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Academic literature on the topic 'Ganymedes'

Author: Grafiati

Published: 4 June 2021

Last updated: 17 February 2022

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Journal articles on the topic "Ganymedes"

1

Eden, P. T. "Two Notes on Euripides." Classical Quarterly 38, no. 2 (December 1988): 560–61. http://dx.doi.org/10.1017/s0009838800037204.

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Students of the Orestes are fortunate to have two excellent commentaries at their disposal, by C. W. Willink (Oxford, 1986) and M. L. West (Warminster, 1987). Neither will help them to understand this line, which is ‘the only allusion to Ganymede's horsemanship’ (Willink ad loc), because ‘no story of riding by Ganymede is known’ (West ad loc). But we are repeatedly reminded that the scene with the Phrygian (1369ff.) has far fewer affinities with tragedy than with comedy, and εύριπιδαριστοφαíζεται Comedy provides the clue, specifically at Ar. Vesp. 50If. and Lys. 676ff. The reference is to the variety of equestrianism for which Ganymede is far from unknown (he was too young to have established an association with any other kind). For Innoavvr) here describes a σχῆμα ἐρωτικóν and the line means Ganymedes concubinus, Iovis supini inguini insidens et equitans, sc. inter causas fuit malorum propter Iunonis invidiam Troianis immissorum.

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Stevens, J. Timothy. "Ganymedes, Persephone, and Mei: The Child as Object of Desire." Dutch Crossing 13, no. 38 (August 1989): 96–109. http://dx.doi.org/10.1080/03096564.1989.11783916.

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Прокофьев, А. М. "Новый полорыл Coelorinchus ganymedes sp. nova из вод Полинезии (Macrouridae)." Вопросы ихтиологии 61, no. 2 (2021): 127–33. http://dx.doi.org/10.31857/s0042875221020193.

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Chaudhary, Zahid. "Controlling the Ganymedes: The colonial gaze in J. R. Ackerley'sHindoo holiday." South Asia: Journal of South Asian Studies 24, sup001 (January 2001): 47–57. http://dx.doi.org/10.1080/00856400108723435.

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Folgar Brea, María José. "Cuando Apolo mató a Ganymedes. El “texte .liij.” de la Epistre Othea." Medievalia 53, no. 1 (May 19, 2021): 5–23. http://dx.doi.org/10.19130/medievalia.2021.53.1.25621.

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Christine de Pizan's Epistre Othea aims to show a variety of models about what does it mean to be a perfect knight. In her book she bases on several sources, among which the Ovide moralisé is one of the most important. Thus, it´s surprising that one of the used exempla conspicuously departs from the content of this work (and others that she knew) by introducing an episode in which Apollo kills Ganymede, not only in the text itself but also in the iconographic program that accompanies it in the manuscripts. This article tries to draw attention to this unique feature in order to seek some possible explanation.

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Prokofiev, A. M. "New grenadier Coelorinchus ganymedes sp. nova from the Waters of Polynesia (Macrouridae)." Journal of Ichthyology 61, no. 2 (March 2021): 175–81. http://dx.doi.org/10.1134/s0032945221020156.

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Jara-Orué, H. M., and B. L. A. Vermeersen. "Tides on Jupiter's moon Ganymede and their relation to its internal structure." Netherlands Journal of Geosciences - Geologie en Mijnbouw 95, no. 2 (March 16, 2016): 191–201. http://dx.doi.org/10.1017/njg.2015.23.

