Academic literature on the topic 'Comete halley'

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Journal articles on the topic "Comete halley"

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Heudier, Jean-Louis. "Comet Halley: A Media Event." International Astronomical Union Colloquium 98 (1988): 205–7. http://dx.doi.org/10.1017/s0252921100092915.

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Comet P/Halley’s life as a “media event” started long ago, because the first use of communication (in the modern sense of the term) goes back to Rabelais, who published in Patagrueline Prognostication pour l’an 1532:“And whyth the comete sene laste yeare and the retrograte of Saturne a greate skoundrell shalle die, all weazynge and courd in scabbes, in the hospitall, and at his death there will be horrible warre between cattes and rattes, dogges and hares, faulcons and duckes, monkes and egges.”Since then ways of spreading ideas have progressed enormously, but comets have remained “fashionable
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Alexandre, Josette. "La comete de Halley a travers les ouvrages et manuscrits de l'Observatoire de Paris." Isis 77, no. 1 (1986): 79–84. http://dx.doi.org/10.1086/354040.

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A'Hearn, Michael F. "Coordinated programs for comet Halley." Symposium - International Astronomical Union 118 (1986): 223–35. http://dx.doi.org/10.1017/s0074180900151356.

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Because comets are so difficult to observe, it is essential to coordinate observations from a variety of telescopes in order to fully understand their behavior. The apparition of Comet Halley represents a unique opportunity for coordinated programs because this is the only predictable comet which is routinely bright enough for the many observational programs desired. The International Halley Watch is playing an advocacy and coordinating role in the observations of Halley. Coordinated photographic observations will provide a record of the development of jets in the coma and of the motion of fea
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Keller, Horst Uwe. "Comets : A Key to Solar System Formation." Zeitschrift für Naturforschung A 44, no. 10 (1989): 867–76. http://dx.doi.org/10.1515/zna-1989-1001.

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Abstract Four lines of information on comets are discussed: their orbits, their relation to other bodies of the planetary system, their physical state and chemical composition, and implications of recent observations of the nucleus of comet Halley. The in situ measurements during the flybys of comet Halley strongly support the assumption that comets are members of the solar system and were created during its formation. The region (heliocentric distance) of their formation is, however, still difficult to assess. The size, shape, and topography of the cometary nucleus suggest that it was formed
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Hage, Joniek I., and J. Mayo Greenberg. "The Dust in the Coma of Comet Halley." International Astronomical Union Colloquium 126 (1991): 261–64. http://dx.doi.org/10.1017/s0252921100066914.

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AbstractThe interstellar dust model of comets is numerically worked out to satisfy several basic constraints provided by observations of comet Halley and to derive the porosity of coma dust. The observational constraints are: (1) the strengths of the 3.4 μm and 9.7 μm emission bands; (2) the relative amount of silicates to organic materials; (3) the mass distribution of the dust. The results indicate that coma dust has a porosity in the range 0.93 < P < 0.975. Preliminary calculations concerning the observed linear polarization of comet Halley are presented.
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Pater, Imke de, Patrick Palmer, and Lewis E. Snyder. "A Review of Radio Interferometric Imaging of Comets." International Astronomical Union Colloquium 116, no. 1 (1989): 175–207. http://dx.doi.org/10.1017/s0252921100109686.

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AbstractWe present an overview of cometary observations carried out with the VLA. These include OH imaging observations, studies of other molecules and searches for continuum emission. Primarily, we discuss the OH observations obtained of Comet Halley, a periodic comet, and Comet Wilson, a “new” comet. The emission from Comet Halley is confined to a region a few times 105 km. The emission from Comet Wilson shows sporadic blobs at large distances (∼ 106 km from the center), which vary abruptly in both position and velocity. The generally accepted picture of excitation by UV pumping in a spheric
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Olivares, Jorge. "A Twice-Told Tail: Reinaldo Arenas's “El Cometa Halley”." PMLA/Publications of the Modern Language Association of America 117, no. 5 (2002): 1188–206. http://dx.doi.org/10.1632/003081202x60279.

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This essay analyzes the articulation of transgressive desires in Reinaldo Arenas's “El Cometa Halley,” a parodic continuation of Federico García Lorca's La casa de Bernarda Alba. I argue that by moving the Alba sisters from Spain to Cuba and liberating their repressed sexualities, Arenas pursues his fantasies of sexual freedom. Linking his rewriting of García Lorca to the historically significant arrival of Halley's comet in 1910, Arenas relies on the comet's phallic tail to set the story in motion. More specifically, “El Cometa Halley” sketches a preoedipal fantasy of mother-son incest that r
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Soja, R. H., E. Grün, P. Strub, et al. "IMEM2: a meteoroid environment model for the inner solar system." Astronomy & Astrophysics 628 (August 2019): A109. http://dx.doi.org/10.1051/0004-6361/201834892.

