P
Peter R. Young
Researcher at Goddard Space Flight Center
Publications - 180
Citations - 12349
Peter R. Young is an academic researcher from Goddard Space Flight Center. The author has contributed to research in topics: Emission spectrum & Spectral line. The author has an hindex of 55, co-authored 180 publications receiving 11246 citations. Previous affiliations of Peter R. Young include Advanced Micro Devices & George Mason University.
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The EUV Imaging Spectrometer for Hinode
J. L. Culhane,Louise K. Harra,A. M. James,K. Al-Janabi,L. Bradley,Rifat A Chaudry,Kerrin Rees,J. Tandy,P. D. Thomas,M. C. R. Whillock,Berend Winter,George A. Doschek,Clarence M. Korendyke,Charles M. Brown,S. H. Myers,J. T. Mariska,John F. Seely,J. Lang,B. J. Kent,B. M. Shaughnessy,Peter R. Young,G. M. Simnett,C. M. Castelli,S. Mahmoud,H. Mapson-Menard,Brian J. Probyn,Roger J. Thomas,Joseph M. Davila,Kenneth P. Dere,David L. Windt,John Shea,R. Hagood,Robert W. Moye,Hirohisa Hara,Takashi Watanabe,K. Matsuzaki,Takeo Kosugi,Viggo Hansteen,Ø. Wikstol +38 more
TL;DR: The EUV Imaging Spectrometer (EIS) as mentioned in this paper is a two-element, normal incidence design with a backside-illuminated, thinned CCD, which has a significantly greater effective area than previous orbiting EUV spectrographs with typical active region 2 -5 s exposure times in the brightest lines.
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Chianti—an atomic database for emission lines. xiii. soft x-ray improvements and other changes
TL;DR: The CHIANTI spectral code as mentioned in this paper consists of two parts: an atomic database and a suite of computer programs in Python and IDL, together, they allow the calculation of the optically thin spectrum of astrophysical objects and provide spectroscopic plasma diagnostics for the analysis of the astrophysical spectra.
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CHIANTI - an atomic database for emission lines. IX. Ionization rates, recombination rates, ionization equilibria for the elements hydrogen through zinc and updated atomic data
TL;DR: The CHIANTI database as mentioned in this paper provides a set of atomic data for the interpretation of astrophysical spectra emitted by collisionally dominated, high temperature, optically thin sources.
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CHIANTI-An Atomic Database for Emission Lines. VII. New Data for X-Rays and Other Improvements
TL;DR: The CHIANTI atomic database as mentioned in this paper contains atomic energy levels, wavelengths, radiative transition probabilities, and collisional excitation data for a large number of ions of astrophysical interest.
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CHIANTI – An atomic database for emission lines. Version 8
TL;DR: This version of the CHIANTI database includes a large amount of new data and ions, which represent a significant improvement in the soft X-ray, EUV and UV spectral regions, which several space missions currently cover.