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AbstractOne of the major scientific objectives of ESA's JUICE (JUpiter ICy moons Explorer) mission, which is scheduled for launch in 2022 and planned to arrive at the Jovian system in 2030, is to characterise the internal water ocean and overlying ice shell of Jupiter's largest moon Ganymede. As part of the strategy developed to realise this objective, the tidal response of Ganymede's interior will be constrained by JUICE's measurements of surface displacements (by the Ganymede Laser Altimeter (GALA) instrument) and variations in the gravitational potential (by the 3GM radio science package) due to the acting diurnal tides. Here we calculate the tidal response at the surface of Ganymede for several plausible internal configurations in order to analyse the relation between the tidal response and the geophysical parameters that characterise Ganymede's interior. Similarly to the case of Jupiter's smallest icy satellite Europa, the tidal response of Ganymede in the presence of a subsurface ocean, which could be as large as about 3.5 m in terms of the induced radial deformation, mostly depends on the structural (thickness, density) and rheological (rigidity, viscosity) properties of the ice-I shell. Nevertheless, the dependence of the tidal response on several geophysical parameters of the interior, in particular on the thickness and rigidity of the ice-I shell, does not allow for the unambiguous determination of the shell thickness from tidal measurements alone. Additional constraints could be provided by the measurement of forced longitudinal librations at the surface, as their amplitude is more sensitive to the rigidity than to the thickness of the shell.

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Lehmer, Owen R., David C. Catling, and Kevin J. Zahnle. "The Longevity of Water Ice on Ganymedes and Europas around Migrated Giant Planets." Astrophysical Journal 839, no. 1 (April 11, 2017): 32. http://dx.doi.org/10.3847/1538-4357/aa67ea.

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Downey, Brynna G., Francis Nimmo, and Isamu Matsuyama. "Inclination damping on Callisto." Monthly Notices of the Royal Astronomical Society 499, no. 1 (September 14, 2020): 40–51. http://dx.doi.org/10.1093/mnras/staa2802.

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ABSTRACT Callisto is thought to possess a subsurface ocean, which will dissipate energy due to obliquity tides. This dissipation should have damped any primordial inclination within 1 Gyr – and yet Callisto retains a present-day inclination. We argue that Callisto’s inclination and eccentricity were both excited in the relatively recent past (∼0.3 Gyr). This excitation occurred as Callisto migrated outwards according to the ‘resonance-locking’ model and passed through a 2:1 mean-motion resonance with Ganymede. Ganymede’s orbital elements were likewise excited by the same event. To explain the present-day orbital elements, we deduce a solid-body tidal k2/Q ≈ 0.05 for Callisto and a significantly lower value for Ganymede.

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Steinbrügge, Gregor, Teresa Steinke, Robin Thor, Alexander Stark, and Hauke Hussmann. "Measuring Ganymede’s Librations with Laser Altimetry." Geosciences 9, no. 7 (July 20, 2019): 320. http://dx.doi.org/10.3390/geosciences9070320.

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Jupiter’s moon Ganymede might be in possession of a subsurface ocean located between two ice layers. However, from Galileo data it is not possible to unambiguously infer the thickness and densities of the individual layers. The upcoming icy satellite mission JUICE (JUpiter ICy moons Explorer) will have the possibility to perform more detailed investigations of Ganymede’s interior structure with the radio science experiment 3GM and the GAnymede Laser Altimeter (GALA). Here we investigate the possibility to derive the rotational state of the outer ice shell by using topography measured by laser altimetry. We discuss two different methods to invert synthetic laser altimetry data. Method 1 is based on a spherical harmonics expansion and Method 2 solves for B-splines on a rectangular grid. While Method 1 has significant limitations due to the omission of high degrees of the global expansion, Method 2 leads to stable results allowing for an estimate of the in-orbit measurement accuracy. We estimate that GALA can measure the amplitude of Ganymede’s librations with an accuracy of 2.5–6.6 μ rad (6.6–17.4 m at the equator). This allows for determining the thickness of an elastic ice shell, if decoupled from the deeper interior by a subsurface ocean, to about an accuracy of 24–65 km.

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Dissertations / Theses on the topic "Ganymedes"

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Paty, Carol S. "Ganymede's magnetosphere : unraveling the Ganymede-Jupiter interaction through combining multi-fluid simulations and observations /." Thesis, Connect to this title online; UW restricted, 2006. http://hdl.handle.net/1773/6811.

