Thematische Bibliographien / Far Ultraviolet Spectroscopic Explorer

Auswahl der wissenschaftlichen Literatur zum Thema „Far Ultraviolet Spectroscopic Explorer“

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Veröffentlicht am 26. Juli 2024

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Zeitschriftenartikel zum Thema "Far Ultraviolet Spectroscopic Explorer"

Moos, Warren. „Lyman the far Ultraviolet Spectroscopic Explorer“. International Astronomical Union Colloquium 123 (1990): 171–76. http://dx.doi.org/10.1017/s0252921100077009.

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AbstractThe Lyman Far Ultraviolet Spectroscopic Explorer mission will obtain high resolution spectra (R 30,000) in the 912–1200 Å region with sufficient sensitivity to study faint sources throughout the galaxy and at large extragalactic distances. This spectral region provides unique tools for solving problems in cosmology (e.g. deuterium), galactic structure and evolution (e.g. O VI and H2), stellar evolution (e.g. O VI) and planetary science (e.g. H2). Recent advances in optical and detector technology, which make this goal possible with a moderate size experimental package, also enable the spectral coverage to extend down to 100 Å with good sensitivity and only a minimal increase in complexity. Thus a secondary goal is to cover the 100–912 Å region with moderate spectral resolution. In 1989, following a Phase A study of the mission concept, NASA selected the mission for Phase A study in 1989. Both Canada and the United Kingdom are participating in the definition and development of the mission.

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Moos, Warren. „The Lyman far ultraviolet spectroscopic explorer“. Advances in Space Research 11, Nr. 11 (Januar 1991): 221–27. http://dx.doi.org/10.1016/0273-1177(91)90079-y.

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Feldman, Paul D. „Spectroscopy of Comets with the Far Ultraviolet Spectroscopic Explorer Satellite“. Physica Scripta T119 (01.01.2005): 7–12. http://dx.doi.org/10.1088/0031-8949/2005/t119/001.

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Young, P. R., A. K. Dupree, B. E. Wood, S. Redfield, J. L. Linsky, T. B. Ake und H. W. Moos. „[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of Capella“. Astrophysical Journal 555, Nr. 2 (10.07.2001): L121—L124. http://dx.doi.org/10.1086/322863.

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Sonneborn, G., H. W. Moos und K. R. Sembach. „In-Orbit Performance of the Far Ultraviolet Spectroscopic Explorer“. Symposium - International Astronomical Union 198 (2000): 244–46. http://dx.doi.org/10.1017/s0074180900166677.

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The Far Ultraviolet Spectroscopic Explorer (FUSE) satellite was launched by a Delta II rocket on 24 June 1999 into a ˜768 km, 25° orbit. Following the In-Orbit Checkout phase, FUSE is obtaining high-resoluti on spectra (λ/Δλ ≳ 20,000) in the spectral range 905 −1187 Å. The sensitivity meets or exceeds the pre-launch predictions. Many QSOs and AGNs have already been observed.

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Murthy, Jayant, und David J. Sahnow. „Observations of the Diffuse Far‐Ultraviolet Background with theFar Ultraviolet Spectroscopic Explorer“. Astrophysical Journal 615, Nr. 1 (November 2004): 315–22. http://dx.doi.org/10.1086/424441.

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Blair, William P., Parviz Ghavamian, Ravi Sankrit und Charles W. Danforth. „Far Ultraviolet Spectroscopic Explorer Survey of Magellanic Cloud Supernova Remnants“. Astrophysical Journal Supplement Series 165, Nr. 2 (August 2006): 480–511. http://dx.doi.org/10.1086/505346.

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Moos, H. W., W. C. Cash, L. L. Cowie, A. F. Davidsen, A. K. Dupree, P. D. Feldman, S. D. Friedman et al. „Overview of the [ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Mission“. Astrophysical Journal 538, Nr. 1 (20.07.2000): L1—L6. http://dx.doi.org/10.1086/312795.

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Hutchings, J. B., A. W. Fullerton, A. P. Cowley und P. C. Schmidtke. „[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] 900–1200 Å Spectroscopy of AM Herculis“. Astronomical Journal 123, Nr. 5 (Mai 2002): 2841–46. http://dx.doi.org/10.1086/340080.

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Murphy, E. M., K. R. Sembach, B. K. Gibson, J. M. Shull, B. D. Savage, K. C. Roth, H. W. Moos, J. C. Green, D. G. York und B. P. Wakker. „[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Spectroscopy of High-Velocity Cloud Complex C“. Astrophysical Journal 538, Nr. 1 (20.07.2000): L35—L38. http://dx.doi.org/10.1086/312801.

