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Gotowa bibliografia na temat „Galilee tours”

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Data publikacji: 25 lipca 2024

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Artykuły w czasopismach na temat "Galilee tours"

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Lieske, J. H. "Galilean Satellites and the Galileo Space Mission". International Astronomical Union Colloquium 165 (1997): 13–20. http://dx.doi.org/10.1017/s0252921100046327.

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AbstractThe Galileo spacecraft arrived at Jupiter in December 1995 to start its two-year mission of exploring the Jovian system. The spacecraft will complete eleven orbits around Jupiter and have ten more close encounters with the outer three Galilean satellites, after the initial close approach to Io on December 7, 1995. Since the Io encounter occurred closer to Io than originally designed, the spacecraft energy change was greater than nominally planned and resulted in an initial spacecraft orbital period about 7 days less than that designed in the nominal tour. A 100-km change in the Io-encounter distance results in an 8-day change in initial period of the spacecraft. Hence the first Ganymede encounter was moved forward one week, and the aim points for the first two Ganymede encounters were altered, but all other encounters would occur on their nominal dates and at the nominal altitudes. This was accomplished without expending spacecraft fuel and resulted in the first Ganymede flyby occurring on June 27, 1996 rather than the nominally scheduled July 4.Earth- and spacecraft-based data were employed in developing ephemerides in support of the Galileo space mission. An analysis of CCD astrometric observations from 1992–1994, of photographic observations from 1967–1993, of mutual event astrometric data from 1973–1991, of Jovian eclipse timing data from 1652–1983, of Doppler data from 1987–1991, and of optical navigation data from the Voyager spacecraft encounter in 1979, produced the satellite ephemerides for the Galileo space mission.
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Schenk, Paul. "A virtual tour of the Galilean Satellites". Proceedings of the International Astronomical Union 6, S269 (styczeń 2010): 254–68. http://dx.doi.org/10.1017/s1743921310007519.

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Galileo's imagination was quick to comprehend the importance of the 4 starry objects he observed near Jupiter in January 1610, not only for himself as a scientist but for our common understanding of the place of the Earth and our species in the cosmos. Even he, however, could not have imagined what those four objects would actually look like once humans got their first good look. Some 369 years the fast traveling Voyager 1 and 2 spacecraft provided that first good look during 1979, followed by an even closer look from the Galileo Orbiter beginning in 1996 through 2001. The following mosaics represent some of the best of those views. They include views of impact craters young and ancient, icy terrains that have been intensely faulted, eroded or disrupted, mountains towering 10 or more kilometers high, and volcanic eruptions hotter than those on Earth. Each of the four Galilean satellites is geologically distinct, betraying very diverse global histories and evolutions. Images and other observations of these 4 objects revealed the importance of tidal heating and subsurface water oceans in planetary evolution, but mapping is very incomplete. New missions to explore these planetary bodies are being planned and the images and observations of the missions that went before will lay the groundwork for these new explorations as we begin the 5th Galilean century.
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Fabíola, P. Magalhães, Walter Gonzalez, Ezequiel Echer, Mariza P. Souza-Echer, Rosaly Lopes, Jeffrey P. Morgenthaler i Julie Rathbun. "Ground-based observations of the [SII] 6731 Å emission lines of the Io plasma torus". Proceedings of the International Astronomical Union 12, S328 (październik 2016): 227–29. http://dx.doi.org/10.1017/s1743921317003738.

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AbstractThe Io Plasma Torus (IPT) is a doughnut-shaped structure of charged particles, composed mainly of sulfur and oxygen ions. The main source of the IPT is the moon Io, the most volcanically active object in the Solar System. Io is the innermost of the Galilean moons of Jupiter, the main source of the magnetospheric plasma and responsible for injecting nearly 1 ton/s of ions into Jupiter's magnetosphere. In this work ground-based observations of the [SII] 6731 Å emission lines are observed, obtained at the MacMath-Pierce Solar Telescope. The results shown here were obtained in late 1997 and occurred shortly after a period of important eruptions observed by the Galileo mission (1996-2003). Several outbursts were observed and periods of intense volcanic activity are important to correlate with periods of brightness enhancements observed at the IPT. The time of response between an eruption and enhancement at IPT is still not well understood.
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C., R. "Galileo at Jupiter: The Goodbye Tour". Science News 161, nr 8 (23.02.2002): 125. http://dx.doi.org/10.2307/4013100.