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Context. The interplanetary dust complex is currently understood to be largely the result of dust production from Jupiter-family comets, with contributions also from longer-period comets (Halley- and Oort-type) and collisionally produced asteroidal dust. Aims. Here we develop a dynamical model of the interplanetary dust cloud from these source populations in order to develop a risk and hazard assessment tool for interplanetary meteoroids in the inner solar system. Methods. The long-duration (1 Myr) integrations of dust grains from Jupiter-family and Halley-type comets and main belt asteroids w
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Chapman, C. R., L. Kresak, B. D. Donn, et al. "Commission 15: Physical Study of Comets, Minor Planets, and Meteorites." Transactions of the International Astronomical Union 19, no. 1 (1985): 167–87. http://dx.doi.org/10.1017/s0251107x00006295.

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The last three years have witnessed a growing interest in the physical properties of the small bodies in the solar system. Perhaps the most significant impetus to research on small bodies has been the imminent arrival of Comet Halley in the inner solar system. This famous comet, which was recovered in autumn 1982, has been the object of intense study during the past year as it has approached the sun and developed a tail. Much of the international, ground-based astronomical research on Halley has been coordinated through the International Halley Watch program. Spacecraft from several nations ha
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Prasad, Debi. "The Interaction of Cometary Plasma with Interplanetary Medium - A Post-Halley View." Symposium - International Astronomical Union 142 (1990): 429–34. http://dx.doi.org/10.1017/s0074180900088355.

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The strong interaction of cometary plasma with the interplanetary medium results the disconnection events and other features observed in plasma tail and the coma of comets. The understanding of these features provide direct probe of the heliospheric magnetic field. However the interpretation of these events is not without ambiguity, as revealed in the recent work with comet Halley. In this paper a review of the “Post-Halley era” developments of the cometary plasma physics is presented.
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Dissertations / Theses on the topic "Comete halley"

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LE, BORGNE JEAN-FRANCOIS. "Polarimetrie des enveloppes d'objets astrophysiques evolues et de la comete halley." Toulouse 3, 1987. http://www.theses.fr/1987TOU30097.

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Utilisation d'un polarimetre photoelectrique monocanal, dans le domaine visible et uv, pour l'observation de l'enveloppe de poussieres de deux supergeantes rouges, des poussieres contenues dans 5 nebuleuses planetaires et des bandes moleculaires de fluorescence des cometes de halley et de hartley-good
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CHAIZY, PATRICK. "Etude de l'environnement ionique et plasma autour du noyau de la comete de halley." Toulouse 3, 1991. http://www.theses.fr/1991TOU30108.

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En mars 1986, la sonde spatiale europeenne giotto passait a 610 km du noyau de la comete de halley. Parmi les instruments scientifiques embarques figurait le spectrometre electrostatique d'electrons et d'ions negatifs rpa-1 eesa de l'experience rpa-copernic. L'analyse de son comportement, avant et pendant la rencontre, a permis de mettre en evidence plusieurs problemes, influencant la qualite des mesures, intrinseques au detecteur ou lies a l'interaction de ce dernier avec le milieu ambiant (du fait de la vitesse de propagation elevee de la sonde: 68,4 km/s). Ce detecteur a permis de reveler l
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Abergel, Alain. "Traitement et analyse des images transmises lors des survols de la comete de halley par les sondes vega." Paris 6, 1987. http://www.theses.fr/1987PA066226.

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Analyse et reduction des donnees ccd enregistrees par les sondes vega lors de la rencontre avec la comete de halley. Description des techniques de filtrage et de correction utilisees pour traiter les images fortement bruitees. Les images obtenues permettent de faire apparaitre les contours illumines par le soleil ainsi que la forme tridimensionnelle du noyau dont les dimensions sont: 16 x 8. 2 x 7. 5 km**(3). De nombreux jets de poussieres partant de la surface du noyau sont clairement mis en evidence
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Colom, Pierre. "Observations radio du radical oh dans la comete de halley : variations temporelles et anisotropie de la production gazeuse." Paris 7, 1989. http://www.theses.fr/1989PA077263.