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Dissertationen zum Thema "Far Ultraviolet Spectroscopic Explorer"

Dunn, Jay Patrick. „Intrinsic Absorption with the Far Ultraviolet Spectroscopic Explorer“. Digital Archive @ GSU, 2007. http://digitalarchive.gsu.edu/phy_astr_diss/21.

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We present a survey of 72 Seyfert galaxies and quasars observed by the Far Ultraviolet Spectroscopic Explorer (FUSE). Our survey is the largest to date searching for intrinsic UV absorption with high spectral resolution, and is the first step toward a more comprehensive study of intrinsic absorption in low-redshift AGN. We have determined that 72 of 253 available active galactic nuclei (AGN) are viable targets for detection of intrinsic absorption lines. We examined these spectra for signs of intrinsic absorption in the O VI doublet (lambda lamdba 1031.9, 1037.6) and Lyman beta (lambda 1025.7). The fraction of Seyfert 1 galaxies and low-redshift quasars at z<0.15 that show evidence of intrinsic UV absorption is ~50, which is slightly lower than Crenshaw et al. found (60%) based on a smaller sample of C IV absorption in Seyfert 1 galaxies observed with the Hubble Space Telescope (HST). The intrinsic absorption lines are mostly blueshifted with respect to the rest frame of the galaxy, indicating outflow of ionized gas from the AGN. With this new fraction we find a global covering factor of the absorbing gas with respect to the central nucleus of ~0.4. We also provide a deeper analysis of the intrinsic absorption features we found in 35 objects. We have characterized the relation between luminosity and velocity, and examined the relationships between equivalent width, full width at half maximum, velocity and continuum flux. The luminosity/velocity correlation has been explored previously by Laor & Brandt (2002), but at a significantly higher redshift and heavily weighted by Broad Absorption Line quasars. Our survey is for lower redshift and lower luminosity objects, mostly Seyfert galaxies. We have also explored each object with multiple observations for variablity in each of the aforementioned quantities and characterized the variation of equivalent width with continuum flux. Variability for low-z AGN has been seen in the past. In our survey, we find that variability of O VI (lambda lambda 1032, 1038) is less common than for the UV doublets of C IV and N V seen at longer wavelengths, because the O VI absorption is usually saturated. Lyman beta absorption variability is more frequent. In the target-by-target examination we find that Broad Absorption Line (BAL) features and Narrow Absorption Line (NAL) features are related, in that they follow a single relationship between the maximum outflow velocity and the AGN luminosity, and both can be exhibited in similar luminosity objects. IRAS F22456-5125 is one particular Seyfert galaxy that we have selected for modelling due to its interesting assortment of intrinsic absorption lines. It shows a system of five individual kinematic components of absorption features in both O VI lines and in several of the Lyman series lines. We find that each of the components are relatively simple to model and appear to be weak in the X-ray.

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Dauer, Véronique. „Spectroscopie à haute résolution dans l'ultraviolet lointain : étude des performances des réseaux du spectrographe spatial FUSE (Far Ultraviolet Spectroscopic explorer) ; amélioration de l'efficacité de ces réseaux par usinage ionique“. Aix-Marseille 3, 1998. http://www.theses.fr/1998AIX30117.

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Le spectrographe fuse (far ultraviolet spectroscopic explorer) de la nasa a pour but d'etudier la bande ultraviolette 90-120 nm avec une haute resolution spatiale ( de 0. 003 nm). Pour atteindre cette performance, des reseaux de diffraction holographiques, spheriques, de haute densite de traits (6000 traits/mm), corriges de certaines aberrations et de dimensions de 3030 cm 2 ont ete choisis. Une partie du travail de these presente ici consiste en l'etude des performances en resolution, efficacite et lumiere parasite des six reseaux de diffraction du spectrographe fuse. Le banc de test et la procedure adoptee pour aligner chaque reseau sont presentes. Les spectres experimentaux sont compares aux spectres theoriques obtenus avec un logiciel de simulation. Une simulation numerique basee sur la theorie electromagnetique des reseaux de diffraction et destinee a ameliorer l'efficacite des reseaux de l'experience fuse a permis l'optimisation des parametres d'enregistrement. Le taux de lumiere parasite de ces reseaux est tres faible, de l'ordre de 10 - 5 a 1 nm de la raie d'emission. Afin d'augmenter encore l'efficacite de diffraction, un programme de recherche et technologie en vue de modifier le profil sinusoidal de reseaux holographiques de 6000 traits/mm par usinage ionique est en cours. Dans le cadre de cette action, un programme de simulation d'erosion directionnelle a notamment ete elabore dans le but de prevoir l'evolution de la topographie de profils usines et d'obtenir un profil dissymetrique optimise pour la mission fuse. Ce programme de recherche et technologie a abouti a l'augmentation significative de l'efficacite des reseaux de type fuse.

