Gotowe bibliografie tematyczne / Astrophysics Technique

Spis treści

  1. Artykuły w czasopismach
  2. Rozprawy doktorskie
  3. Książki
  4. Części książek
  5. Streszczenia konferencji

Gotowa bibliografia na temat „Astrophysics Technique”

Autor: Grafiati
Data publikacji: 4 czerwca 2021
Data aktualizacji: 31 stycznia 2023

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Artykuły w czasopismach na temat "Astrophysics Technique"

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Shen, Yang-Ping, Bing Guo, and Wei-Ping Liu. "An indirect technique in nuclear astrophysics: alpha-cluster transfer reaction." EPJ Web of Conferences 260 (2022): 01001. http://dx.doi.org/10.1051/epjconf/202226001001.

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Helium(4He, or α)is the second most abundant element in the observable Universe. The α-particle induced reactions such as(α, γ), (α, n) and (α, p) play a crucial role in nuclear astrophysics, especially for understanding stellar heliumburning. Because of the strong Coulomb repulsion, it is greatly hindered to directly measure the cross sections for these α-capture reactions at stellar energies. Alpha-cluster transfer reaction is a powerful tool for investigation of astrophysical(α, γ), (α, n)and(α, p)reactions since it can preferentially populate the natural-parity states with an α-cluster str
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Rahma, Siti Nur, Suliyanah Suliyanah, and Abdul Halim. "How do Astrophysics and the Qur'an Perceive the Extraterrestrial Life? A Qualitative Study." Jurnal Pendidikan Fisika 10, no. 2 (April 20, 2022): 107–22. http://dx.doi.org/10.26618/jpf.v10i2.7433.

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The topic of extraterrestrial life is still only a theory and the truth is still being investigated. Therefore, this research aims to analyze the beginning formation of the universe according to astrophysics and the Qur’an, astrophysics discoveries about extraterrestrial life, and letters in the Qur’an that hint at extraterrestrial life, as well as analyzing the relationship between astrophysics and letters in the Qur’an related to extraterrestrial life. This research is qualitative research with a method consisting of library research and interviews. The primary data of this research comes fr
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Longair, Malcolm. "Radio astronomy and the rise of high-energy astrophysics two anniversaries." International Journal of Modern Physics D 28, no. 02 (January 2019): 1930004. http://dx.doi.org/10.1142/s0218271819300040.

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This paper celebrates the 100th anniversary of the birth of Martin Ryle and the 50th anniversary of the discovery of pulsars by Jocelyn Bell and Antony Hewish. Ryle and Hewish received the 1974 Nobel Prize in Physics, the first in the area of astrophysics. Their interests strongly overlapped, one of the key papers on the practical implementation of the technique of aperture synthesis being co-authored by Ryle and Hewish. The discovery of pulsars and the roles played by Hewish and Bell are described. These key advances were at the heart of the dramatic rise of high-energy astrophysics in the 19
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Mukhamedzhanov, A. M., L. D. Blokhintsev, B. F. Irgaziev, A. S. Kadyrov, M. La Cognata, C. Spitaleri, and R. E. Tribble. "Trojan Horse as an indirect technique in nuclear astrophysics." Journal of Physics G: Nuclear and Particle Physics 35, no. 1 (December 13, 2007): 014016. http://dx.doi.org/10.1088/0954-3899/35/1/014016.

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Spitaleri, Claudio. "Trojan Horse technique to measure nuclear astrophysics rearrangement reactions." Journal of Physics: Conference Series 420 (March 25, 2013): 012137. http://dx.doi.org/10.1088/1742-6596/420/1/012137.

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Tumino, A., C. Spitaleri, S. Cherubini, V. Crucillà, C. Fu, Z. Elekes, Z. Fülöp, et al. "The trojan horse method as indirect technique in nuclear astrophysics." Journal of Physics: Conference Series 111 (May 1, 2008): 012033. http://dx.doi.org/10.1088/1742-6596/111/1/012033.

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Minier, Vincent, Gilles Durand, Pierre-Olivier Lagage, and M. Talvard. "CAMISTIC: THz/submm astronomy at Dome C in Antarctica." Proceedings of the International Astronomical Union 2, no. 14 (August 2006): 709–10. http://dx.doi.org/10.1017/s1743921307012367.

