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The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI). Mission Description and Early Results.
. Ed(S): Lin, Robert P.; Dennis, Brian R.; Benz, Arnold O.
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Description for The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI). Mission Description and Early Results.
Hardback. Explains the functioning of Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI). This book introduces data analysis techniques including spectroscopy and image reconstruction. It is suitable for scientists and students. Editor(s): Lin, Robert P.; Dennis, Brian R.; Benz, Arnold O. Num Pages: 456 pages, biography. BIC Classification: PGS; PHVB. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 235 x 155 x 25. Weight in Grams: 835.
The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) satellite was launched on 5 February 2002. Its objective is to study the energy release and particle acceleration in solar flares through observations of X-rays and gamma rays. Two novel technologies are combined to obtain both spectra and images over a broad energy range. For the spectroscopy, cooled hyperpure germanium detectors are used to cover the energy range from 3 keV to 17 MeV with unprecedented keV-class resolution. Since focusing optics are not possible for making images with such high energy photons, tungsten and molybdenum absorbing grids are used to modulate ... Read more
The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) satellite was launched on 5 February 2002. Its objective is to study the energy release and particle acceleration in solar flares through observations of X-rays and gamma rays. Two novel technologies are combined to obtain both spectra and images over a broad energy range. For the spectroscopy, cooled hyperpure germanium detectors are used to cover the energy range from 3 keV to 17 MeV with unprecedented keV-class resolution. Since focusing optics are not possible for making images with such high energy photons, tungsten and molybdenum absorbing grids are used to modulate ... Read more
Product Details
Format
Hardback
Publication date
2003
Publisher
Kluwer Academic Publishers United States
Number of pages
456
Condition
New
Number of Pages
456
Place of Publication
New York, NY, United States
ISBN
9781402011078
SKU
V9781402011078
Shipping Time
Usually ships in 15 to 20 working days
Ref
99-15
Reviews for The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI). Mission Description and Early Results.
"...important and useful to the study of solar flares and related phenomena." (Space Flight, 45 (2003)