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» » UV and X-Ray Spectroscopy of Laboratory and Astrophysical Plasmas
UV and X-Ray Spectroscopy of Laboratory and Astrophysical Plasmas e-book

Author:

Eric H. Silver,Steven M. Kahn

Language:

English

Category:

Math

Subcategory:

Astronomy & Space Science

ePub size:

1944 kb

Other formats:

azw rtf mbr txt

Rating:

4.7

Publisher:

Cambridge University Press; First Edition edition (July 30, 1993)

Pages:

628

ISBN:

052143470X

UV and X-Ray Spectroscopy of Laboratory and Astrophysical Plasmas e-book

by Eric H. Silver,Steven M. Kahn


Eric H. Silver, Steven M. Kahn. UV and X-ray spectroscopy of astrophysical and laboratory plasmas draws interest from many disciplines. Contributions from international specialists are collected together in this book from a timely recent conference.

Eric H. In astrophysics, the Hubble Space Telescope, Astro 1 and ROSAT observatories are now providing UV and X-ray spectra and images of cosmic sources in unprecedented detail, while the Yohkoh mission recently collected superb data on the solar corona

Eric H. In astrophysics, the Hubble Space Telescope, Astro 1 and ROSAT observatories are now providing UV and X-ray spectra and images of cosmic sources in unprecedented detail, while the Yohkoh mission recently collected superb data on the solar corona

UV and X-ray spectroscopy of astrophysical and laboratory plasmas draws interest from many disciplines. Contributions from international specialists are collected together in this book from a timely recent conference

UV and X-ray spectroscopy of astrophysical and laboratory plasmas draws interest from many disciplines. In astrophysics, the Hubble Space Telescope, Astro 1 and ROSAT observatories are now providing UV and X-ray spectra and images of cosmic sources in unprecede UV and X-ray spectroscopy of astrophysical and laboratory plasmas draws interest from many disciplines.

The second objective is to establish our microcalorimeter as an essential x-ray diagnostic for laboratory astrophysics studies. We propose to develop a dedicated microcalorimeter spectrometer for the EBIT (electron beam ion trap)

The second objective is to establish our microcalorimeter as an essential x-ray diagnostic for laboratory astrophysics studies. We propose to develop a dedicated microcalorimeter spectrometer for the EBIT (electron beam ion trap). The third objective is to investigate innovative ideas related to possible flight opportunities.

oceedings{Silver1993UVAX, title {UV and x-ray spectroscopy of astrophysical and laboratory . colloquium held at Berkeley, California, 3-5 February 1992}, author {Eric H. Silver and Steven M. Kahn}, year {1993} }.

oceedings{Silver1993UVAX, title {UV and x-ray spectroscopy of astrophysical and laboratory plasmas : proceedings from the tenth international colloquium held at Berkeley, California, 3-5 February 1992}, author {Eric H. Eric H. Contents Scientific organizing committee List of participants Preface Part I. Atomic Processes and Overview Part II. UV Spectroscopy Part III. X-Ray Spectroscopy.

Cambridge University Press. Assembled Product Dimensions (L x W x H). 8 x . 4 x . 8 Inches.

Journal de physique - t. 49. - - Colloque C1, supplement au no. 3 (mars 1988), Journal de physique - t. 49, Journal de physique - 1988, C1. ID Numbers.

Cite this chapter as: Kahn S. (2005) Soft X-Ray Spectroscopy of Astrophysical Plasmas. In: High-Energy Spectroscopic Astrophysics.

Local Thermodynamic Equilibrium Slater Determinant Astrophysical Plasma Dielectronic Recombination Collisional Excitation. These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves. Cite this chapter as: Kahn S. Saas-Fee Advanced Course, vol 30.

X-ray spectroscopy of astrophysical plasmas. Authors: Steven M Kahn Ehud Behar Ali Kinkhabwala Daniel W Savin. Philos Trans A Math Phys Eng Sci 2002 Sep;360(1798):1923-33.

UV and X-ray spectroscopy of astrophysical and laboratory plasmas draws interest from many disciplines. Contributions from international specialists are collected together in this book from a timely recent conference. In astrophysics, the Hubble Space Telescope, Astro 1 and ROSAT observatories are now providing UV and X-ray spectra and images of cosmic sources in unprecedented detail, while the Yohkoh mission recently collected superb data on the solar corona. In the laboratory, the development of ion-trap facilities and novel laser experiments are providing vital new data on high temperature plasmas. Recent innovations in the technology of spectroscopic instrumentation are discussed. These papers constitute an excellent up-to-date review of developments in short-wave length spectroscopy and offer a solid introduction to its theoretical and experimental foundations.

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