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Submillimetre (submm) astronomy is the prime technique to unveil the birth and early evolution of a broad range of astrophysical objects. It is a relatively new branch of observational astrophysics which focuses on studies of the cold Universe, i.e., objects radiating a significant – if not dominant – fraction of their energy at wavelengths ranging from ∼ 100 μm to ∼ 1 mm. Submm continuum observations are particularly powerful to measure the luminosities, temperatures and masses of cold dust emitting objects. Examples of such objects include star-forming clouds in our Galaxy, prestellar cores
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Bukvić, S., Dj Spasojević, and V. Žigman. "Advanced fit technique for astrophysical spectra." Astronomy & Astrophysics 477, no. 3 (November 12, 2007): 967–77. http://dx.doi.org/10.1051/0004-6361:20065969.

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Crossland, Tom, Pontus Stenetorp, Sebastian Riedel, Daisuke Kawata, Thomas D. Kitching, and Rupert A. C. Croft. "Towards machine-assisted meta-studies: the Hubble constant." Monthly Notices of the Royal Astronomical Society 492, no. 3 (December 23, 2019): 3217–28. http://dx.doi.org/10.1093/mnras/stz3400.

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ABSTRACT We present an approach for automatic extraction of measured values from the astrophysical literature, using the Hubble constant for our pilot study. Our rules-based model – a classical technique in natural language processing – has successfully extracted 298 measurements of the Hubble constant, with uncertainties, from the 208 541 available arXiv astrophysics papers. We have also created an artificial neural network classifier to identify papers in arXiv which report novel measurements. From the analysis of our results we find that reporting measurements with uncertainties and the cor
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SINNIS, GUS. "TeV ASTROPHYSICS WITH THE MILAGRO AND HAWC OBSERVATORIES." International Journal of Modern Physics D 22, no. 11 (September 2013): 1360010. http://dx.doi.org/10.1142/s0218271813600109.

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Ground-based gamma-ray astronomy has historically implemented two dramatically different techniques. One method employs Imaging Atmospheric Cherenkov Telescope(s) (IACT) that detect the Cherenkov light generated in the atmosphere by extensive air showers. The other method employs particle detectors that directly detect the particles that reach ground level — known as Extensive Air Shower (EAS) arrays. Until recently, the IACT method had been the only technique to yield solid detections of TeV gamma-ray sources. Utilizing water Chernkov technology, Milagro, was the first EAS array to discover n
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Rozprawy doktorskie na temat "Astrophysics Technique"

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MacRae, John Hamish Kenneth. "The detection of very high energy cosmic gamma rays using the atmospheric Cerenkov technique." Thesis, Durham University, 1985. http://etheses.dur.ac.uk/7854/.

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This thesis is concerned with the detection of very high energy cosmic gamma rays using the atmospheric Cerenkov technique. A general introduction to gamma ray detection techniques is followed by a detailed discussion of the principles of the atmospheric Cerenkov technique and the history of its use prior to this work. The design and operation of the University of Durham facility in Dugway, Utah is described in depth. Monte Carlo computer simulations have been developed to assist in both the understanding of the equipment and the analysis of the results for the Durham facility. The variation o
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Tisserand, Patrick. "Recherches d'astres sombres massifs du halo galactique par la technique des microlentilles gravitationnelles avec les caméras d'EROS-2." Phd thesis, Université de Nice Sophia-Antipolis, 2004. http://tel.archives-ouvertes.fr/tel-00008267.

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Le problème de la masse manquante galactique prend sa source dans l'étude des courbes de rotation des galaxies spirales. Une des hypothèses privilégiées durant les vingt dernières années est la présence d'un halo entourant chaque galaxie composé d'objets compacts sombres (les machos) qui peuvent être détectés indirectement par le phénomène gravitationnel de microlentille. Le travail présenté dans cette thèse concerne l'analyse des courbes de lumière de plus de 55 millions d'étoiles des deux Nuages de Magellan, observées de juin 1996 à février 2003, avec les caméras de l'expérience EROS2. Deux
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Filip, Münz. "La simulation électronique de CELESTE : étude des biais et application à l'obsevation de la Nébuleuse de Crabe." Phd thesis, Université Paris-Diderot - Paris VII, 2003. http://tel.archives-ouvertes.fr/tel-00003334.

