Relevant bibliographies by topics / Specters of Marx

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Academic literature on the topic 'Specters of Marx'

Author: Grafiati
Published: 4 June 2021
Last updated: 9 February 2022

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Journal articles on the topic "Specters of Marx"

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Martin, Bill. "Specters of Marx." International Philosophical Quarterly 36, no. 2 (1996): 243–45. http://dx.doi.org/10.5840/ipq199636214.

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Marshall, Donald G. "Specters of Marx." International Studies in Philosophy 29, no. 4 (1997): 104–5. http://dx.doi.org/10.5840/intstudphil1997294100.

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Critchley, Simon. "On Derrida's Specters of Marx." Philosophy & Social Criticism 21, no. 3 (April 1995): 1–30. http://dx.doi.org/10.1177/019145379502100301.

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Bewes, Timothy. "Vulgar Marxism: The Spectre Haunting Specters of Marx." Parallax 7, no. 3 (July 2001): 83–95. http://dx.doi.org/10.1080/13534640110063995.

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Zehfuss, Maja, Antonio Y. Vázquez-Arroyo, Dan Bulley, and Bal Sokhi-Bulley. "The Political Import of Deconstruction—Derrida’s Limits?: A Forum on Jacques Derrida’s Specters of Marx after 25 Years, Part I." Contexto Internacional 41, no. 3 (December 2019): 621–42. http://dx.doi.org/10.1590/s0102-8529.2019410300007.

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Abstract Jacques Derrida delivered the basis of The Specters of Marx: The State of the Debt, the Work of Mourning, & the New International as a plenary address at the conference ‘Whither Marxism?’ hosted by the University of California, Riverside, in 1993. The longer book version was published in French the same year and appeared in English and Portuguese the following year. In the decade after the publication of Specters, Derrida’s analyses provoked a large critical literature and invited both consternation and celebration by figures such as Antonio Negri, Wendy Brown and Frederic Jameson. This forum seeks to stimulate new reflections on Derrida, deconstruction and Specters of Marx by considering how the futures past announced by the book have fared after an eventful quarter century. Maja Zehfuss, Antonio Vázquez-Arroyo and Dan Bulley and Bal Sokhi-Bulley offer sharp, occasionally exasperated, meditations on the political import of deconstruction and the limits of Derrida’s diagnoses in Specters of Marx but also identify possible paths forward for a global politics taking inspiration in Derrida’s work of the 1990s.
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Johnson, Fletcher. "Specters of Marx in Lu Xun's Early Fiction." Derrida Today 11, no. 1 (May 2018): 7–21. http://dx.doi.org/10.3366/drt.2018.0165.

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Lu Xun is considered by many scholars the most influential modern Chinese writer, likened to Tolstoy, Shakespeare and Goethe in both scope and cultural impact, to the extent that Lu Xun scholarship has earned its own formal appellative: ‘Luxunology’. This impact is due not only to the initial impact of Lu Xun's fiction, but also greatly to Mao Zedong's use of Lu Xun during the Cultural Revolution. The history of Lu Xun's early fiction is analogous to the various historical manifestations, and original ‘spirit’, of Marxism. Through close readings of Lu Xun's early fiction, and then detailing the relationship between Mao Zedong's use of Lu Xun in the Cultural Revolution, I will explore Jacques Derrida's 1993 work Specters of Marx, especially focusing on Derrida's distinction between the ‘spirit’ and the ‘spectre’.
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Rodrigues, Carla, Rafael Haddock-Lobo, and Marcelo José Derzi Moraes. "Specters of Colonialidade: A Forum on Jacques Derrida’s Specters of Marx after 25 Years, Part V." Contexto Internacional 42, no. 1 (April 2020): 149–71. http://dx.doi.org/10.1590/s0102-8529.2019420100007.

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Abstract Jacques Derrida delivered the basis of The Specters of Marx: The State of the Debt, the Work of Mourning, & the New International as a plenary address at the conference ‘Whither Marxism?’ hosted by the University of California, Riverside, in 1993. The longer book version was published in French the same year and appeared in English and Portuguese the following year. In the decade after the publication of Specters, Derrida’s analyses provoked a large critical literature and invited both consternation and celebration by figures such as Antonio Negri, Wendy Brown and Frederic Jameson. This forum seeks to stimulate new reflections on Derrida, deconstruction and Specters of Marx by considering how the futures past announced by the book have fared after an eventful quarter century. In this fifth group of contributions, three philosophers explore the specters of colonialidade, the specifically Brazilian legacies of Portuguese and European coloniality. Carla Rodrigues opens the dialogue by exploring the haunting and melancholy provoked by colonial forms of violence and shows how confronting Brazilian necropolitics sustains the Derridean legacy; Rafael Haddock-Lobo offers a meditation on the difficulties of being before the law and standing before specters as a means of being justly haunted by the others of European philosophy in Brazil; finally, Marcelo Moraes continues the theme of Europe as a specter-producing machine and invokes specifically the presences of indigenous and Afro-Brazilian political resistances with the aim of deconstructing coloniality.
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Hirst, Aggie, Tom Houseman, Paulo Cesar Duque-Estrada, Jenny Edkins, and Cristiano Mendes. "Disobeying Marx, Disobeying Derrida—Hopes & Risks: A Forum on Jacques Derrida’s Specters of Marx after 25 Years, Part II." Contexto Internacional 41, no. 3 (December 2019): 643–62. http://dx.doi.org/10.1590/s0102-8529.2019410300008.

