Academic literature on the topic 'Occultation de la violence'
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Journal articles on the topic "Occultation de la violence"
Luis, Ballester Brage, Rosario Pozo Gordaliza, and Carmen Orte Socías. "Delocalized Prostitution: Occultation of the New Modalities of Violence." Procedia - Social and Behavioral Sciences 161 (December 2014): 90–95. http://dx.doi.org/10.1016/j.sbspro.2014.12.015.
Full textLacombe, Delphine. "Visibilité et occultation des violences masculines envers les femmes au Nicaragua (1979-1996)." Problèmes d'Amérique latine 84, no. 2 (2012): 13. http://dx.doi.org/10.3917/pal.084.0013.
Full textStahl, Don. "The Occultation." Chicago Review 40, no. 4 (1994): 19. http://dx.doi.org/10.2307/25305877.
Full textDyson, Freeman J. "Occultation Astronomy." International Astronomical Union Colloquium 123 (1990): 413–15. http://dx.doi.org/10.1017/s0252921100077368.
Full textKammarti, Adrian. "La double occultation." Critique 901, no. 6 (May 24, 2022): 577–87. http://dx.doi.org/10.3917/criti.901.0577.
Full textStagliano, J. J. "Dynamical occultation correction." Physics and Chemistry of the Earth, Part B: Hydrology, Oceans and Atmosphere 25, no. 10-12 (January 2000): 833–35. http://dx.doi.org/10.1016/s1464-1909(00)00111-8.
Full textSchaefer, Bradley E., Henk J. J. Bulder, and Jean Bourgeois. "Lunar occultation visibility." Icarus 100, no. 1 (November 1992): 60–72. http://dx.doi.org/10.1016/0019-1035(92)90018-3.
Full textAgol, Eric. "Occultation and Microlensing." Astrophysical Journal 579, no. 1 (November 2002): 430–36. http://dx.doi.org/10.1086/342880.
Full textLiu, Congliang, Gottfried Kirchengast, Yueqiang Sun, Veronika Proschek, Xin Wang, Longfei Tian, Qifei Du, et al. "Impacts of Orbital and Constellation Parameters on the Number and Spatiotemporal Coverage of LEO-LEO Occultation Events." Remote Sensing 13, no. 23 (November 29, 2021): 4849. http://dx.doi.org/10.3390/rs13234849.
Full textZhu, Qinglin, Mingchen Sun, Xiang Dong, and Pengfei Zhu. "Design and Simulation of Stellar Occultation Infrared Band Constellation." Remote Sensing 14, no. 14 (July 10, 2022): 3327. http://dx.doi.org/10.3390/rs14143327.
Full textDissertations / Theses on the topic "Occultation de la violence"
Prigent, Pierre-Guillaume. "Les stratégies des pères violents en contexte de séparation parentale : contrôle coercitif, complicité institutionnelle et résistance des femmes." Thesis, Brest, 2021. http://www.theses.fr/2021BRES0102.
Full textIn this thesis, we study the strategies that abusive fathers adopt in the context of parental separation. Based on interviews with twenty women who have separated from an abusive partner with whom they had children, we identify the tactics employed by abusers before, during and after separation: isolation, deprivation of resources, control, intimidation, devaluation, confusion, overburden of responsibility and violence. These tactics accumulate, combine and intertwine in the strategy to maintain power and control over the victimised woman and children. Social and institutional responses to violence may replicate the tactics identified, and may involve complicity with the abuser.The space for action of the victims, reduced during the relationship and then extended by the separation, is again restricted by the principle of joint parental authority, which implies maintaining the link that can expose the victims to further violence and subject them to control of their daily activities by the aggressor.Women's resistance to post-separation violence and control and their attempts to protect the children are then seen as an obstacle to co-parenting. Victims' parental rights may be curtailed or the children's residence transferred to the abuser. This analysis highlights the institutional resistance to taking post-separation domestic violence into account in parenting
Olkin, Catherine Blair. "Stellar occultation studies of Triton's atmosphere." Thesis, Massachusetts Institute of Technology, 1996. http://hdl.handle.net/1721.1/55046.
Full textIncludes bibliographical references (p. 127-136).
by Catherine Blair Olkin.