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Cette thèse présente le domaine de l'astronomie gamma et les principales sources de notre Galaxie (pulsars et SNRs) et celles situées à des distances cosmologiques (noyaux actifs de galaxie). La technique Cerenkov permet aux observatoires au sol de détecter des rayons gamma d'énergie du GeV absorbés dans l'atmosphère après avoir développé une cascade électromagnétique. Le projet CELESTE a atteint le but d'un seuil bas de 30 GeV, utilisant une grande surface de collection de l'ancienne centrale solaire de Thémis (Pyrénées Orientales). Une étude des principaux éléments du dispositif - un système
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Kreckelbergh, Stephane. "Contrôle longitudinal et caractérisation optique du détecteur Virgo." Phd thesis, Université Paris Sud - Paris XI, 2005. http://tel.archives-ouvertes.fr/tel-00012159.

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Le détecteur Virgo est constitué d'un interféromètre de Michelson avec des cavités Fabry-Perot de 3 km de long dans les bras et utilise la technique de recyclage de puissance. Il a pour but la détection directe des ondes gravitationnelles émises par des sources astrophysiques. <br />Pour atteindre sa sensibilité, Virgo doit être emmené à son point de fonctionnement par des asservissements tant longitudinaux qu'angulaires. Pour cela, nous avons mis en place un algorithme de contrôle longitudinal ("lock") qui partant d'un interféromètre libre l'emmène à son point de fonctionnement. Pour arriver
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Platts, Emma. "Computational analysis techniques using fast radio bursts to probe astrophysics." Doctoral thesis, Faculty of Science, 2021. http://hdl.handle.net/11427/33921.

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This thesis focuses on Fast Radio Bursts (FRBs) and presents computational techniques that can be used to understand these enigmatic events and the Universe around them. Chapter 1 provides a theoretical overview of FRBs; providing a foundation for the chapters that follow. Chapter 2 details current understandings by providing a review of FRB properties and progenitor theories. In Chapter 3, we implement non-parametric techniques to measure the elusive baryonic halo of the Milky Way. We show that even with a limited data set, FRBs and an appropriate set of statistical tools can provide reasonab
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Lindgren, Sara. "Metallicity determination of M dwarfs." Doctoral thesis, Uppsala universitet, Observationell astrofysik, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-332102.

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M dwarfs constitute around 70% of all stars in the local Galaxy. Their multitude together with their long main-sequence lifetimes make them important for studies of global properties of the Galaxy such as the initial mass function or the structure and kinematics of stellar populations. In addition, the exoplanet community is showing an increasing interest for those small, cold stars. However, very few M dwarfs are well characterized, and in the case of exoplanetary systems the stellar parameters have a direct influence on the derived planet properties. Stellar parameters of M dwarfs are diffic
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Sajjad, Saeeda. "Développement d'outils de simulation et de reconstruction de gerbes de particules pour l'astronomie gamma avec les futurs imageurs Tcherenkov." Phd thesis, Université Montpellier II - Sciences et Techniques du Languedoc, 2007. http://tel.archives-ouvertes.fr/tel-00408835.

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Le futur de l'astronomie gamma au sol repose sur l'utilisation de grands réseaux d'imageurs Tcherenkov atmosphériques (IACT) avec des capacités améliorées : seuil en énergie plus bas, meilleure sensibilité, meilleurs résolution et pouvoir de rejet. Pour concevoir ces systèmes et optimiser leurs caractéristiques, il est nécessaire de comprendre les gerbes atmosphériques et de disposer d'outils de simulation adaptés permettant d'évaluer les performances des réseaux. La première partie de cette thèse traite des gerbes atmosphériques, des propriétés de la lumière Tcherenkov qu'elles émettent et de
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Popescu, Marcel. "Techniques d'observation spectroscopique d'astéroïdes." Phd thesis, Observatoire de Paris, 2012. http://tel.archives-ouvertes.fr/tel-00785991.

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L'objectif fondamental des sciences planétaires est la compréhension de la formation et de l'évolution du Système Solaire. Pour atteindre cet objectif les astéroïdes présentent un intérêt tout particulier pour la communauté scientifique. En effet, nous pouvons regarder la population astéroïdale comme une fenêtre vers le passée, par laquelle nous regardons les débuts de la formation du système planétaire. Ils sont les témoins des premiers moments de la formation des planètes gardant dans leur structure la complexité chimique de la nébuleuse primordiale. Pour cette raison, les études physiques e
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Adamakis, Sotiris. "Application of statistical analysis techniques to solar and stellar phenomena." Thesis, University of Central Lancashire, 2009. http://clok.uclan.ac.uk/20908/.