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Abstract Jacques Derrida delivered the basis of The Specters of Marx: The State of the Debt, the Work of Mourning, & the New International as a plenary address at the conference ‘Whither Marxism?’ hosted by the University of California, Riverside, in 1993. The longer book version was published in French the same year and appeared in English and Portuguese the following year. In the decade after the publication of Specters, Derrida’s analyses provoked a large critical literature and invited both consternation and celebration by figures such as Antonio Negri, Wendy Brown and Frederic Jameson. This forum seeks to stimulate new reflections on Derrida, deconstruction and Specters of Marx by considering how the futures past announced by the book have fared after an eventful quarter century. In this group of contributions, Aggie Hirst and Tom Houseman, Paulo Cesar Duque-Estrada, Jenny Edkins and Cristiano Mendes reflect on the legacies of Marx and Derrida: on whether Derrida emphasized the wrong Marxian heritage, on the promise and risks of hauntology, on the ghostly potential for justice amidst devastation, and on the paradox of deconstruction’s legacy itself.
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Plangesis, Yannis. "Deconstruction and Marxism Jacques Derrida's Specters of Marx." Philosophical Inquiry 18, no. 3 (1996): 91–115. http://dx.doi.org/10.5840/philinquiry1996183/47.

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Sing, Manfred, and Miriam Younes. "The Specters of Marx in Edward Said’s Orientalism." Welt des Islams 53, no. 2 (2013): 149–91. http://dx.doi.org/10.1163/15700607-0532p0001.

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Edward Said’s Orientalism was not only an attack on Western scholarship and impe­rialism, but also on Marxism. Said depicted Karl Marx as yet another Orientalist, Marxism as a form of Western domination and Arab Marxism as an expression of Self-Orientalization. Said claimed to have surpassed Marxism and Marxists who were “blinded to the fact of imperialism”. Said’s ambivalent relation to Marxism has not been thoroughly studied until now although it forms an important cornerstone in his argumentation and self-representation. This lacuna is surprising since many early Arab critics of Orientalism came from a Marxist background. Said either ignored them or rebuffed their interventions as “dogmatist”. The following article analyzes the nature of the conflict between the two sides and their underlying differences and reflects on the conditions affecting the Arab reception of Orientalism.
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Dissertations / Theses on the topic "Specters of Marx"

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Rosàs, Tosas Mar. "Exploración de la noción de mesianicidad sin mesianismo de Jaques Derrida y sus implicaciones eticopolíticas." Doctoral thesis, Universitat Pompeu Fabra, 2012. http://hdl.handle.net/10803/80835.

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This thesis explores the sense and the implications of the messianicity without messianism, a quasi-concept coined by the thinker Jacques Derrida (1930-2004) in the 1990s that refers to a “structure of experience” characterized by a lack of conclusion. On the one hand, this thesis examines the role that this notion plays within the vast work of Derrida; it aims at demonstrating that it neither indicates a rupture nor it constitutes a mere reformulation of his previous postulates. On the other hand, it establishes a dialogue between this quasi-concept and the use that a number of authors of the XXth century and the beginning of the XXIst, from different contexts and interests, do of the messianic tradition in order to formulate their own understandings of history, linguistics, politics and ethics. This thesis goes in depth into the shortcomings of the proposals of these authors and claims that the messianicity without messianism avoids many of them and offers a more fertile model for describing reality and acting in it. The final aim is to contribute to the reception of this quasi-concept ―which, in our opinion, so far has been slanted and insufficient― and prove that it rescues us from both the risks of the fundamentalisms and those of the paralyzing “everything goes” brought about by the phenomenon of the death of God.
Esta tesis explora el sentido y las implicaciones de la mesianicidad sin mesianismo, un casi-concepto acuñado por el pensador Jacques Derrida (1930-2004) en los años noventa del siglo XX que alude a una “estructura general de la experiencia” caracterizada por la ausencia de conclusión. Por un lado, esta tesis examina el papel que dicha noción desempeña dentro de la vasta obra de Derrida; quiere demostrar que ni supone una ruptura en su obra ni se trata de una mera reformulación de postulados anteriores. Por el otro, establece un diálogo entre este casi-concepto y el uso que una serie de autores del siglo XX e inicios del XXI, desde contextos e intereses distintos, hacen de la tradición mesiánica para formular sus propias concepciones de la historia, la lingüística, la política y la ética. Esta tesis ahonda en las limitaciones de las propuestas de estos autores y defiende que la mesianicidad sin mesianismo evita muchas de ellas y ofrece un modelo más fértil para describir la realidad e intervenir en ella. Todo ello con la voluntad de contribuir a la recepción de este casi-concepto ―que consideramos que, hasta el momento, ha sido sesgada e insuficiente― y mostrar que nos rescata de los riesgos tanto de los fundamentalismos como del paralizante “todo vale” acarreado por el fenómeno de la muerte de Dios.
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Melchiorri, Riccardo. "Calibration et préparation à la spectro-imagerie planétaire." Paris 7, 2004. http://www.theses.fr/2004PA077218.