Ph.D.
Salyk, Colette Vanessa. "Stellar occultation investigations of Pluto's atmosphere." Thesis, Massachusetts Institute of Technology, 2003. http://hdl.handle.net/1721.1/114110.
Full textCataloged from PDF version of thesis. Page 21 missing from original thesis.
Includes bibliographical references (pages 27-28).
We investigate the shape of Pluto's atmosphere using data from the occultation of the V=15.7 star P131.1 by Pluto on 2002 Aug 21 (UT). We find that Pluto's atmosphere, as projected onto the sky, is noticeably non-circular. This implies an overall ellipsoidal shape, which could be an indication of high winds and/or latitudinal stratification. We decide to compare our results to those obtained from datasets of the occultation of P8 by Pluto on 1988 June 9 (UT). Previous analyses of these datasets by Millis et al. (1993) had led to the conclusion that Pluto's atmospheric shape did not deviate from that of a sphere. However, we find that the 1988 datasets do not conclusively demonstrate that this is the case. We conclude that Pluto's atmosphere is currently non-spherical and could have been non-spherical at the time of the 1988 occultation. Implications for high winds and/or latitudinal stratification present exciting possibilities to be investigated by the upcoming New Horizons mission to Pluto.
by Colette Salyk.
S.B.
Cooray, Asantha Roshan. "Stellar occultation observations of Saturn's upper atmosphere." Thesis, Massachusetts Institute of Technology, 1997. http://hdl.handle.net/1721.1/53030.
Full textIncludes bibliographical references (leaves 74-79).
by Asantha Roshan Cooray.
M.S.
Foust, Jeffrey Alan 1971. "Stellar occultation studies of Saturn's upper atmosphere." Thesis, Massachusetts Institute of Technology, 1999. http://hdl.handle.net/1721.1/9528.
Full textIncludes bibliographical references (p. 224-230).
The properties of Saturn's upper atmosphere are not well-known despite several spacecraft flybys. However, the region of 1-100 [mu]bar can be studied in detail by observing stellar occultations -- when the planet passes in front of a star -- from ground-based or Earth-orbiting telescopes. We use data from five such occultations: three observed in 1995 by the Faint Object Spectrograph (FOS) on the Hubble Space Telescope (HST), one observed in 1996 at the NASA Infrared Telescope Facility (IRTF) and one in 1989 observed by a different instrument at the IRTF. The data span latitudes from 52° south to 75 ° north. We fit isothermal models to each data set and also perform numerical inversions. These analyses show that temperatures in the 1-10 [mu]bar range can vary significantly as a function of season and latitude, ranging from 121 to 160 K, in accordance with radiative transfer models for the atmosphere. We also search for evidence of gravity wave saturation in Saturn's upper atmosphere, as seen in other planetary atmospheres, by analyzing the power spectra of temperature and density data and by studying the temperature lapse rate in the atmosphere. Our analysis is consistent with saturated gravity waves for all data sets, although gravity wave saturation is not the sole explanation for the spectra. We take advantage of the wavelength-resolved HST FOS data to study the composition of Saturn's upper atmosphere. We measured the difference in feature times for data taken at two wavelengths, and use the different refractivities of hydrogen and helium, as a function of wavelength to compute the relative amounts of the two elements in the planet's atmosphere. We find that the helium mass fraction is 0.26 ± 0.10, higher than that found using Voyager data, but marginally consistent with theoretical models for the evolution of Saturn's atmosphere, although the large error bars on the results make a definitive conclusion problematic.
by Jeffrey Alan Foust.
Ph.D.
Bérard, Diane. "Etude des anneaux de Chariklo par occultation stellaire." Thesis, Paris 6, 2017. http://www.theses.fr/2017PA066128/document.
