Treffer: Observation of the CIV effect in interstellar clouds : A speculation on the physical mechanism for their existence : Space and cosmic plasma
Title:
Observation of the CIV effect in interstellar clouds : A speculation on the physical mechanism for their existence : Space and cosmic plasma
Authors:
Source:
IEEE transactions on plasma science. 28(6):2122-2127
Publisher Information:
New York, NY: Institute of Electrical and Electronics Engineers, 2000.
Publication Year:
2000
Physical Description:
print, 23 ref
Original Material:
INIST-CNRS
Subject Terms:
Nuclear physics, Physique nucléaire, Plasma physics, Physique des plasmas, Sciences exactes et technologie, Exact sciences and technology, Physique, Physics, Generalites, General, Instruments, appareillage, composants et techniques communs à plusieurs branches de la physique et de l'astronomie, Instruments, apparatus, components and techniques common to several branches of physics and astronomy, Instruments, appareillage et composants en technique et recherche spatiale (satellite, engin spatial, etc.), Spaceborne and space research instruments, apparatus and components (satellites, space vehicles, etc.), Terre, ocean, espace, Earth, ocean, space, Astronomie, Astronomy, Astronomie fondamentale et astrophysique. Instrumentation, techniques, et observations astronomiques, Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations, Divers (incluant l'archéoastronomie), Historical astronomy and archaeoastronomy; and other topics in fundamental astronomy and astrophysics; instrumentation, techniques, and astronomical observations, Systèmes stellaires. Objets et systèmes galactiques et extragalactiques. L'univers, Stellar systems. Galactic and extragalactic objects and systems. The universe, Divers, Other topics on stellar systems; galactic and extragalactic objects and systems; the universe, Spaceborne and space research instruments, apparatus, and components (satellites, space vehicles, etc.), Astronomical and space-research instrumentation, Interstellar medium (ISM) and nebulae in external galaxies, Charge électrostatique, Electrostatic charge, Carga electrostática, Etude théorique, Theoretical study, Ionisation, Ionization, Nuage interstellaire, Interstellar clouds, Plasma, Potentiel ionisation, Ionization potential, Vitesse critique, Critical velocity
Document Type:
Fachzeitschrift
Article
File Description:
text
Language:
English
Author Affiliations:
U. S. Department of Energy, Washington, DC 20585, United States
Los Alamos National Laboratory, Los Alamos, NM 87545, United States
Physics Department, University of Memphis, Memphis, TN 38152, United States
Los Alamos National Laboratory, Los Alamos, NM 87545, United States
Physics Department, University of Memphis, Memphis, TN 38152, United States
ISSN:
0093-3813
Rights:
Copyright 2001 INIST-CNRS
CC BY 4.0
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
CC BY 4.0
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
Notes:
Astronomy
Metrology
Metrology
Accession Number:
edscal.882618
Database:
PASCAL Archive
Weitere Informationen
Observations of neutral hydrogen (HI) emission profiles produced by gas in the local interstellar medium are found to be characterized by four linewidth regimes. Dominant and pervasive features have widths on average of 5.2, 13, and 31 km/s, and a very broad component approximately 50 km/s wide. A striking coincidence exists between these linewidths and the magnitudes of the critical ionization velocities of the most abundant atomic species in interstellar space: 6 km/s for sodium and calcium; 13 km/s for carbon, oxygen, and nitrogen; 34 km/s for helium; and 51 km/s for hydrogen. The data relate to observations near neutral hydrogen structures that are filamentary.