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Kruszynski, Anette. "Der Ganymed-Mythos in Emblematik und mythographischer Literatur des 16. Jahrhunderts /." Worms : Werner, 1985. http://catalogue.bnf.fr/ark:/12148/cb348977583.

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Deliberal, Sonia Maria. "O (des)enlace do interdiscurso, da cenografia e do ethos entre Meu nome é esperança! e Corações de pedra, de Ganymédes José." Pontifícia Universidade Católica de São Paulo, 2019. https://tede2.pucsp.br/handle/handle/22002.

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Submitted by Filipe dos Santos (fsantos@pucsp.br) on 2019-03-19T12:31:27Z No. of bitstreams: 1 Sonia Maria Deliberal.pdf: 1347369 bytes, checksum: dffbd37164ae509aac981fb397cfb45c (MD5)
Made available in DSpace on 2019-03-19T12:31:27Z (GMT). No. of bitstreams: 1 Sonia Maria Deliberal.pdf: 1347369 bytes, checksum: dffbd37164ae509aac981fb397cfb45c (MD5) Previous issue date: 2019-02-22
The present dissertation is located in the line of research entitled "Text and Discourse in Oral and Written Modalities", part of the Program of Postgraduate Studies in Portuguese Language, Pontifical Catholic University of São Paulo - PUC / SP. The central theme of this research is to analyze, from the perspective of the Discourse Analysis (AD) of the French line, the exclusion between two novels of Ganymédes José, namely: My Name is Hope!, 1974, and Hearts of Stone, The aim is to approach literature as a producer of discourse that is constituted in - and by - language; thus, it is necessary to observe the socio-historical conditions, in order to situate the discourses contemplated for analysis. The selected theme is justified by the observations made during the student environment, during a course in Basic Education, in contact with deaf students, at which time it was possible to verify the presence of exclusion. The research problem raised was to verify the way in which the writer positioned himself and constituted his discourses in the different contexts before the exclusions. Based on studies carried out by Maingueneau, the present investigation aims at the observation: of the role of interdiscourse in the consideration of the effects of sense and in the interweaving of different universes; of scenography, with the development of the enunciation constituted between the enunciator, co-enunciator, involving the topography and the chronography; and of ethos in the construction of the image of the enunciator accomplished by the co-enunciator and its process of incorporation. This study reveals the importance of theoretical and methodological procedures to favor the knowledge of discourse
A presente dissertação situa-se na linha de pesquisa intitulada “Texto e Discurso nas Modalidades Oral e Escrita”, integrante do Programa de Estudos Pós-Graduados em Língua Portuguesa, da Pontifícia Universidade Católica de São Paulo – PUC/SP. O tema central desta pesquisa é analisar, sob a perspectiva da Análise do Discurso (AD) de linha francesa, a exclusão entre dois romances de Ganymédes José, quais sejam: Meu Nome é Esperança!, do ano de 1974, e Corações de Pedra, de 1984. O intuito é abordar a literatura como produtora de discurso que se constitui na – e pela – linguagem; assim sendo, faz-se necessário observar as condições sócio-históricas, a fim de situar os discursos contemplados para análise. O tema selecionado se justifica a partir das observações realizadas no meio estudantil, durante percurso na Educação Básica, em contato com alunos surdos, ocasião em que foi possível constatar, ainda, a presença da exclusão. O problema de pesquisa levantado foi o de verificar o modo como o escritor se posicionou e constituiu seus discursos nos diferentes contextos frente às exclusões. Partindo de estudos realizados por Maingueneau, a presente investigação visa à observação: do papel do interdiscurso na consideração dos efeitos de sentido e no entrelaçamento de diferentes universos; da cenografia, com o desenvolvimento da enunciação constituída entre o enunciador, co-enunciador, envolvendo a topografia e a cronografia; e do ethos na construção da imagem do enunciador realizada pelo co-enunciador e seu processo de incorporação. Esse estudo revela a importância dos procedimentos teóricos e metodológicos em favorecer o conhecimento do discurso

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Jia, Xianzhe. "Ganymede's magnetosphere observations and modeling /." Diss., Restricted to subscribing institutions, 2009. http://proquest.umi.com/pqdweb?did=1925733131&sid=9&Fmt=2&clientId=1564&RQT=309&VName=PQD.

