Overview Review of the Goddard method Update on instrument/detector evolution (a purely phenomenological approach) Characterization of the soft proton.
UK Spectrum Policy Forum - Rachel Clark, Ofcom - Spectrum Sharing
Seewave Analysis
X-ray Emission from Massive Stars: Using Emission Line Profiles to Constrain Wind Kinematics, Geometry, and Opacity David Cohen Dept. of Physics and Astronomy.
David Cohen Dept. of Physics and Astronomy Swarthmore College
Large Two-way Arrays
1. INTRODUCTION As the brightest dwarf nova and one of the brightest cataclysmic variables of any kind, SS Cygni has been extensively observed. Its outbursts,
1. INTRODUCTION
Spectra of Gravity Wave Turbulence in a Laboratory Flume S Lukaschuk 1, P Denissenko 1, S Nazarenko 2 1 Fluid Dynamics Laboratory, University of Hull 2.
WAVELET TRANSFORM