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Cicerrella, Elizabeth. „Dielectric functions and optical bandgaps of high-K dielectrics by far ultraviolet spectroscopic ellipsometry /“. Full text open access at:, 2006. http://content.ohsu.edu/u?/etd,2.

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Bücher zum Thema "Far Ultraviolet Spectroscopic Explorer"

Future Directions in Ultraviolet Spectroscopy Conference (2008 Annapolis, Md.). Future directions in ultraviolet spectroscopy: A conference inspired by the accomplishments of the Far Ultraviolet Spectroscopic Explorer Mission : Annapolis, Maryland, 20-22 October 2008. Herausgegeben von Sonneborn George. Melville, N.Y: American Institute of Physics, 2009.

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United States. National Aeronautics and Space Administration., Hrsg. Global auroral imaging for the Dynamics Explorer mission: NAG5-483 : summary of research, November 01, 1984-January 31, 1998. Iowa City, IA: Dept. of Physics and Astronomy, University of Iowa, 1998.

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National Aeronautics and Space Administration (NASA) Staff. Pre-Phase A: Development of a Far-Ultraviolet Photometric- and Spectroscopic-Survey Small-Explorer Experiment. Independently Published, 2018.

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Buchteile zum Thema "Far Ultraviolet Spectroscopic Explorer"

Moos, Warren. „Lyman the Far Ultraviolet Spectroscopic Explorer“. In Observatories in Earth Orbit and Beyond, 171–76. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-011-3454-5_19.

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Hoard, D. W., und Paula Szkody. „Observations of Cataclysmic Variables With the Far Ultraviolet Spectroscopic Explorer“. In Astrophysics and Space Science Library, 201–6. Dordrecht: Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-0403-8_28.

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Martin, C., und J. Steiner. „Far-Ultraviolet Background Studies with the Pan-American Astrophysics Explorer (PAX)“. In The Galactic and Extragalactic Background Radiation, 456–58. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0653-2_92.

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Stoicheff, Boris P. „Spectroscopic studies in the far ultraviolet (80-200nm) using nonlinear tunable sources“. In Frontiers in Nonlinear Optics, 26–51. Boca Raton: CRC Press, 2021. http://dx.doi.org/10.1201/9781003209638-3.

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MOOS, WARREN, und SCOTT D. FRIEDMAN. „THE LYMAN FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER“. In Extreme Ultraviolet Astronomy, 457–63. Elsevier, 1991. http://dx.doi.org/10.1016/b978-0-08-037302-7.50055-0.

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Atkins, Peter, George Ratcliffe, Mark Wormald und Julio de Paula. „Ultraviolet and visible spectroscopy“. In Physical Chemistry for the Life Sciences. Oxford University Press, 2023. http://dx.doi.org/10.1093/hesc/9780198830108.003.0055.

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This chapter turns to ultraviolet and visible spectroscopy. The spectroscopic techniques which use electromagnetic radiation in the visible and ultraviolet region explore transitions in which the distribution of electrons changes. However, when electrons are excited from one molecular orbital to another, the molecule bursts into vibration and the absorption in biochemically interesting media are spread over many wavelengths. The general features of absorption in this region of the electromagnetic spectrum can be discussed in terms of groups of atoms with characteristic absorption and the transitions of d-electrons in metalloproteins. Techniques have been developed that use another feature of radiation, the possibility that it is polarized.

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„12. Carryover of Sampling Errors and Other Problems in Far-Infrared to Far-Ultraviolet Spectra to Associated Applications“. In Spectroscopic Methods in Mineralogy and Material Sciences, 481–508. De Gruyter, 2014. http://dx.doi.org/10.1515/9781614517863.481.

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Konferenzberichte zum Thema "Far Ultraviolet Spectroscopic Explorer"

Cash, Webster. „Optics for Lyman, The Far Ultraviolet Spectroscopic Explorer“. In Space Optics for Astrophysics and Earth and Planetary Remote Sensing. Washington, D.C.: Optica Publishing Group, 1988. http://dx.doi.org/10.1364/soa.1988.tuc3.