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L'observation des cometes aux radiofrequences permet aussi bien d'etudier la cinematique que la quantite des gaz rejetes par leurs noyaux. Le suivi quotidien de la comete de halley pendant plus d'un an au radiotelescope de la station de nancay a permis d'analyser les variations a long et a court terme du taux de production des radicaux oh, traceurs de la molecule d'eau qui est la plus abondante dans une atmosphere cometaire. Il ressort clairement que le taux de production gazeuse etait plus eleve apres la perihelie qu'avant, a distance heliocentrique egale. De janvier a mai 1986, le taux de pr
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ROUSSELOT, PHILIPPE. "Analyse de spectres de la comete de halley obtenus le 9 mars 1986 par le spectromere tks : etude de la distribution de oh et modelisation du spectre d'emission de c2 en fonction du temps." Paris 6, 1993. http://www.theses.fr/1993PA066465.

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Les spectres de la coma interne de la comete de halley, obtenus le 9 mars 1986 lors de la rencontre de la sonde vega 2 avec halley, ont permis d'etudier la distribution du radical oh et le spectre de fluorescence du radical c2. Lorsqu'on tente de modeliser la distribution radiale du radical oh on peut mettre en evidence le role joue par l'epaisseur optique de la coma. Cette epaisseur optique a deux effets principaux se manifestant clairement avec les donnees obtenues : 1) un effet de saturation des raies d'emission de la bande (o,o) centree a 309 nm; 2) une diminution du taux de creation des r
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DiSanti, Michael Antonio. "The production and spatial distribution of neutral and ionized water vapor in comet P/Halley." Diss., The University of Arizona, 1989. http://hdl.handle.net/10150/184644.

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This study addressed the problem of water vapor production and distribution in comet P/Halley, based upon interpretation of observational data obtained during the recent 1985-86 apparition. The data was acquired using the Lunar and Planetary Laboratory charge-coupled device (CCD) on the 154-cm Catalina telescope of the University of Arizona Observatories. Our data acquisition system was employed in two modes. The long-slit (∼200") spectroscopy mode covered the wavelength range 5200-10400 Å at a spectral resolution ∼14 Å. The narrow band filter imaging mode allowed two-dimensional mapping of se
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Chakaveh, Sepideh. "Dust emission by comet P/Halley 1982i." Thesis, University of Kent, 1989. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.328204.

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Sekhar, A. "Evolution of Halley-type comets and meteoroid streams." Thesis, Queen's University Belfast, 2014. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.676720.

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The overall objective of the thesis is to understand the long term orbital dynamics of comets and meteoroid streams. The initial idea focused mainly on detailed analysis of Jovian resonances in Orionids and Leonids. Special emphasis was given to study their influences in causing meteoroutbursts and storms on Earth. The theoretical simulations matched with observational records to a very good degree. This work led to the curious question as to whether any resonance mechanism could be driven due to Saturn's gravity. Subsequent analysis showed that Saturn's influences can also become vital when t
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Evans, S. T. "Hypervelocity impact studies on the Giotto comet Halley mission." Thesis, University of Kent, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.233399.

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Pankiewicz, George S. "Dust environment modelling from encounters with comet P/Halley." Thesis, University of Kent, 1989. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.328097.

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Books on the topic "Comete halley"

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Littmann, Mark. Comet Halley: Once in a lifetime. American Chemical Society, 1985.

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Joseph, Pope. Next apparition of Halley's Comet. s.n., 1996.

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Burgos, Estrella. El Cometa Halley. SEP Cultura, 1985.

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Faria, Peter Leroy. Cometa de Halley. Editora UFMG/PROED, 1986.

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Zaratti, F. El cometa Halley. [s.n.], 1985.

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Brown, Peter Lancaster. Halley & his comet. Blanford Press, 1985.

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Greig, Brian. Halleys comet. Writers Press, 1985.

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Bailey, Mark E. Halley's Comet: An introduction to comets and the 1985/6 sighting of Comet Halley. The University of Manchester, 1985.

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Terence, Murtagh, ed. A comet called Halley. Cambridge University Press, 1985.

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Lancaster-Brown, Peter. Halley and his comet. Blandford Press, 1985.

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Book chapters on the topic "Comete halley"

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Encrenaz, Therese. "Comet Halley." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_327-3.

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Encrenaz, Therese. "Comet Halley." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_327.

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Encrenaz, Therese. "Comet Halley." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-11274-4_327.

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Visvanathan, N., Z. Meglick, and D. T. Wickramasinghe. "Spectropolarimetry of Comet Halley." In Origin and Evolution of Interplanetary Dust. Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-011-3640-2_51.

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Hadavi, Hadi. "Astrometry of Comet Halley." In Stargazers. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-74020-6_65.