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Teeling, Michael J. "Geology of Galileo Regio quadrangle, Ganymede." Kansas State University, 1987. http://hdl.handle.net/2097/18557.

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Ahlberg, Carl Daniel, and Wera Mauritz. "Modeling Far Ultraviolet Auroral Ovals at Ganymede." Thesis, KTH, Skolan för elektroteknik och datavetenskap (EECS), 2018. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-239382.

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Ganymede, one of Jupiters moons, differs from other moons in the Solar System as it has its own magnetic field. This rare property shapes the morphology on the existing far ultraviolet oxygen auroral ovals on the celestial body in the northern and southern hemisphere created by high energy electrons colliding into the atmosphere.With the help of the Hubble Space Telescope (HST) this phenomenon has been captured and analyzed multiple times during the past 20 years using the on-board Space Telescope Imaging Spectrograph (STIS). The ultimate goal of this project is recreating the far ultraviolet oxygen auroral emissions on Ganymede as a 3D computer model in MATLAB by using the data recovered from HST.The method used to reach this goal was to implement a model with main characteristics of the auroral ovals, project it onto a plane and then use a Cauchy distribution to filter the model. To compare the model with images from HST, a χ2-value was calculated for every pixel in each image. To further improvethe model the Nelder-Mead Simplex optimization method was applied.The project succeeded in such a way that the final model created views of the locations and the appearance of the bright spots that represent the auroral ovals around Ganymede with an accurate result in relation to the given data.

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Payan, Alexia Paule Marie-Renee. "Uncovering local magnetospheric processes governing the morphology and periodicity of Ganymede’s aurora using three-dimensional multifluid simulations of Ganymede’s magnetosphere." Thesis, Georgia Institute of Technology, 2013. http://hdl.handle.net/1853/51756.

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The electrodynamic interaction of Ganymede’s mini-magnetosphere with Jupiter’s corotating magnetospheric plasma has been shown to give rise to strong current systems closing through the moon and its ionosphere as well as through its magnetopause and magnetotail current sheet. This interaction is strongly evidenced by the presence of aurorae at Ganymede and of a bright Ganymede footprint on Jupiter’s ionosphere. This footprint is located equatorward of the main auroral emissions, at the magnetic longitude of the field line threading Ganymede. The brightness of Ganymede’s auroral footprint at Jupiter along with its latitudinal position have been shown to depend on the position of Ganymede relative to the center of the Jovian plasma sheet. Additionally, observations using the Hubble Space Telescope showed that Ganymede’s auroral footprint brightness is characterized by variations of three different timescales: 5 hours, 10-40 minutes, and ~100 seconds. The goal of the present study is to examine the relationship between the longest and the shortest timescale periodicities of Ganymede’s auroral footprint brightness and the local processes occurring at Ganymede. This is done by coupling a specifically developed brightness model to a three-dimensional multifluid model which tracks the energies and fluxes of the various sources of charged particles that precipitate into Ganymede’s ionosphere to generate the aurora. It is shown that the predicted auroral brightnesses and morphologies agree well with observations of Ganymede’s aurora from the Hubble Space Telescope. Our results also suggest the presence of short- and long-period variabilities in the auroral emissions at Ganymede due to magnetic reconnections on the magnetopause and in the magnetotail, and support the hypothesis of a correlation between the variability of Ganymede’s auroral footprint on Jupiter’s ionosphere and the variability in the brightness and morphology of the aurora at Ganymede. Finally, the modeled aurora at Ganymede reveals that the periodicities in the morphology and brightness of the auroral emissions are produced by two different dynamic reconnection mechanisms. The Jovian flow facing side aurora is generated by electrons sourced in the Jovian plasma and penetrating into Ganymede’s ionosphere through the cusps above the separatrix region. In this case, the reconnection processes responsible for the auroral emissions occur on Ganymede’s magnetopause between the Jovian magnetic field lines and the open magnetic field lines threading Ganymede’s Polar Regions. As for the magnetotail side aurora, it is generated by electrons originating from Ganymede’s magnetospheric flow. These electrons are accelerated along closed magnetic field lines created by magnetic reconnection in Ganymede’s magnetotail, and precipitate into Ganymede’s ionosphere at much lower latitudes, below the separatrix region.