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Bultel, Benjamin. "Serpentinisation et carbonatation de la croûte Martienne." Thesis, Lyon, 2016. http://www.theses.fr/2016LYSE1004/document.

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Depuis ces 3 derniers milliards d'années l'eau liquide est extrêmement peu présente sur Mars. Cependant les multiples données disponibles sur la planète montrent des preuves d'une présence importante d'eau liquide depuis l'accrétion de la planète jusqu'à environ 3,7 milliards d'années. L'hypothèse dominante aujourd'hui est que Mars possédait une atmosphère plus dense (possiblement riche en CO2) au début de son histoire. Une grande partie de cette atmosphère et de l'eau auraient été perdu dans l'espace. Une autre hypothèse pour la diminution de la quantité d'eau liquide disponible et pour la diminution de l'atmosphère est le stockage d'eau et de CO2 dans la croûte. La croûte martienne est étudiée via les données de spectro-imagerie CRISM pour caractériser l'altération hydrothermale primitive de la planète. Des détections de serpentine et de carbonates confirment que le stockage d'une partie de l'eau et de l'atmosphère martienne a eu lieu. Des contraintes supplémentaires sont apportées par de la modélisation géochimique de la serpentinisation et de la carbonatation de la croûte martienne via les programme EQ3/6. L'importance de la serpentinisation et de la carbonatation de la croûte martienne est ainsi réévaluée. Les résultats permettent d'ouvrir la réflexion sur le rôle de la serpentinisation et de la carbonatation sur l'évolution de la quantité d'eau liquide disponible et sur l'évolution de l'atmosphère. En outre, les conditions thermodynamiques permettent d'apporter des contraintes sur le potentiel exobiologique de la croûte martienne
Over the last 3 billion years liquid water has an extremely limited presence on Mars. However, the multiple data available on the planet show evidences of a significant presence of liquid water from the accretion of the planet until about 3.7 billion years. The prevailing hypothesis today is that Mars had a denser atmosphere (possibly rich in CO2) early in its history. Much of this atmosphere and water were lost in space. Another possibility for reducing the amount of liquid water available and the reduction of the atmosphere is the water storage of water and CO2 in the crust. The Martian crust is studied via CRISM spectro-imaging data to characterize the early hydrothermal alteration of the planet. Serpentine and carbonates of detections confirm that the storage of a portion of the water and the atmosphere of Mars occurred. Additional constraints are provided by the geochemical modeling of serpentinization and carbonation of the Martian crust through EQ3/6 programs. The importance of serpentinization and carbonation of the Martian crust is thus reassessed. The results allow to open the debate on the role of serpentinization and carbonation on the evolution of the liquid water available and the evolution of the atmosphere. In addition, the thermodynamic conditions help provide constraints on the exobiology potential of the Martian crust
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Fernando, Jennifer. "Caractérisation des propriétés physiques de la surface de Mars à partir de mesures spectro-photométriques orbitales." Thesis, Paris 11, 2014. http://www.theses.fr/2014PA112293/document.