Full textStellar occultations are a very powerful tool to study small bodies of the Outer Solar System, which are usually too faint or too far away to be studied by others techniques. They occur when a body passes in front of a background star. The stellar flux will then be intercepted during several seconds/minutes. Observation of the occulted star in time allows us to study the shape and size of the occulting object and its vicinity (ring, atmosphere or satellite). For the first time, two dense and narrow rings have been discovered on June 2013 around the biggest known Centaur Chariklo (body’s diameter: 250 km and rings diameter: 800 km). My work shows the 16 observed occultations by Chariklo and/or its rings since 2013. Those data are the only one available about this planetary system today. A first study of their structure and their geometry is conducted. Another part of my work was to study an occultation by the dwarf planet Haumea recorded on January 2017. It revealed the presence of a ring of radius ~2281 km around this tri-axial body. This discovery made Haumea the second body with a ring orbiting around except the four giant planets. This occultation allows us to derive the shape, size (1161x852x513 km) and density of the main body. This second discovery tends to show that rings in small planetary systems are more common that we thought. The release of Gaia DR1 catalog in 2016 greatly improved our predictions of such occultations. In the forthcoming years, efforts will be made on detailed and localized studies of Chariklo’s and Haumea’s rings, but also on search for other small rings systems in order to better understand the origins and the evolution mechanisms of such systems
Griggs, Erin R. "Analyses for a Modernized GNSS Radio Occultation Receiver." Thesis, University of Colorado at Boulder, 2015. http://pqdtopen.proquest.com/#viewpdf?dispub=3704709.
Full textGlobal Navigation Satellite System (GNSS) radio occultation (RO) is a remote sensing technique that exploits existing navigation signals to make global, real-time observations of the Earth's atmosphere. A specialized RO receiver makes measurements of signals originating from a transmitter onboard a GNSS spacecraft near the Earth's horizon. The radio wave is altered during passage through the Earth's atmosphere. The changes in the received signals are translated to the refractivity characteristics of the intervening medium, which enable the calculation of atmospheric pressure, temperature, and humidity. Current satellite missions employing GNSS RO have provided invaluable and timely information for weather and climate applications. Existing constellations of occultation satellites, however, are aging and producing fewer quality measurements. Replacement fleets of RO satellites are imperative to sustain and improve the global coverage and operational impact achieved by the current generation of RO satellites. This dissertation describes studies that facilitate the development of next generation RO receivers and satellite constellations. Multiple research efforts were conducted that aim to improve the quantity and quality of measurements made by a future satellite-based RO collection system. These studies range in magnitude and impact, and begin with a receiver development study using ground-based occultation data. Future RO constellations and collection opportunities were simulated and autonomous occultation prediction and scheduling capabilities were implemented. Finally, a comprehensive study was conducted to characterize the stability of the GNSS atomic frequency standards. Oscillator stability for a subset of satellites in the GNSS was found to be of insufficient quality at timescales relevant to RO collections and would degrade the atmospheric profiling capabilities of an RO system utilizing these signals. Recommendations for a high-rate clock correction network are proposed, which provides significant improvement to the fractional errors in the derived refractivity, pressure, and temperature values caused by the oscillator instabilities.
Hilbert, Bryan (Bryan Nathaniel) 1977. "Stellar occultation lightcurve modeling for elliptical occulting bodies." Thesis, Massachusetts Institute of Technology, 2001. http://hdl.handle.net/1721.1/54444.
Full textIncludes bibliographical references (leaf 41).