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Alday, Parejo Juan. "Ganymede's hydrogen corona and FUV albedo from HST/STIS images." Thesis, KTH, Rymd- och plasmafysik, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-223964.

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Ganymedes är största månen i vårt Solsystem, och är ett föremål för intensiv vetenskaplig forskning under senaste decenier. Sedan 1998, STIS (Space Telescope Imaging Spectrograph) instrumentet ombord rymdteleskopet Hubble (HST) har observerat Ganymedes i UV ljus med våglängder mellan 1150 Å och 1730 Å i fem olika omgångar. Bilder av månen har tagits när Ganymedes var i olika positioner i sin bana. Detta gör det möjligt att jämföra båda hemisfärer av månen, och att undersöka eventuell tidsvariation. I denna rapport HST/STIS observationer av Ganymedes analyseras med målsättningen att undersöka månens exosfär bestående av atomär syre samt månens albedo i FUV våglänger. Väteexosfären, också kallad korona, förväntas sprida Lyman- ljuset vid 1216 Å, som kan observeras av STIS. Observationer i denna våglängd analyseras och en modell är framtagen för olika källor som bidrar vid denna våglängd. En uppskattning görs också av en eventuell absorption av Ganymedes emissioner i Jordens övre atmosfär, som kan uppgå till 85%. Jämförelse av modellen med bilder från HST/STIS tyder på att Ganymedes har en väteexosfär med ytdensiteten av (2-8) 103 cm􀀀3. Under Hubble kampanj 13328 har däremot betydligt lägre antal väteatomer detekterats, som kan bero på skillnader i magnetosfäriska omgivningen av månen jämfört med tidigare observationer. FUV albedo av månens yta har undersökts genom jämförelser av reflektansen vid olika våglängder, inklusive eventuella skillnader mellan olika hemisfärer. Vi finner att bakre (i förhållande till rörelsen i banan, som månen är låst i) hemisfären är ljusare än främre hemisfären för < 1600 Å. För längre våglängder, > 2000 Å, har motsatta resultat rapporterats tidigare, där främre hemisfären var ljusare. Detta tyder på att Ganymedes ytreflektans har en spektral inversion mellan 1600-2000 Å. Vi noterar även att ytreflektansen ökar med kortare våglängd för < 1400 Å, som kan bero på att ytans växelverkan med rymdpartiklar.
Ganymede, the largest moon in our Solar System, has been a target for intensive scientific research during the past decades. Since 1998, the Space Telescope Imaging Spectrograph (STIS) onboard of the Hubble Space Telescope (HST) has observed it in five different HST campaigns, operating in a wavelength range between 1150-1730 Å. The images were obtained when Ganymede was located at different orbital phase, providing information about both the trailing and leading hemispheres, and allowing for the search of potential hemispherical and time variability. Here, we analyze Ganymede’s HST/STIS observations in the search for a hydrogen exosphere and the study of the far-ultraviolet (FUV) albedo at different wavelengths. The hydrogen corona is expected to scatter sunlight at the Lyman- wavelength (1216 Å), which is within STIS’ spectral range. We analyze the observations at this particular wavelength, and derive models for the different sources of emission that are expected to contribute to the signal. We also estimate the potential extinction of Ganymede’s coronal emissions in the Earth’s upper atmosphere, which can be up to 85%. The comparison between the HST/STIS images and the model allows us to detect the hydrogen exosphere, which we estimate to be in a range of approximately (2-8) 103 cm􀀀3. The atomic hydrogen abundance in Ganymede’s atmosphere during HST campaign 13328 appears to be significantly lower, which could be related to differences in the plasma magnetospheric environment. We study Ganymede’s FUV albedo comparing the reflectance at different wavelengths, and potential difference between leading and trailing hemispheres. We find out that the trailing hemisphere is brighter than the leading side for < 1600 Å. This dichotomy is opposite to the previous results reported for > 2000 Å, where the leading hemisphere is actually brighter. Hence, there is a spectral inversion of Ganymede’s surface reflectivity at some wavelength in the range 1600-2000 Å. We also find out that the reflectivity of the surface increases for < 1400 Å, which might be related to space weathering processes on the surface.