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Depuis leur formation, les surfaces des corps de notre Système Solaire montrent une diversité étonnante. Cette diversité est le reflet des processus géologiques qui ont modelé les surfaces planétaires au cours du temps. Parmi les objets du Système Solaire, Mars constitue un objet particulièrement intéressant car il présente de nombreuses similitudes avec notre planète. La minéralogie de la surface de Mars est bien documentée. Cependant, on dispose de peu d'information sur les paramètres physiques des matériaux qui sont également des traceurs des processus géologiques. Un des objectifs de cette thèse est de développer et de valider un outil permettant leur détermination à partir de techniques d'investigation spatiale depuis l'orbite et d’interpréter les résultats. Pour cela, une approche basée sur la photométrie, qui étudie les propriétés de diffusion des matériaux de surface, a été développée et validée. Ces propriétés de diffusion dépendent de la composition mais aussi des propriétés physiques des matériaux comme la taille, la forme, la structure interne, la rugosité des grains et la rugosité de la surface. Les données hyperspectrales multi-angulaires CRISM (Compact Reconnaissance Imaging Spectrometer for Mars) à bord de la sonde Mars Reconnaissance Orbiter (11 images prises à des angles d'émergence variés) ont été utilisées, permettant de contraindre le comportement de diffusion des matériaux de surface. Tout d'abord, les données sont corrigées de la contribution atmosphérique à l'aide de l'algorithme nommée MARS-ReCO (Multi-angle Approach for Retrieval of Surface Reflectance for CRISM Observations), développé en collaboration avec Xavier Ceamanos et Sylvain Douté (IPAG) au cours de la thèse. Puis, les données de réflectance de surface à différentes géométries sont analysées en inversant à l’aide d’une approche bayésienne le modèle photométrique de Hapke qui décrit le transfert radiatif en milieu granulaire. Ce modèle dépend de six paramètres photométriques de surface (e.g., albédo de diffusion, fonction de phase, rugosité macroscopique de la surface), reliés aux propriétés physiques des matériaux comme la taille, la structure interne, la forme, la rugosité des grains, et la rugosité de la surface.Une première application a été menée au niveau des sites d'atterrissage des rovers de la mission Mars Exploration Rover, où des données orbitales et in situ sont disponibles. Ces dernières sont utilisées comme «vérité terrain» pour valider les interprétations des paramètres photométriques estimés. Dans ce travail, des cartes des paramètres photométriques ont été fournies le long et autour du trajet des rovers permettant d'avoir accès aux informations des propriétés des matériaux sur une étendue plus importante que les données in situ. Une interprétation de chacun des paramètres et un lien aux propriétés physiques et aux processus géologiques ont été fournis. Les résultats montrent des propriétés de diffusion variés au sein d'une observation CRISM (10x10km) suggérant que les surfaces sont contrôlées par des processus géologiques plus locaux (e.g., processus éoliens, fragmentation de la croûte par impact).Une dernière partie se focalise sur la détermination des propriétés de diffusion des matériaux de surface de différents terrains géologiques formés dans des contextes différents. Le but est d'identifier les variabilités des propriétés de diffusion à travers Mars
The PhD work focuses on the characterization of geological processes on planetary surfaces. Due to the lack of broad scale in situ information about the surface physical properties of the Martian materials (recording the geological processes), my work centers on the development and validation of an approach for their estimation from orbital spaceborne datasets. In addition, determining the physical properties has an implication for the spectroscopic interpretation notably for the mineral abundances. More specifically, I developed an approach for the determination and the analysis of the Martian surface scattering properties using CRISM (Compact Reconnaissance Imaging Spectrometer for Mars) observations [Murchie et al., 2007] on-board MRO (Mars Reconnaissance Orbiter). CRISM provides multi-angular (varied emission angles) hyperspectral images which allow the characterization of the surface scattering behavior at ∼200m/pixel. The scattering behavior depends on the material composition but also the physical properties such as the grain size, shape, internal structure, and the surface roughness / porosity. The main objective is to observe the spatial variations of the surface scattering properties and the photometric parameters as a function of geological units.The methodology I employ is based on the estimation of the surface photometric parameters in term of surface physical properties. After an atmospheric correction (aerosols) by the Multi-angle Approach for Retrieval of the Surface Reflectance from CRISM Observations (MARS-ReCO) [Ceamanos et al., 2013] developed in collaboration with X. Ceamanos and S. Douté (IPAG, France), I analyze the surface reflectance taken at varied geometries by inverting the Hapke photometric model [Hapke, 1993] depending on six parameters (single scattering albedo, 2-term phase function, macroscopic roughness and 2-term opposition effects parameters) in a Bayesian framework [Fernando et al., 2013]. The algorithm for the correction for the aerosols and the methodology for the estimates of surface photometric parameters have been validated by comparing the results from orbit to the in situ photometric measurements from Mars Exploration Rover (MER) rovers [Fernando et al. 2013].The MER landing sites located at Gusev Crater and Meridiani Planum provide an excellent opportunity to ground truth and validate the interpretation of derived Hapke photometric parameters as both orbital and in situ data are readily available over numerous geological terrains. Orbital results are consistent with the in situ observations. In my work, I mapped the surface scattering properties in and around the rover path, providing extended information over a wider area. Significant variations in the scattering properties are observed inside a CRISM observation (10x10km) suggesting that the surfaces are controlled by local geological and climatic processes [Fernando et al., in revision].The last part of this work focuses on the determination of the surface photometric parameters of different Martian geological terrains under different contexts in order to identify variabilities of the scattering properties
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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 radicaux oh par photodissociation des molecules d'eau, due a l'absorption du rayonnement solaire dans la region tres proche du noyau par ces memes molecules d'eau. Le spectre d'emission de c2 presente des variations a l'interieur de la coma. Ces variations sont expliquees par le temps important (environ 3000 s) mis par ce radical pour atteindre son equilibre de fluorescence a partir de sa creation, et par deux sources distinctes (le noyau et une source diffuse, ayant une autre molecule-mere). Un modele du spectre de fluorescence, base sur une methode type monte-carlo, et etabli en fonction de la distribution initiale d'energie et du temps, est presente de facon detaillee
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HURTREZ, STEPHANE. "Caracterisation geologique des surfaces de mars et de la terre par spectro-imagerie infrarouge." Paris 11, 1995. http://www.theses.fr/1995PA112434.

