Magnetic sail braking vs two-stage fusion rockets
F.Longo SNR 1 GLAST LAT GLAST Italian SW meeting 11 march 2004 SNR Francesco Longo University and INFN, Trieste, Italy [email protected] Slides.
Generation of Magnetic Fields in Gravitationally Forming Structures in the Early Universe Russell M. Kulsrud Princeton Plasma Physics Laboratory.
Magnetic Fields in the Milky Way_netherlands_2014
Cosmic Microwave Background, Foregrounds and Component Separation What are foregrounds and how to deal with them in CMB data analysis Carlo Baccigalupi,
High energy emission from supernova remnants and regions of star formation Diego F. Torres [email protected] Lawrence Livermore Lab. California,
Post MSc lectures, SINP, December 2012 Pratik Majumdar SINP, Kolkata Outline: Shock Acceleration Fermi’s theory of 2 nd and 1 st order acceleration.
An attempt to detect Cosmic Rays coming into our atmosphere with the help of some statistics By Rodney Howe, MS. GIS/Remote Sensing 07.02.2002.
Jo-Anne Brown Observations of the Galactic Magnetic Field from the International Galactic Plane Survey.
Contamination of the CMB Planck data by galactic polarized emissions L. Fauvet, J.F. Macίas-Pérez.
Galactic Diffuse Gamma-ray Emission, the EGRET Model, and GLAST Science Stanley D. Hunter NASA/GSFC Code 661 [email protected].
Electromagnetic Waves Physics 202 Professor Lee Carkner Lecture 21.