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Bland, Michael T. "The Tectonic, Thermal and Magnetic Evolution of Icy Satellites." Diss., The University of Arizona, 2008. http://hdl.handle.net/10150/194804.

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Focusing on Ganymede and Enceladus, this work addresses a number of issues regarding icy satellite evolution, including the ultimate cause of Ganymede's tectonic and cryovolcanic resurfacing, the production of Ganymede's magnetic field, the formation of Ganymede's grooved terrain, and the tectonic and thermal evolution of Enceladus.Both Ganymede's resurfacing and the production of its magnetic field may be attributable to the Galilean satellites' passage through a Laplace-like resonance that excited Ganymede's orbital eccentricity. I examine how resonance passage effects Ganymede's thermal evolution using a coupled orbital-thermal model. Dissipation of tidal energy in Ganymede's ice shell permits high heat fluxes in its past, consistent with the formation of the grooved terrain; however, it also leads to the formation of a thin ice shell, which would have significant consequences for Ganymede's geologic history. In contrast, negligible tidal dissipation occurs in Ganymede's silicate mantle. Thus, passage through a Laplace-like resonance cannot reinvigorate Ganymede's metallic core or enable present-day magnetic field generation.Ganymede's thermal evolution has driven tectonic deformation on its surface, producing numerous swaths of ridges and troughs termed ``grooved terrain.'' Grooved terrain likely formed via unstable extension of Ganymede's lithosphere, but questions regarding instability growth at large strains remain unanswered. To address these questions, I use the finite-element model TEKTON to simulation the extension of an icy lithosphere to examine instability growth at finite strains. My results indicate that large-amplitude deformation requires lower thermal gradients than have been suggested by analytical models; however, the maximum deformation amplitudes produced by our numerical models are lower than typical observed groove amplitudes.Finally, I apply our finite-element modeling to the formation of ridges and troughs on Enceladus. Comparison between our models and photoclinometry profiles of Enceladus' topography indicate that the heat flux was high at the time of ridge and trough formation. Thus, the tectonic resurfacing and high heat fluxes currently observed at Enceladus' south pole may be only the latest episode in a long history of localized resurfacing and global reorientation.

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Peters, Friedrich Ernst. "Sächsische Ubiquität." Universität Potsdam, 2012. http://opus.kobv.de/ubp/volltexte/2012/5799/.

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Books on the topic "Ganymedes"

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Priest, Cherie. Ganymede. New York: Tor Books, 2011.

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Ganymede in the Renaissance: Homosexuality in art and society. New Haven: Yale University Press, 1986.

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Sheffield, Charles. The Ganymede Club. New York: Tom Doherty Associates, 1996.

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Ibrahim, Yosip. I visited Ganymede. Miami, FL, U.S.A: American Institute of Interplanetary Relations, 1996.