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Une methode d'etude des images multi-spectrales infrarouges ism (phobos-arat) et aviris est developpee. Elle repose sur la representation graphique de deux parametres caracteristiques de chaque spectre de la region etudiee l'un en fonction de l'autre. Les nuages de points obtenus, delimitent des familles spectrales, correspondant a des surfaces planetaires ayant des proprietes physico-chimiques voisines. On determine alors (par moyenne) un spectre representatif de chaque famille. Chaque representant peut etre caracterise ensuite spectralement en termes de bandes d'absorption et de mineralogie. Enfin, apres avoir affecte une couleur a chaque famille spectrale determinee, on colorie sur une carte de la region etudiee chaque element d'image de la couleur de la famille auquel son spectre appartient. On obtient ainsi une carte d'unites spectrales permettant de visualiser les relations geologiques entre les diverses unites decrites. L'application s'avere riche en enseignements sur mars, plus delicate sur terre en raison des sols, et de la vegetation et des variations topographiques. Une annexe presente un travail sur le volcanisme relie aux interactions tectoniques entre les bassins d'impacts geants sur mars, et montre aussi qu'elles peuvent expliquer en partie la distribution des reliquats de failles concentriques associees aux bassins d'impacts
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Lamartinie, Sujit. "Définition et tests du système de refroidissement du détecteur de l'imageur spectral miniaturisé ÇIVA-MARS pour l'étude in-situ d'échantillons martiens." Paris 6, 2003. http://www.theses.fr/2003PA066177.

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Carr, Jeff. "A Spectre is Haunting Samuel Clemens: A Marxist Critique of Wealth as Resolution in Mark Twain's Novels." TopSCHOLAR®, 2006. http://digitalcommons.wku.edu/theses/447.

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The distribution of wealth occurs frequently in Mark Twain's novels, especially at the resolution. Indeed, Twain uses wealth as resolution in The Adventures of Tom Sawyer, The Prince and the Pauper, The Adventures of Huckleberry Finn, and Pudd'nhead Wilson. The repeated use of this formula in the author's approach to novel writing indicates the tremendous influence that capitalism had in shaping his worldview. In his early works, Twain appears to endorse capitalism in his use of wealth as resolution. Tom Sawyer, The Prince and the Pauper, and Huckleberry Finn each conclude with the distribution of capital as a reward to the protagonists and as an effective solution to conflicts presented throughout the texts. However, the tone of Pudd'nhead Wilson is decidedly different. This later novel ends with wealth as resolution, but the result is not the happiness granted to characters in Twain's previous works. Instead, the fates of Tom Driscoll, Chambers, and Roxy leave the reader with a sense of the inadequacy of capitalism. Twain's change in his approach reveals a rejection of bourgeois values. An examination at the resolution to all four novels reveals Twain's shifting Weltanschauung, culminating with a rejection of the dominant ideology in Pudd'nhead Wilson.
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Schädler, Marc René [Verfasser]. "Robust automatic speech recognition and modeling of auditory discrimination experiments with auditory spectro-temporal features / Marc René Schädler." Oldenburg : BIS-Verlag, 2016. http://d-nb.info/1113296755/34.

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Bonello, Guillaume. "Etalonnage au sol d'expériences spatiales de spectro-imagerie visible et proche infrarouge pour l'étude de surfaces planétaires : cas de VIRTIS sur ROSETTA et OMEGA sur MARS-EXPRESS." Paris 11, 2001. http://www.theses.fr/2001PA112341.

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Cette thèse est consacrée à l'étude, la réalisation, la qualification et la mise en oeuvre d'un dispositif expérimental d'étalonnage au sol pour les expériences spatiales de spectro-imagerie fonctionnant dans la domaine visible et proche infrarouge VIRTIS et OMEGA. Dans les 20 dernières années, la spectro-imagerie s'est imposée comme une technique de télédétection unique pour étudier les surfaces et les atmosphères des objets planétaires, de manière préparatoire ou complémentaire aux analyses in-situ. Mais les expériences passés ont aussi montré toute la complexité de l'analyse des mesures issues de ce type d'instruments : des artefacts instrumentaux peuvent engendrer une mauvaise interprétation des données acquises entraînant une mise en échec des scénarios scientifiques déduits. Ces biais ne peuvent être levés que par une minutieuse analyse des réponses instrumentales des expériences développées, elle nécessite d'apporter un soin particulier à la phase d'étalonnage devenant partie prenante de l'analyse scientifique. La première partie de ce travail a consisté à élaborer un cahier des charges du dispositif en fonction des performances des expériences étudiées. Les études relatives aux différents sous-ensembles conduisant à la réalisation du dispositif d'étalonnage ont pu ensuite être menées. La validation et la caractérisation des performances intrinsèques de ce dispositif ont constitué la plus grande partie des résultats de ce travail étant donnés qu'elles conditionnent la qualité de l'étalonnage et donc le retour scientifique des expériences. Ceux-ci ont montré la parfaite adéquation du dispositif réalisé aux spécifications requises. La mise en oeuvre du dispositif dans le cadre de l'étalonnage du modèle de vol de VIRTIS a confirmé ces résultats. Dans le cas d'OMEGA, des mesures directes d'échantillons minéralogiques observés en réflectance augmentera, pour la première fois, les possibilités de préparation de la réduction de données de la mission scientifique
This thesis is dedicated to the study, the implementation, the qualification and the use of a ground calibration set-up for the visible and near infrared imaging spectrometer space experiments VIRTIS and OMEGA. Over the past 20 years, imaging spectrometry was essential to remote sensing surfaces and atmospheres of planetary objects, prior and in addition to in-situ analyses. However, the last experiments also showed the complexity of the analyses of measurements resulting from this type of instruments. Indeed, artifacts from the instrument can generate wrong interpretations of the data and consequently of the inferred scientific scenarios. This needs a meticulous analysis of the instrumental responses of the developed experiments, taking a particular care to the calibration phase becoming part of the scientific analysis process. The first part of this work consisted in working out a specification document of the set-up according to the performances of the studied experiments. We could then carry out the studies relating to the various subsets leading to the realization of the calibration set-up. The validation and the characterization of the intrinsic performances of this set-up constituted most of the results of this work since they condition the quality of the calibration and thus the scientific return of the experiments. These results showed the perfect adequacy of the device carried out with the necessary specifications. The use of the device within the framework of the calibration of the VIRTIS flight model confirmed these results. In the case of OMEGA, direct measurements of mineralogical samples observed in reflectance will increase, for the first time, the possibilities of preparation of the scientific data reduction
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Books on the topic "Specters of Marx"

