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The Reuven Ramaty High Energy Solar Spec
. Ed(S): Lin, Robert P.; Dennis, Brian R.; Benz, Arnold O.
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Description for The Reuven Ramaty High Energy Solar Spec
Paperback. Editor(s): Lin, Robert P.; Dennis, Brian R.; Benz, Arnold O. Num Pages: 456 pages, biography. BIC Classification: PG; PHVB. Category: (P) Professional & Vocational. Dimension: 235 x 155 x 23. Weight in Grams: 712.
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
Paperback
Publication date
2010
Publisher
Springer Netherlands
Number of pages
456
Condition
New
Number of Pages
456
Place of Publication
Dordrecht, Netherlands
ISBN
9789048162123
SKU
V9789048162123
Shipping Time
Usually ships in 15 to 20 working days
Ref
99-15
Reviews for The Reuven Ramaty High Energy Solar Spec
"...important and useful to the study of solar flares and related phenomena." (Space Flight, 45 (2003)