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Sheffield, Charles. The Ganymede Club. New York: TOR, 1995.

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Stealing Ganymede: A novel. Hulls Cove, ME: Rebel Satori Press, 2008.

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Walker, Constance. Lost roses of Ganymede House. New York, NY: Kensington Pub. Corp., 1989.

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Denton, Bradley. Buddy Holly is alive and well on Ganymede. New York: Morrow, 1991.

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Denton, Bradley. Buddy Holly is alive and well on Ganymede. New York: Avon Books, 1991.

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Denton, Bradley. Buddy Holly is alive and well on Ganymede. New York: Avon Books, 1992.

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Book chapters on the topic "Ganymedes"

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Henin, Bernard. "Ganymede." In Exploring the Ocean Worlds of Our Solar System, 79–96. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-93476-1_4.

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Encrenaz, Therese. "Ganymede." In Encyclopedia of Astrobiology, 920–21. Berlin, Heidelberg: Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_619.

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Encrenaz, Therese. "Ganymede." In Encyclopedia of Astrobiology, 1–2. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_619-2.

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Encrenaz, Therese. "Ganymede." In Encyclopedia of Astrobiology, 630–31. Berlin, Heidelberg: Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-11274-4_619.

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Hargitai, Henrik. "Groove (Ganymede)." In Encyclopedia of Planetary Landforms, 1–9. New York, NY: Springer New York, 2014. http://dx.doi.org/10.1007/978-1-4614-9213-9_181-1.

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Hargitai, Henrik. "Groove (Ganymede)." In Encyclopedia of Planetary Landforms, 884–91. New York, NY: Springer New York, 2015. http://dx.doi.org/10.1007/978-1-4614-3134-3_181.

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Bruyn, J., B. Haak, S. H. Levie, P. J. J. Van Thiel, and E. Van De Wetering. "The rape of Ganymede." In A Corpus of Rembrandt Paintings, 161–67. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0811-6_14.

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Keilson-Lauritz, Marita. "Ganymed trifft Tadzio." In Ikonen des Begehrens, 23–39. Stuttgart: J.B. Metzler, 1997. http://dx.doi.org/10.1007/978-3-476-04268-2_2.

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Forni, O. P., P. G. Thomas, and P. L. Masson. "Importance of the Tectonic Motions on Ganymede." In Ices in the Solar System, 759–66. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5418-2_51.

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Bianchi, R., and R. Casacchia. "Some Remarks on the Geology of Ganymede." In Ices in the Solar System, 767–79. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5418-2_52.

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Conference papers on the topic "Ganymedes"

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Aboudan, Alessio, Giacomo Colombatti, Stefano Debei, and Pasquale Palumbo. "Analysis of Ganymede rotational state using JANUS telescope." In 2019 IEEE 5th International Workshop on Metrology for AeroSpace (MetroAeroSpace). IEEE, 2019. http://dx.doi.org/10.1109/metroaerospace.2019.8869654.

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"Radio emission from satellite-Jupiter interactions (especially Ganymede)." In Planetary Radio Emissions VIII. Vienna: Austrian Academy of Sciences Press, 2018. http://dx.doi.org/10.1553/pre8s45.

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Sbalchiero, Elisa, Sanchari Thakur, and Lorenzo Bruzzone. "3D radar sounder simulations of geological targets on Ganymede Jovian Moon." In Image and Signal Processing for Remote Sensing XXV, edited by Lorenzo Bruzzone, Francesca Bovolo, and Jon Atli Benediktsson. SPIE, 2019. http://dx.doi.org/10.1117/12.2533066.

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Benton, Mark. "Crew Exploration Lander for Ganymede, Callisto, and Earth's Moon: Vehicle System Design." In 45th AIAA/ASME/SAE/ASEE Joint Propulsion Conference & Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2009. http://dx.doi.org/10.2514/6.2009-5179.