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Jacques, Derrida. Specters of Marx: The state of the debt, the work of mourning, and the New international. New York: Routledge, 1994.

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Jacques, Derrida. Specters of Marx: The state of the debt, the work of mourning, and the new international. New York: Routledge, 1994.

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Zahn, Theodor. Specter of the Past. New York: Bantam Books, 1997.

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Star Wars: Specter of the Past: Hand of Thrawn Duology - Book 1. New York: Bantam Books, 1997.

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Jacques, Derrida. Spectres de Marx: L'état de la dette, le travail du deuil et la nouvelle Internationale. Paris: Editions Galilée, 1993.

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Two boys, divided by fortune, united by tragedy: A true story of the pursuit of justice. Philadelphia: Camino Books, 2008.

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Derrida, Africa, and the Middle East. New York: Palgrave Macmillan, 2009.

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Simsion, Graeme C. The rosie effect. Melbourne, Victoria: Text Publishing, 2014.

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Simsion, Graeme C. L'effet Rosie: Ou le Théorème de la cigogne. Paris: NiL, 2015.

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Simsion, Graeme C. The Rosie effect. Thorndike, Maine: Center Point Large Print, 2015.

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Book chapters on the topic "Specters of Marx"

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Pawling, Christopher. "Rediscovering Commitment: Jacques Derrida’s Specters of Marx." In Critical Theory and Political Engagement, 61–87. London: Palgrave Macmillan UK, 2013. http://dx.doi.org/10.1057/9781137315236_4.

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Jobling, David. "Jerusalem and Memory: On a Long Parenthesis in Derrida’s Specters of Marx." In Derrida’s Bible, 99–115. New York: Palgrave Macmillan US, 2004. http://dx.doi.org/10.1007/978-1-137-09037-9_7.

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Charley, Jonathan. "Spectres of Marx in City X." In Forty Ways To Think About Architecture, 155–62. Hoboken, NJ, USA: John Wiley & Sons, Inc., 2015. http://dx.doi.org/10.1002/9781118822531.ch22.

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Carpenter, Sara, and Shahrzad Mojab. "Introduction: A Specter Haunts Adult Education: Crafting a Marxist-Feminist Framework for Adult Education and Learning." In Educating from Marx, 3–18. New York: Palgrave Macmillan US, 2011. http://dx.doi.org/10.1057/9780230370371_1.

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Parkin-Gounelas, Ruth. "Anachrony and Anatopia: Spectres of Marx, Derrida and Gothic Fiction." In Ghosts, 127–43. London: Palgrave Macmillan UK, 1999. http://dx.doi.org/10.1057/9780230374812_6.

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Reames, Donald V. "Summary and Conclusions." In Solar Energetic Particles, 221–25. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-66402-2_10.

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AbstractIn this chapter we summarize our current understanding of SEPs, of properties of the sites of their origin and of the physical processes that accelerate or modify them. These processes can leave an indelible mark on the abundances of elements, isotopes, ionization states, anisotropies, energy spectra and time profiles of the SEPs. Transport of the ions to us along magnetic fields can impose new variations in large events or even enhance the visibility of the source parameters as the SEPs expand into the heliosphere. We lack physical models that can follow the complexity of SEP abundance variations.
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Reames, Donald V. "High Energies and Radiation Effects." In Solar Energetic Particles, 135–49. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-66402-2_6.

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AbstractIn this chapter we characterize the high-energy spectra of protons that can penetrate shielding and determine the radiation dose to humans and equipment in space. High-energy spectral breaks or “knees”, seen in all large SEP events, determine the contribution of highly penetrating protons. The streaming limit, discussed earlier, places an upper bound on particle fluences early in events and the radial variation of intensities is important for near-solar and deep-space missions. The streaming limit is a strong function of radial distance from the Sun. We also consider requirements for a radiation storm shelter for deep space, a mission to Mars, suitability of exoplanets for life, and radiation-induced chemistry of the upper atmosphere of Earth.
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Trill, Suzanne. "Spectres and Sisters: Mary Sidney and the ‘Perennial Puzzle’ of Renaissance Women’s Writing." In Renaissance Configurations, 191–211. London: Palgrave Macmillan UK, 1998. http://dx.doi.org/10.1057/9780230378667_9.