We present a new method of calculating model lightcurves for stellar occultations by the Jovian planets. We model the occulting planet as a three-dimensional body of non-zero ellipticity, and define two ellipses of intersection with the body which dictate the appearance of the lightcurve. These include the visible-limb plane ellipse, which is the observed figure of the body as seen in the sky, and the line-of-sight ellipse, which contains the line of sight to the occulted star, and is the plane in which the starlight is refracted. The observed stellar flux during the occultation is primarily dictated by the ellipticity and subsequent radius of curvature of the instantaneous ellipse in the line-of-sight plane. This new method is applied to several test cases, as well as to the Jovian occultation of HIP9369 on 10 October 1999. Lightcurves generated by this model are compared to identical situations using the method published in Hubbard et al. (1997), showing that the Hubbard model works well for low-latitude occultations, but fails at higher latitudes. In the case of the high-latitude Jovian occultation, the best-fit lightcurve, produced from this new method, yielded a half-light equatorial radius of 71,343±1.2 km with a scale height of 19.25±0.5km, and an isothermal temperature of 139K. The same data, fit using a lightcurve generated by the method described in Hubbard et al. (1997), resulted in a half-light equatorial radius of 71,819km with a scale height of 17.9km with errors comparable to the previous fit, resulting in an isothermal temperature of 129K. Lightcurves are numerically generated for an ellipsoidal planet and, for comparison, an approximation to the ellipsoidal case consisting of a sphere with radius equal to the radius of curvature of the ellipsoid at the half-light point. We find that in the case of an occultation where the line-of-sight ellipticity does not vary, that the radius of curvature approximation matches the ellipsoidal planet lightcurve to within 0.007%. For an oblique occultation however, the line-of-sight ellipticity varies, and the approximation, using only a single radius of curvature sphere, is only good to about 1%. As a result, we find that using a model such as that presented in Baum and Code (1953) to fit the lightcurve of an ellipsoidal planet can return values for half-light radius (after accounting for the distance between the center of curvature and the center of the body) which may match the local distance to the center of the ellipsoid to a fraction of a percent, while returning values of scale height which may be in error by several percent. Test cases are also then put through numerical inversions, to obtain temperature versus pressure profiles. Test cases with spherical planets return temperature profiles that match those used to create the lightcurves, while test cases with ellipsoidal planets return temperature profiles which can differ from the input temperatures by tens of degrees, assuming a constant local gravity over the course of the occultation.
by Bryan Hilbert.
S.M.
Lange, Martin, and Christoph Jacobi. "Analysis of gravity waves from radio occultation measurements." Universitätsbibliothek Leipzig, 2017. http://nbn-resolving.de/urn:nbn:de:bsz:15-qucosa-217072.
Full textAtmosphärische Schwerewellen führen im Höhenbereich 10-30 km zu periodischen Störungendes Hintergrundtemperaturfeldes in der Größenordnung von 2-3 K, die in Temperaturprofilen aus Radiookkultationsmessungen aufgelöst werden. Aufgrund der sphärischen Symmetrieannahme im Retrievalverfahren und durch die niedrige horizontale Auflösung des Messverfahrens werden Phasenverschiebungen und Dämpfung der Amplitude verursacht, die zu beachtlichen Fehlern bei den abgeleiteten Temperaturen führen. Der Einfluss der geometrischen Wellenparameter und der Messgeometrie auf ebene Schwerewellen im Bereich 100-1000 km horizontale und 1-10 km vertikale Wellenlänge wird untersucht mit einem 2D-Modell, dass sich auf ein Gebiet von ±1000 km um den Tangentenpunkt und von 10-50 km in der Höhe erstreckt. Die Untersuchung zeigt, dass mit Radiookkultationsmessungen mehr als 90% der simulierten Wellen aufgelöst werden und mehr als 50% mit Amplituden oberhalb von 90% der ursprünglichen. Die geometrischen Parameter können jedoch nicht aus Einzelmessungen abgeleitet werden, da ein Signal zu verschiedenen Kombinationen von Wellenparametern und Sichtwinkel zugeordnet werden kann. Auch relativ kurze Wellen mit horizontalen Wellenlängen unterhalb von 200 km können korrekt in der Amplitude und Phase aufgelöst werden, falls die Neigung des Wellenvektors gegen die vertikale gering ist oder der Sichtwinkel des Empfängersatelliten in Richtung der Wellenberge ist
Lange, Martin, and Christoph Jacobi. "Analysis of gravity waves from radio occultation measurements." Wissenschaftliche Mitteilungen des Leipziger Instituts für Meteorologie ; 26 = Meteorologische Arbeiten aus Leipzig ; 7 (2002), S. 101-108, 2002. https://ul.qucosa.de/id/qucosa%3A15225.