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Palca, Joseph. "Space probes: Planetary tour for Galileo". Nature 323, nr 6085 (wrzesień 1986): 197. http://dx.doi.org/10.1038/323197a0.

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Esposito, L. W., C. A. Barth, A. R. Hendrix, C. W. Hord, A. I. F. Stewart, J. M. Ajello i R. A. West. "Galileo UVS Results and Cassini Preview". Highlights of Astronomy 11, nr 2 (1998): 1054–56. http://dx.doi.org/10.1017/s1539299600019584.

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AbstractUVS results from Jupiter show the Io torus colder and brighter than the Voyager observations. Aurora near Jupiter’s poles emit 1-4 MR from altitudes of 300 – 400 km. Ganymede and Callisto have extended hydrogen exospheres. The near-UV reflectance of the Galilean satellites shows SO2, magnetospheric alteration, and O3. Remote sensing of Jupiter’s stratospheric haze determines that it thickens and darkens towards higher latitudes.
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Kivelson, M. G., K. K. Khurana, R. J. Walker, J. Warnecke, C. T. Russell, J. A. Linker, D. J. Southwood i C. Polanskey. "Io's Interaction with the Plasma Torus: Galileo Magnetometer Report". Science 274, nr 5286 (18.10.1996): 396–98. http://dx.doi.org/10.1126/science.274.5286.396.

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Bagenal, F., F. J. Crary, A. I. F. Stewart, N. M. Schneider, D. A. Gurnett, W. S. Kurth, L. A. Frank i W. R. Paterson. "Galileo measurements of plasma density in the Io torus". Geophysical Research Letters 24, nr 17 (1.09.1997): 2119–22. http://dx.doi.org/10.1029/97gl01254.

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Nerney, Edward G., Fran Bagenal i Andrew J. Steffl. "Io plasma torus ion composition: Voyager, Galileo, and Cassini". Journal of Geophysical Research: Space Physics 122, nr 1 (styczeń 2017): 727–44. http://dx.doi.org/10.1002/2016ja023306.

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Thorne, R. M., T. P. Armstrong, S. Stone, D. J. Williams, R. W. McEntire, S. J. Bolton, D. A. Gurnett i M. G. Kivelson. "Galileo evidence for rapid interchange transport in the Io torus". Geophysical Research Letters 24, nr 17 (1.09.1997): 2131–34. http://dx.doi.org/10.1029/97gl01788.

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Rozprawy doktorskie na temat "Galilee tours"

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Williams, Ryan. "Galilean moon tour using simplified trajectory computational techniques". Diss., Columbia, Mo. : University of Missouri-Columbia, 2006. http://hdl.handle.net/10355/4563.

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Thesis (M.S.)--University of Missouri-Columbia, 2006.
The entire dissertation/thesis text is included in the research.pdf file; the official abstract appears in the short.pdf file (which also appears in the research.pdf); a non-technical general description, or public abstract, appears in the public.pdf file. Title from title screen of research.pdf file viewed on (February 23, 2007) Includes bibliographical references.
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Książki na temat "Galilee tours"

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H, Aichele Jean, i Jet Propulsion Laboratory (U.S.), red. Galileo: The tour guide (and a summary of the mission to date). [Pasadena, Calif.]: Jet Propulsion Laboratory, California Institute of Technology, 1996.

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Moi, Galilée: Mathématicien et philosophe florentin, qui contre tous osa regarder le ciel en sa vérité. Tournai: Casterman, 1989.

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Ecole pratique des hautes études, red. La Galicie au temps des Habsbourg: 1772-1918. Histoire, société, cultures en contact. [Actes du colloque international organisé en janvier 2009 à Tours, université François-Rabelais, et à Paris, école pratique des hautes études]. Tours: Presses universitaires François-Rabelais, 2010.

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RENDEZ-VOUS EN GALILÉE - Journal de voyage à vélo - Tours-Galilée. Paris: Editions L'Harmattan, 2012.

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Crawford, Matthew r. Rejection at Nazareth in the Gospels of Mark, Matthew, Luke—and Tatian. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198814801.003.0006.