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Van Cromphaut, Caroline, Valdirene G. de Resende, Eddy De Grave, and Robert E. Vandenberghe. "Temperature dependence of the hyperfine parameters of the iron bearing phases in the Mössbauer spectra collected by the Mars Exploration Rover Spirit." In ISIAME 2008, 325–30. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-01370-6_42.

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"Injunctions of Marx." In Specters of Marx, 21–80. Routledge, 2012. http://dx.doi.org/10.4324/9780203821619-8.

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Conference papers on the topic "Specters of Marx"

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Eng, Alivia, Melissa Rice, Michael D. Kraft, Kristiana Lapo, Kathleen M. Hoza, and Sean R. Mulcahy. "INFLUENCE OF SILICA COATINGS ON THE REFLECTANCE SPECTRA OF MARS ANALOG BASALTS." In GSA 2020 Connects Online. Geological Society of America, 2020. http://dx.doi.org/10.1130/abs/2020am-359885.

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Efimov, A. I., L. A. Lukanina, L. N. Samoznaev, V. K. Rudash, I. V. Chashei, M. K. Bird, M. Pätzold, et al. "Coronal Radio Sounding Experiments with Mars Express: Scintillation Spectra during Low Solar Activity." In TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP, 2010. http://dx.doi.org/10.1063/1.3395973.

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Martin, Fiore, Oussama Metatla, Nick Bryan-Kinns, and Tony Stockman. "Accessible Spectrum Analyser." In The 22nd International Conference on Auditory Display. Arlington, Virginia: The International Community for Auditory Display, 2016. http://dx.doi.org/10.21785/icad2016.041.

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This paper presents the Accessible Spectrum Analyser (ASA) developed as part of the DePic project (Design Patterns for Inclusive collaboration) at Queen Mary University of London. The ASA uses sonification to provide an accessible representation of frequency spectra to visually impaired audio engineers. The software is free and open source and is distributed as a VST plug-in under OSX and Windows. The aim of reporting this work at the ICAD 2016 conference is to solicit feedback about the design of the present tool and its more generalized counterpart, as well as to invite ideas for other possible applications where it is thought that auditory spectral analysis may be useful, for example in situations where line of sight is not always possible.
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Violante-Carvalho, Nelson, and Ian S. Robinson. "On the Performance of the MPI Algorithm for the Retrieval of Significant Wave Height From ERS Synthetic Aperture Radar." In ASME 2003 22nd International Conference on Offshore Mechanics and Arctic Engineering. ASMEDC, 2003. http://dx.doi.org/10.1115/omae2003-37070.

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Spaceborne Synthetic Aperture Radar (SAR) is to date the only source of two dimensional directional wave spectra with continuous and global coverage when operated in the so-called SAR Wave Mode (SWM). Since the launch in 1991 of the first European Remote Sensing Satellite ERS-1 and more recently with ENVISAT millions of SWM imagettes containing detailed spectral information are now available in quasi-real time. This huge amount of directional wave data has opened up many exciting possibilities for the improvement of our knowledge of the dynamics of ocean waves. However the retrieval of wave spectra from SAR images is not a trivial exercise due to the nonlinearities involved in the mapping mechanism. The Max-Planck Institut (MPI) scheme was the first ever proposed and most widely used algorithm to retrieve directional wave spectra from SAR images. In this work significant wave height retrieved from SAR images using the MPI scheme are compared against one year of directional buoy measurements obtained in deep water and against WAM spectra. Our results show that for periods shorter than 12 seconds the WAM model performs better than the MPI method, even considering the fact that the model is used as first guess to the MPI scheme. However, for periods longer than 12 seconds (the part of the spectrum directly observed by SAR) the MPI method performs better than WAM. This is in contrast with the results obtained by Voorrips et al. (2001), who found that the performance of the WAM model is superior even when only the low wavenumber part of the spectrum is considered.
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Dixon, Darian T., Melissa S. Rice, and Edward A. Cloutis. "HYDRATED SULFATES ON MARS: CHARACTERIZING VISIBLE TO NEAR-INFRARED SPECTRA AND IMPLICATIONS FOR ROVER-BASED MULTISPECTRAL IMAGERS." In GSA Annual Meeting in Denver, Colorado, USA - 2016. Geological Society of America, 2016. http://dx.doi.org/10.1130/abs/2016am-287194.

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Yiu, M. W., H. Li, and Y. Zhou. "Wavelet Analysis of Reynolds Number Effect on 3-D Vorticity in a Turbulent Near Wake." In ASME/JSME 2003 4th Joint Fluids Summer Engineering Conference. ASMEDC, 2003. http://dx.doi.org/10.1115/fedsm2003-45025.

