Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics.
Strong nonresonant amplification of magnetic fields in particle accelerating shocks A. E. Vladimirov, D. C. Ellison, A. M. Bykov Submitted to ApJL.
Exploring the Solar Wind with Ultraviolet Light Steven R. Cranmer and the UVCS/SOHO Team Harvard-Smithsonian Center for Astrophysics.
Leaky Stars: Steven R. Cranmer & many others Harvard-Smithsonian Center for Astrophysics Pulsations, Waves, and Turbulence in Stellar Winds across the.