The Spectroscopy of Plasma Evolution from Astrophysical Radiation Mission
The Spectroscopy of Plasma Evolution from Astrophysical Radiation Mission
The Spectroscopy of Plasma Evolution from Astrophysical Radiation (or the Far-ultraviolet Imaging Spectrograph) instruments, flown aboard the STSAT-1 satellite mission, have provided the first large-area spectral mapping of the cosmic far ultraviolet (FUV, lambda 900-1750 Ang) background. We observe diffuse radiation from hot (10^4 to 10^6 K) and ionized plasmas, molecular hydrogen, and dust scattered starlight. These data provide for the unprecedented detection and discovery of spectral emission from a variety of interstellar environments, including the general medium, molecular clouds, supernova remnants, and super-bubbles. We describe the mission and its data, present an overview of the diffuse FUV sky's appearance and spectrum, and introduce the scientific findings detailed later in this volume.
H. Jin、J. Edelstein、I. -S. Yuk、K. I Seon、J. -T. Lim、B. Y. Welsh、E. Sim、J. -H. Park、J. -H. Shinn、J. Adolfo、K. Ryu、W. M. Feuerstein、K. Nishikida、K. W. Min、D. H. Lee、M. Bowen、W. Han、E. J. Korpela、K. McKee、U. -W. Nam、C. Heiles
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H. Jin,J. Edelstein,I. -S. Yuk,K. I Seon,J. -T. Lim,B. Y. Welsh,E. Sim,J. -H. Park,J. -H. Shinn,J. Adolfo,K. Ryu,W. M. Feuerstein,K. Nishikida,K. W. Min,D. H. Lee,M. Bowen,W. Han,E. J. Korpela,K. McKee,U. -W. Nam,C. Heiles.The Spectroscopy of Plasma Evolution from Astrophysical Radiation Mission[EB/OL].(2006-01-26)[2025-07-02].https://arxiv.org/abs/astro-ph/0601587.点此复制
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