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Currently, solar observers are investigating spectroscopic images of the Sun's outermost atmosphere (the corona), which are challenging long-held views on the density and temperature structure of this environment. The corona is "filled" with magnetic strands but determining their precise nature is not straightforward. One way of revealing the nature of the coronal heating mechanism is by comparing simple theoretical one dimensional hydrostatic loop models with observations of the temperature and/or density structure along these features. The most wellknown method for dealing with comparisons l
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Hills, Graeme Lawrence. "The application of polarimetric techniques to gamma ray astronomy." Thesis, University of Southampton, 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.243187.

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Książki na temat "Astrophysics Technique"

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Observational astrophysics. Cambridge: Cambridge University Press, 1995.

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P, Ehrenfreund, ed. Laboratory astrophysics and space research. Boston: Kluwer Academic Publishers, 1999.

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International, School of Physics "Enrico Fermi" (1989 Varenna Italy). Solid-state astrophysics: 27 June-7 July 1989. Amsterdam: North-Holland, 1991.

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Kitchin, C. R. Astrophysical techniques. 5th ed. Boca Raton: CRC Press, 2008.

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Kitchin, C. R. Astrophysical techniques. 4th ed. Bristol: Institute of Physics Pub., 2003.

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Kitchin, C. R. Astrophysical techniques. 3rd ed. Bristol: Institute of Physics Pub., 1998.

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Kitchin, C. R. Astrophysical techniques. 2nd ed. Bristol [England]: IOP Pub., 1991.

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(Claudio), Spitaleri C., Rolfs Claus E, and Pizzone Rosario Gianluca, eds. Fifth European Summer School on Experimental Nuclear Astrophysics, Santa Tecla, Sicily, Italy, 20-27 September 2009. Melville, N.Y: American Institute of Physics, 2010.

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van, Paradijs J., Maitzen H. M. 1943-, and European Astrophysics Doctoral Network, eds. Galactic high-energy astrophysics ; High-accuracy timing and positional astronomy: Lectures held at the Astrophysics School IV, organized by the European Astrophysics Doctoral Network (EADN) in Graz, Austria, 19-31 August 1991. Berlin: Springer-Verlag, 1993.

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Liège International Astrophysical Colloquium (27th 1987). Observational astrophysics with high precision data: Proceedings of the 27th Liège International Astrophysical Colloquium, June 23-26, 1987. Cointe-Ougrée, Belgique: Université de Liège, Institut d'astrophysique, 1987.

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Części książek na temat "Astrophysics Technique"

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Rowe, B. R., J. B. Marquette, and G. Dupeyrat. "Measurements Of Ion-Molecule Reaction Rate Coefficients Between 8 and 160 K by the Cresu Technique." In Molecular Astrophysics, 631–38. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5432-8_31.

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Porter, N. A. "The Atmospheric Čerenkov Technique in the Search for PBH." In TeV Gamma-Ray Astrophysics, 67–69. Dordrecht: Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0171-1_6.

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Fors, O., and J. Núñez. "CCD Scanning Technique Applied to Millisecond Photometric Observations." In Highlights of Spanish Astrophysics II, 293–96. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-017-1776-2_68.

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Weekes, Trevor C. "The Atmospheric Cherenkov Technique in Very High Energy Gamma-Ray Astronomy." In TeV Gamma-Ray Astrophysics, 1–15. Dordrecht: Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0171-1_1.

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Singh, Puneet, Amit Chatterjee, Vimal Bhatia, and Shashi Prakash. "Viability Assessment of Kidney Bean Seed (Phaseolus Vulgaris sp.) Using Robust Biospeckle Indexing Technique." In Computational Mathematics, Nanoelectronics, and Astrophysics, 189–95. Singapore: Springer Singapore, 2021. http://dx.doi.org/10.1007/978-981-15-9708-4_18.

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Champavert, N., and H. Wozniak. "A New Chemodynamical Tool to Study the Evolution of Galaxies in the Local Universe: a Quick and Accurate Numerical Technique to Compute the Gas Cooling Rate for any Chemical Composition." In Eso Astrophysics Symposia, 409–11. Berlin, Heidelberg: Springer Berlin Heidelberg, 2007. http://dx.doi.org/10.1007/978-3-540-73484-0_75.