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While Jesus’ rejection in his hometown is common to all three synoptic accounts, the placement of this episode differs. Mark and Matthew narrate his rejection at the synagogue of Nazareth only after a period of successful ministry elsewhere. Luke collapses the Markan timeline by relocating the scene in the synagogue in Nazareth to the initial preaching tour through Galilee, and he also recounts an unsuccessful attempt to cast Jesus from the cliff outside the town. This trajectory of rewriting can be extended to include the Diatessaron of Tatian, where the first half of the Lukan pericope is left in the preaching tour through Galilee, while the second half is postponed until later in the narrative. In his redaction of prior sources, Tatian’s editorial work is comparable to that of Matthew and Luke. His work was regarded by its primary users as the Gospel, and not just as a ‘gospel harmony’.
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Galileo Positioning Technology. Springer, 2012.

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Casati, Roberto. La Découverte de l'ombre : De Platon à Galilée, une énigme qui a fasciné tous les grands penseurs de l'humanité. Albin Michel, 2002.

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Części książek na temat "Galilee tours"

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Thomas, N. "The IO Plasma Torus". W The Three Galileos: The Man, the Spacecraft, the Telescope, 225–38. Dordrecht: Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-015-8790-7_18.

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Mee, Nicholas. "Diamonds in the Sky!" W The Cosmic Mystery Tour, 101–9. Oxford University Press, 2019. http://dx.doi.org/10.1093/oso/9780198831860.003.0013.

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After consuming their nuclear fuel, most stars lose their outer envelopes and all that remains is the collapsed core of the star, an object known as a white dwarf. Ever since Galileo pointed a telescope at the night sky, each advance in telescope making has resulted in sensational discoveries. Alvan Clark & Sons ground some of the biggest telescope lenses ever made. Alvan Graham Clark discovered Sirius B while testing one of these lenses. Eddington deduced that Sirius B has a size similar to that of the Earth, but with the mass of the Sun, and was an example of a new class of stars—white dwarfs. The easiest white dwarf to see with a telescope orbits the star Keid. In Star Trek, the planet Vulcan orbits the star Keid A.
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"Classical Physics in Galilean and Minkowski Spacetimes". W A Unified Grand Tour of Theoretical Physics, 65–116. CRC Press, 2012. http://dx.doi.org/10.1201/b12906-8.

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"Classical Physics in Galilean and Minkowski Spacetimes". W A Unified Grand Tour of Theoretical Physics, 2nd edition, 61–98. Taylor & Francis, 2015. http://dx.doi.org/10.1201/noe0750306041-7.

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"Classical Physics in Galilean and Minkowski Spacetimes". W A Unified Grand Tour of Theoretical Physics, 2nd edition. Taylor & Francis, 2001. http://dx.doi.org/10.1201/noe0750306041.ch3.

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Streszczenia konferencji na temat "Galilee tours"

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MURROW, D., i R. JACOBSON. "Galilean satellite ephemeris improvement using Galileo tour encounter information". W Astrodynamics Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1988. http://dx.doi.org/10.2514/6.1988-4249.

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MOULTRIE, B., P. KENYON, J. KECHICHIAN, R. DAVIS i F. NICHOLSON. "Galilean satellite tour orbit determination assessment". W 25th AIAA Aerospace Sciences Meeting. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1987. http://dx.doi.org/10.2514/6.1987-95.

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LONGUSKI, J., i A. WOLF. "The Galileo orbital tour for the 1986 launch opportunity". W Astrodynamics Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1986. http://dx.doi.org/10.2514/6.1986-2006.

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Izzo, Dario, Luís F. Simões, Marcus Märtens, Guido C. H. E. de Croon, Aurelie Heritier i Chit Hong Yam. "Search for a grand tour of the jupiter galilean moons". W Proceeding of the fifteenth annual conference. New York, New York, USA: ACM Press, 2013. http://dx.doi.org/10.1145/2463372.2463524.

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Elsner, R. F., B. D. Ramsey, D. A. Swartz, J. A. Gaskin, P. Rehak, J. H. WaiteJr., J. F. Cooper i R. E. Johnson. "X-ray probes of Jupiter's auroral zones, Galilean moons, and the Io plasma torus". W Optics & Photonics 2005, redaktorzy Richard B. Hoover, Gilbert V. Levin, Alexei Y. Rozanov i G. Randall Gladstone. SPIE, 2005. http://dx.doi.org/10.1117/12.613655.

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