Full textAtmosphärische Schwerewellen führen im Höhenbereich 10-30 km zu periodischen Störungendes Hintergrundtemperaturfeldes in der Größenordnung von 2-3 K, die in Temperaturprofilen aus Radiookkultationsmessungen aufgelöst werden. Aufgrund der sphärischen Symmetrieannahme im Retrievalverfahren und durch die niedrige horizontale Auflösung des Messverfahrens werden Phasenverschiebungen und Dämpfung der Amplitude verursacht, die zu beachtlichen Fehlern bei den abgeleiteten Temperaturen führen. Der Einfluss der geometrischen Wellenparameter und der Messgeometrie auf ebene Schwerewellen im Bereich 100-1000 km horizontale und 1-10 km vertikale Wellenlänge wird untersucht mit einem 2D-Modell, dass sich auf ein Gebiet von ±1000 km um den Tangentenpunkt und von 10-50 km in der Höhe erstreckt. Die Untersuchung zeigt, dass mit Radiookkultationsmessungen mehr als 90% der simulierten Wellen aufgelöst werden und mehr als 50% mit Amplituden oberhalb von 90% der ursprünglichen. Die geometrischen Parameter können jedoch nicht aus Einzelmessungen abgeleitet werden, da ein Signal zu verschiedenen Kombinationen von Wellenparametern und Sichtwinkel zugeordnet werden kann. Auch relativ kurze Wellen mit horizontalen Wellenlängen unterhalb von 200 km können korrekt in der Amplitude und Phase aufgelöst werden, falls die Neigung des Wellenvektors gegen die vertikale gering ist oder der Sichtwinkel des Empfängersatelliten in Richtung der Wellenberge ist.
Books on the topic "Occultation de la violence"
Steiner, Andrea, Barbara Pirscher, Ulrich Foelsche, and Gottfried Kirchengast, eds. New Horizons in Occultation Research. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00321-9.
Full textMauldin, L. E. Halogen occultation experiment integrated test plan. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1986.
Find full textBuglia, James J. Photon counts from stellar occultation sources. [Washington, DC]: National Aeronautics and Space Administration, Scientific and Technical Information Office, 1987.
Find full textHarvey, Gale A. Halogen Occultation Experiment (HALOE) optical filter characterization. Hampton, Va: Langley Research Center, 1989.
Find full textBernath, Peter F. The Atmospheric Chemistry Experiment ACE at 10: A solar occultation anthology. Hampton, Virginia, USA: A. Deepak Publishing, a Division of Science and Technology Corporation, 2013.
Find full textWeinreb, Michael P. Balloon-based infrared solar occultation measurements of stratospheric O, HO, HNO, and CFC1. Washington, D.C: National Environmental Satellite, Data, and Information Service, 1987.
Find full textWeinreb, Michael P. Balloon-based infrared solar occultation measurements of stratospheric O, HO, HNO, and CFC1. Washington, D.C: National Environmental Satellite, Data, and Information Service, 1987.
Find full textLangwith, Jacqueline. Violence. Detroit, MI: Greenhaven Press, 2010.
Find full textVaze, Vrunda. Violence. Pune: Aalochana, 2007.
Find full textJacqueline, Langwith, ed. Violence. Detroit, MI: Greenhaven Press, 2010.
Find full textBook chapters on the topic "Occultation de la violence"
Georgoudi, Stella. "L’«occultation de la violence» dans le sacrifice grec: données anciennes, discours modernes." In Bibliothèque de l'Ecole des Hautes Etudes, Sciences Religieuses, 115–47. Turnhout: Brepols Publishers, 2005. http://dx.doi.org/10.1484/m.behe-eb.4.00023.
Full textRouan, Daniel. "Occultation." In Encyclopedia of Astrobiology, 1751–52. Berlin, Heidelberg: Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_4011.
Full textRouan, Daniel. "Occultation." In Encyclopedia of Astrobiology, 1160–61. Berlin, Heidelberg: Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-11274-4_4011.
Full textRouan, Daniel. "Occultation." In Encyclopedia of Astrobiology, 1. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_4011-2.
Full textDyson, Freeman J. "Occultation Astronomy." In Observatories in Earth Orbit and Beyond, 413–15. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-011-3454-5_55.
Full textAo, Chi O. "GPS, Occultation Systems." In Encyclopedia of Remote Sensing, 264–68. New York, NY: Springer New York, 2014. http://dx.doi.org/10.1007/978-0-387-36699-9_61.
Full textBlick, Christian, and Sarah Eberle. "Radio Occultation via Satellites." In Handbook of Geomathematics, 1089–125. Berlin, Heidelberg: Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-642-54551-1_100.