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Lestrade, Jean-François, Alan E. E. Rogers, Arthur E. Niell, and Robert A. Preston. "Astrometry of Millijansky Sources using a Phase Reference VLBI Technique." In The Impact of VLBI on Astrophysics and Geophysics, 323–24. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2949-4_109.

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Kankainen, A., Yu N. Novikov, H. Schatz, and C. Weber. "Mass measurements of neutron-deficient nuclei and their implications for astrophysics." In Three decades of research using IGISOL technique at the University of Jyväskylä, 345–63. Dordrecht: Springer Netherlands, 2012. http://dx.doi.org/10.1007/978-94-007-5555-0_27.

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Gupta, Sumit, Devendra Kumar, Jagdev Singh, and Sushila. "An Efficient Computational Technique for Nonlinear Emden-Fowler Equations Arising in Astrophysics and Space Science." In 4th International Conference on Computational Mathematics and Engineering Sciences (CMES-2019), 76–98. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-39112-6_5.

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Wood, Matt. "Numerical Techniques in Astrophysics." In Planets, Stars and Stellar Systems, 481–502. Dordrecht: Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-5618-2_11.

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Streszczenia konferencji na temat "Astrophysics Technique"

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Mukha, Ivan, Hajime Susa, Marcel Arnould, Sydney Gales, Tohru Motobayashi, Christoph Scheidenberger, and Hiroaki Utsunomiya. "2p radioactivity studied by tracking technique." In TOURS SYMPOSIUM ON NUCLEAR PHYSICS AND ASTROPHYSICS—VII. AIP, 2010. http://dx.doi.org/10.1063/1.3455942.

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Ivashchenko, Ganna, Olga Sergijenko, and Olena Torbaniuk. "Improved technique for quasar composite spectra generation." In VI European Summer School on Experimental Nuclear Astrophysics. Trieste, Italy: Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.148.0007.

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Garcia, Iskya. "Water Cherenkov Detector installation by the Vertical Muon Equivalent technique." In 4th School on Cosmic Rays and Astrophysics. Trieste, Italy: Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.118.0009.

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Hadinia, B. "First Identification of γ-rays in 106Te Using Recoil Decay Tagging Technique". У FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS - FINUSTAR. AIP, 2006. http://dx.doi.org/10.1063/1.2200981.

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Brown, J. R., M. A. Bentley, M. J. Taylor, P. Aldrich, D. Bazin, J. M. Cook, C. A. Diget, et al. "Mirrored Fragmentation Reactions—A New Technique for Probing Isospin Symmetry in Exotic Nuclei." In FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2. AIP, 2008. http://dx.doi.org/10.1063/1.2939325.

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Doukellis, G., G. Galios, S. Kossionides, and Themis Paradellis. "Novel technique for measurements of neutron cross sections and its application to nuclear astrophysics." In 4th International Conference on Applications of Nuclear Techniques: Neutrons and their Applications, edited by George Vourvopoulos and Themis Paradellis. SPIE, 1995. http://dx.doi.org/10.1117/12.204199.

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Kwak, Kyujin. "Numerical Simulation of 2-D Relativistic Hydrodynamics Using Adaptive Mesh Refinement Technique." In GAMMA-RAY BURSTS IN THE SWIFT ERA: Sixteenth Maryland Astrophysics Conference. AIP, 2006. http://dx.doi.org/10.1063/1.2207878.

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Karimabadi, H. "A New Simulation Technique for Study of Collisionless Shocks: Self-Adaptive Simulations." In THE PHYSICS OF COLLISIONLESS SHOCKS: 4th Annual IGPP International Astrophysics Conference. AIP, 2005. http://dx.doi.org/10.1063/1.2032675.

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BOYLE, PATRICK J. "DEVELOPMENT OF THE IMAGING ATMOSPHERIC CHERENKOV TECHNIQUE AT THE WHIPPLE OBSERVATORY." In Proceedings of the 13th Course of the International School of Cosmic Ray Astrophysics. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812702968_0028.

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Connors, Riley, David van Eijnatten, Chiara Ceccobello, and Sera Markoff. "Using a joint spectral fitting technique to explore the outflow geometry of GX 339-4 during the hard state." In 11th INTEGRAL Conference Gamma-Ray Astrophysics in Multi-Wavelength Perspective. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.285.0071.

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Możesz być także zainteresowany rozszerzonymi bibliografiami na temat „Astrophysics Technique” dla poszczególnych typów źródeł:
Artykuły w czasopismach Rozprawy doktorskie Książki
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Do bibliografii