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Lyman, the Far Ultraviolet Explorer, is a space astrophysics mission designed to explore the spectra of celestial sources in the ultraviolet from 100 to 1250Å, the gap between the Hubble Space Telescope and the Advanced X-ray Astrophysics Facility. Lyman was recently selected by NASA as one of four missions to enter Phase A studies with a goal of launch in the mid-1990’s. It is envisioned as a community observatory in the tradition of the International Ultraviolet Explorer.

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Sahnow, David J., Henry W. Moos, Scott D. Friedman, William P. Blair, Steven J. Conard, Jeffrey W. Kruk, Edward M. Murphy, William R. Oegerle und Thomas B. Ake III. „Far Ultraviolet Spectroscopic Explorer: one year in orbit“. In International Symposium on Optical Science and Technology, herausgegeben von Silvano Fineschi, Clarence M. Korendyke, Oswald H. W. Siegmund und Bruce E. Woodgate. SPIE, 2000. http://dx.doi.org/10.1117/12.410516.

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Conard, Steven J., Robert H. Barkhouser, Jordan P. Evans, Scott D. Friedman, Jeffrey W. Kruk, Henry W. Moos, Raymond G. Ohl IV und David J. Sahnow. „Far Ultraviolet Spectroscopic Explorer optical system: lessons learned“. In International Symposium on Optical Science and Technology, herausgegeben von Silvano Fineschi, Clarence M. Korendyke, Oswald H. W. Siegmund und Bruce E. Woodgate. SPIE, 2000. http://dx.doi.org/10.1117/12.410522.

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Green, James C., Erik Wilkinson und Scott D. Friedman. „Design of the Far Ultraviolet Spectroscopic Explorer spectrograph“. In SPIE's 1994 International Symposium on Optics, Imaging, and Instrumentation, herausgegeben von Silvano Fineschi. SPIE, 1994. http://dx.doi.org/10.1117/12.193190.

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Ohl IV, Raymond G., Robert H. Barkhouser, Steven J. Conard, Scott D. Friedman, Jeffrey Hampton, Henry W. Moos, Paul Nikulla, Cristina M. Oliveira und Timo T. Saha. „Performance of the Far Ultraviolet Spectroscopic Explorer mirror assemblies“. In International Symposium on Optical Science and Technology, herausgegeben von Silvano Fineschi, Clarence M. Korendyke, Oswald H. W. Siegmund und Bruce E. Woodgate. SPIE, 2000. http://dx.doi.org/10.1117/12.410517.

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Sahnow, David J., Cathleen VanDyke, Qian Gong, James C. Bremer und Michael J. Kennedy. „Optical performance budget for the Far Ultraviolet Spectroscopic Explorer“. In SPIE's 1996 International Symposium on Optical Science, Engineering, and Instrumentation, herausgegeben von Robert E. Fischer und Warren J. Smith. SPIE, 1996. http://dx.doi.org/10.1117/12.256237.

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Osantowski, John F., Pam M. Davila und Timo T. Saha. „Telescope Technology For The Far Ultraviolet Spectroscopic Explorer (FUSE)“. In 29th Annual Technical Symposium, herausgegeben von Gregory M. Sanger. SPIE, 1986. http://dx.doi.org/10.1117/12.950409.

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Kennedy, Michael J., Scott D. Friedman, Robert H. Barkhouser, Jeffrey Hampton und Paul Nikulla. „Design of the Far Ultraviolet Spectroscopic Explorer mirror assemblies“. In SPIE's 1996 International Symposium on Optical Science, Engineering, and Instrumentation, herausgegeben von Pierre Y. Bely und James B. Breckinridge. SPIE, 1996. http://dx.doi.org/10.1117/12.255098.

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Conard, Steven J., Kevin W. Redman, Robert H. Barkhouser und Joel A. Johnson. „Optical alignment of the Far-Ultraviolet Spectroscopic Explorer (FUSE)“. In SPIE's International Symposium on Optical Science, Engineering, and Instrumentation, herausgegeben von Oswald H. W. Siegmund und Kathryn A. Flanagan. SPIE, 1999. http://dx.doi.org/10.1117/12.366541.

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Gordon, Karl D., Stefan Cartledge, Geoffrey Clayton, Michael E. Van Steenberg, George Sonneborn, H. Warren Moos und William P. Blair. „FUSE Far Ultraviolet Dust Extinction Curves“. In FUTURE DIRECTIONS IN ULTRAVIOLET SPECTROSCOPY: A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic Explorer Mission. AIP, 2009. http://dx.doi.org/10.1063/1.3154027.

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