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When Reynolds number, Re (≡U∞d/v, where U∞ is the free stream velocity, d is the cylinder diameter and v is the kinematic viscosity of the fluid), is in the range of 103 to 104, there is a large variation in the near-wake formation region in terms of the base pressure coefficient, the fluctuating lift coefficient, the vortex formation length, which have previously been connected to the generation of small-scale Kelvin-Helmholtz vortices. This work aims to investigate how this Re variation affects the three components of vorticity in terms of time-averaged and small-scale structures and also to provide a relatively complete set of 3-D vorticity data. All three components of vorticity data were simultaneously measured in the intermediate region of the turbulent wake using a multi-wire vorticity probe. It is observed that the root-mean-square (rms) values of the three vorticity components increase with Re, especially the streamwise component, which shows a large jump from Re = 5×103 to 104. At the central frequencies of f0 and 2f0, the contributions from the large-scale and intermediate-scale structures of ωzi2/(ωz2)max decreases 13% and 16% respectively as the Re. increases. However, at the central frequency of 16f0, the contribution of the small-scale structure of ωzi2/(ωz2)max dramatic suddenly 7% increase at Re = 5×103 to 104. The result suggest the generation of small-scale Kelvin-Helmholtz vortices in the spanwise structure. The effect of Re on vorticity signals, spectra, contributions from the wavelet components to the vorticity variances are also examined.
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Aquaro, D., M. D. Carelli, G. Forasassi, R. Lo Frano, and N. Zaccari. "Seismic Response of Reactor Vessel Internals in the IRIS Reactor." In 14th International Conference on Nuclear Engineering. ASMEDC, 2006. http://dx.doi.org/10.1115/icone14-89579.

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The intent of this paper is the presentation and discussion of a methodology for the evaluation and analysis of seismic loads effects on a nuclear power plant. To help in focussing the presented methodology, a preliminary simplified analysis of an integral, medium size next generation PWR reactor structure (IRIS project, an integral configuration PWR under study by an international group) was considered as an application example also for models/codes evaluation. The performed preliminary seismic analysis, even though by no means complete, is intended to evaluate the method of calculating the effects of dynamic loads propagation to the reactor internals for structural design as well as geometrical and functional optimisation purposes. To this goal, finite element method and separated (sub) structures approaches were employed for studying the overall dynamic behaviour of the nuclear reactor vessel. The analysis was set up by means of numerical models, implemented on the MARC FEM code, on the basis of Design Response Spectra as indicated on the relevant rules for Nuclear Power Plants (NRC 1.60) design. The seismic analysis is indented to evaluate the dynamic loads propagated from the ground through the Containment System and Vessel to the Steam Generator’s tubes.
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Herrero-Martin, David, Max Kauer, Grzegorz Sienski, Argyro Fourtouna, Robert Kralovics, and Heinrich Kovar. "Abstract LB-462: AGO2 PAR-CLIP suggests a shift in specific miRNA target spectra upon modulation of EWS-FLI1 in Ewing's sarcoma." In Proceedings: AACR 103rd Annual Meeting 2012‐‐ Mar 31‐Apr 4, 2012; Chicago, IL. American Association for Cancer Research, 2012. http://dx.doi.org/10.1158/1538-7445.am2012-lb-462.

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Forristall, George Z., Stephen F. Barstow, Harald E. Krogstad, Marc Prevosto, Paul H. Taylor, and Peter Tromans. "Wave Crest Sensor Intercomparison Study: An Overview of WACSIS." In ASME 2002 21st International Conference on Offshore Mechanics and Arctic Engineering. ASMEDC, 2002. http://dx.doi.org/10.1115/omae2002-28438.

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The Wave Crest Sensor Intercomparison Study (WACSIS) was designed as a thorough investigation of the statistical distribution of crest heights. Measurements were made in the southern North Sea during the winter of 1997–1998 from the Meetpost Noordwijk in 18 m water depth. The platform was outfitted with several popular wave sensors, including Saab and Marex radars, an EMI laser, a Baylor wave staff and a Vlissingen step gauge. Buoys were moored nearby to obtain directional spectra. Two video cameras viewed the ocean under the wave sensors and their signals were recorded digitally. The data analysis focused on comparisons of the crest height measurements from the various sensors and comparisons of the crest height distributions derived from the sensors and from theories. Some of the sensors had greater than expected energy at high frequencies. Once the measurements were filtered at 0.64 Hz, the Baylor, EMI and Vlissingen crest height distributions matched quite closely, while those from the other sensors were a few percent higher. The Baylor and EMI crest distributions agreed very well with the statistics from second order simulations, while previous parameterizations of the crest height distribution were generally too high. We conclude that crest height distributions derived from second order simulations can be used with confidence in engineering calculations. The data were also used in investigations of crest and trough shapes and the joint height/period distribution.
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Magnusson, Susanne, Thomas Wiebe, Ulf Kristoffersson, Helena Jernström, and Håkan Olsson. "Abstract 5512: Increased incidence of adult cancers in relatives of childhood cancer patients and difference in tumor spectra between families with single and multiple cases of childhood tumors." In Proceedings: AACR 103rd Annual Meeting 2012‐‐ Mar 31‐Apr 4, 2012; Chicago, IL. American Association for Cancer Research, 2012. http://dx.doi.org/10.1158/1538-7445.am2012-5512.

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Reports on the topic "Specters of Marx"

1

Stave, Sean C., Kevin E. Dorow, Brian D. Glasgow, Jacob M. Benz, and Jesse A. Willett. MARS June 2012 Flight Data: Natural Background and Point Source Spectra. Office of Scientific and Technical Information (OSTI), November 2012. http://dx.doi.org/10.2172/1113622.

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