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Cameron, Marissa E., Bridget R. Smith-Konter, Liliane Burkhard, D. Alex Patthoff, Robert T. Pappalardo, and Geoffrey C. Collins. "STRIKE-SLIP TECTONISM ON GANYMEDE: INVESTIGATING COULOMB FAILURE AT A GLOBAL SCALE." In GSA Annual Meeting in Seattle, Washington, USA - 2017. Geological Society of America, 2017. http://dx.doi.org/10.1130/abs/2017am-303482.

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Benton, Mark. "Conceptual Design of Crew Lander for Exploration of the Moon, Ganymede, and Callisto." In 47th AIAA Aerospace Sciences Meeting including The New Horizons Forum and Aerospace Exposition. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2009. http://dx.doi.org/10.2514/6.2009-656.

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Lynam, Alfred, and Alan Didion. "Impulsive Trajectories from Earth to Callisto-Io-Ganymede Triple Flyby Capture at Jupiter." In AIAA/AAS Astrodynamics Specialist Conference. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2014. http://dx.doi.org/10.2514/6.2014-4106.

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Franqui, Aline, Spencer T. Seufert, Matheus Cosenza, and Masataka Okutsu. "Impactor Missions to Europa and Ganymede: Seismic Approach for Estimating Icy Crust Thickness." In 54th AIAA Aerospace Sciences Meeting. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2016. http://dx.doi.org/10.2514/6.2016-0220.

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Jones, Brandon, Marissa F. Vogt, Michael Chaffin, Mathieu Choukroun, Negar Ehsan, Luke Gibbons, Kennda Lynch, et al. "Concept for a new frontiers mission to Ganymede: A Planetary Science Summer School study." In 2011 IEEE Aerospace Conference. IEEE, 2011. http://dx.doi.org/10.1109/aero.2011.5747290.

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Atwell, William, Lawrence W. Townsend, Thomas Miller, and Christina Campbell. "Depth Dose Exposures in the Magnetosphere of Jupiter at the Icy Moons: Callisto, Ganymede, and Europa." In International Conference On Environmental Systems. 400 Commonwealth Drive, Warrendale, PA, United States: SAE International, 2004. http://dx.doi.org/10.4271/2004-01-2326.

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Reports on the topic "Ganymedes"

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Shaded relief and surface markings of the Osiris Quadrangle of Ganymede; air brush base for the Osiris Quadrangle of Ganymede. US Geological Survey, 1987. http://dx.doi.org/10.3133/i1769.

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Geologic map of the Uruk Sulcus Quadrangle of Ganymede. US Geological Survey, 1988. http://dx.doi.org/10.3133/i1934.

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Geologic map of the Philus Sulcus Quadrangle of Ganymede. US Geological Survey, 1989. http://dx.doi.org/10.3133/i1966.

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Controlled color photomosaic map of Ganymede Jg 15M CMNK. US Geological Survey, 2003. http://dx.doi.org/10.3133/i2762.

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Geologic map of the Etana region (Jg-1) of Ganymede. US Geological Survey, 1995. http://dx.doi.org/10.3133/i2497.

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Geologic map of the Hathor region (Jg-15) of Ganymede. US Geological Survey, 1994. http://dx.doi.org/10.3133/i2388.

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Shaded relief and surface markings of the Namtar Quadrangle; Ganymede. US Geological Survey, 1988. http://dx.doi.org/10.3133/i1871.

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Geologic map of the Galileo Regio Quadrangle (Jg-3) of Ganymede. US Geological Survey, 1997. http://dx.doi.org/10.3133/i2534.

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Geologic map of the Memphis Facula Quadrangle (Jg-7) of Ganymede. US Geological Survey, 1992. http://dx.doi.org/10.3133/i2289.

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Shaded relief and surface markings of the Hathor region of Ganymede. US Geological Survey, 1987. http://dx.doi.org/10.3133/i1860.

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