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Greenberg, J. Mayo, and Aigen Li. "From Interstellar Dust to Comets: Distributed Co in Comet Halley." In Astrophysics and Space Science Library. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5252-5_14.

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Huntress, Wesley T., and Mikhail Ya Marov. "The International Comet Halley campaign." In Soviet Robots in the Solar System. Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-7898-1_18.

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Kikuchi, S., Y. Mikami, T. Mukai, S. Mukai, and J. H. Hough. "Polarimetry of comet P/Halley." In Exploration of Halley’s Comet. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-82971-0_122.

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Sivaraman, K. R., G. S. D. Babu, B. S. Shylaja, and R. Rajamohan. "Spectrophotometry of comet P/Halley." In Exploration of Halley’s Comet. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-82971-0_98.

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A’Hearn, Michael F. "Coordinated Programs for Comet Halley." In Instrumentation and Research Programmes for Small Telescopes. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-010-9433-7_38.

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Conference papers on the topic "Comete halley"

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Neugebauer, M. "Pickup ions observed at comet Halley." In Particle acceleration in cosmic plasmas. AIP, 1992. http://dx.doi.org/10.1063/1.42697.

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Fomenkova, Marina, and Sherwood Chang. "Carbon in comet Halley dust particles." In Analysis of interplanetary dust: NASA/LPI workshop. AIP, 1994. http://dx.doi.org/10.1063/1.46508.

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WYCKOFF, SUSAN. "Ground-based observations of Halley's Comet." In 25th AIAA Aerospace Sciences Meeting. American Institute of Aeronautics and Astronautics, 1987. http://dx.doi.org/10.2514/6.1987-630.

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HECHLER, F., T. MORLEY, and P. MAHR. "Properties of comet Halley derived from thermal models and astrometric data." In Astrodynamics Conference. American Institute of Aeronautics and Astronautics, 1986. http://dx.doi.org/10.2514/6.1986-2172.

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McKenna-Lawlor, Susan. "Particle acceleration above the pick-up energy at comet 1P/Halley." In PHYSICS OF THE HELIOSPHERE: A 10 YEAR RETROSPECTIVE: Proceedings of the 10th Annual International Astrophysics Conference. AIP, 2012. http://dx.doi.org/10.1063/1.4723608.

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Moreels, Guy, and Jacques Clairemidi. "Spectral Images Of The Inner Coma Of Comet Halley Taken From The VEGA 2 Interplanetary Spacecraft." In 1989 Intl Congress on Optical Science and Engineering, edited by Jacques F. Duvernoy. SPIE, 1989. http://dx.doi.org/10.1117/12.961653.

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Guineva, Veneta, Atanas Atanassov, and Stoyanka Staykova. "Creation of the CO+ spectrum for analysis of Halley's Comet spectrum." In 10th International School on Quantum Electronics: Lasers--Physics and Applications, edited by Peter A. Atanasov and Dimitar V. Stoyanov. SPIE, 1999. http://dx.doi.org/10.1117/12.347642.

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Rousselot, P., B. Goidet-Devel, J. Clairemidi, and G. Moreels. "Excitation mechanisms of the C2 Swam bands in Comet Halley’s spectrum." In The 50th international meeting of physical chemistry: Molecules and grains in space. AIP, 1994. http://dx.doi.org/10.1063/1.46603.

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Stoeva, Penka, Rolf Werner, Veneta Guineva, and Stoyanka Staykova. "Investigation of Halley's Comet dust size distribution by Vega-2 interplanetary station visual spectra analysis." In 10th International School on Quantum Electronics: Lasers--Physics and Applications, edited by Peter A. Atanasov and Dimitar V. Stoyanov. SPIE, 1999. http://dx.doi.org/10.1117/12.347641.

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Ferraro, Fabrizio, Enrico Sciubba, and Claudia Toro. "Integrated Study of a Minimum Exergy Destruction Building Conditioning System." In ASME 2013 International Mechanical Engineering Congress and Exposition. American Society of Mechanical Engineers, 2013. http://dx.doi.org/10.1115/imece2013-62672.

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The relatively low average conversion efficiency of air-conditioning systems and the recently imposed upper bounds to the final energy use in the heating and cooling of residential buildings suggest to consider new approaches to design less energy intensive systems. An integrated, exergy-based approach for the optimal matching of internal and external heating plants in building conditioning systems has been proposed — and its theoretical basis discussed — in a previous paper. The procedure allows the designer to obtain a pseudo-optimal integration of the building and its heating plant (heating
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