Full textBlick, Christian, and Sarah Eberle. "Radio Occultation via Satellites." In Handbook of Geomathematics, 1–33. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27793-1_100-1.
Full textBlick, Christian, and Sarah Eberle. "Radio Occultation via Satellites." In Handbook of Geomathematics, 1–33. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27793-1_100-2.
Full textMillis, Robert L. "Occultation Studies with Small Telescopes." In Instrumentation and Research Programmes for Small Telescopes, 199–211. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-010-9433-7_36.
Full textConference papers on the topic "Occultation de la violence"
Demina, Natalya. "ANALYSIS OF 430322 LUNAR OCCULTATION." In 17th International Multidisciplinary Scientific GeoConference SGEM2017. Stef92 Technology, 2017. http://dx.doi.org/10.5593/sgem2017/62/s28.113.
Full textMoeller, R. "Atmospheric Occultation Student (ATOS) experiment." In 38th Aerospace Sciences Meeting and Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2000. http://dx.doi.org/10.2514/6.2000-9.
Full textDu, Qifei, Yueqiang Sun, Shijing Wang, Guangwu Zhu, Peng Tao, Zhengting Liu, and Weihua Bai. "Dual-band GPS occultation receiver." In Seventh International Symposium on Instrumentation and Control Technology, edited by Jiancheng Fang and Zhongyu Wang. SPIE, 2008. http://dx.doi.org/10.1117/12.807139.
Full textZin, A., S. Zago, E. Mangolini, S. Landenna, L. Marradi, R. Notarpietro, S. Radicella, B. Nava, and V. Catalano. "The ROSA radio occultation project." In 2012 6th ESA Workshop on Satellite Navigation Technologies (Navitec 2012) & European Workshop on GNSS Signals and Signal Processing. IEEE, 2012. http://dx.doi.org/10.1109/navitec.2012.6423096.
Full textBellini, Rosanna, Jay Rainey, Andrew Garbett, and Pamela Briggs. "Vocalising Violence." In C&T 2019: The 9th International Conference on Communities & Technologies - Transforming Communities. New York, NY, USA: ACM, 2019. http://dx.doi.org/10.1145/3328320.3328405.
Full textGordley, Larry L., R. Earl Thompson, Guy M. Beaver, James M. Russell III, Lance E. Deaver, and Mark E. Hervig. "Impact of Pinatubo aerosol extinction on the Halogen Occultation Experiment (HALOE) infrared occultation measurements." In SPIE's 1994 International Symposium on Optics, Imaging, and Instrumentation, edited by Jinxue Wang and Paul B. Hays. SPIE, 1994. http://dx.doi.org/10.1117/12.187596.
Full textSweeney, David, Chi Ao, Panagiotis Vergados, Nilton Renno, David Kass, and German Martinez. "Enabling Mars Radio Occultation by Smallsats." In 2021 IEEE Aerospace Conference. IEEE, 2021. http://dx.doi.org/10.1109/aero50100.2021.9438147.
Full textLiu, Congliang, Gottfried Kirchengast, Yueqiang Sun, Qifei Du, Weihua Bai, Veronika Proschek, Xianyi Wang, et al. "Study on LEO-LEO microwave occultation." In 2017 IEEE International Geoscience and Remote Sensing Symposium (IGARSS). IEEE, 2017. http://dx.doi.org/10.1109/igarss.2017.8127009.
Full textRussell III, James M. "Overview of the halogen occultation experiment." In Orlando '91, Orlando, FL, edited by James L. McElroy and Robert J. McNeal. SPIE, 1991. http://dx.doi.org/10.1117/12.46653.
Full textKennedy, Traci M., Rosanne M. Jocson, Francheska Alers-Rojas, and Rosario Ceballo. "76 Preventing the cycle of violence: community violence exposure and attitudes toward violence among latino adolescents." In SAVIR 2017. BMJ Publishing Group Ltd, 2017. http://dx.doi.org/10.1136/injuryprev-2017-042560.76.
Full textReports on the topic "Occultation de la violence"
Miller, Richard, M. Ajello, J. F. Beacom, Peter Forbes Bloser, Adam Burrows, Christopher Lee Fryer, J. O. Goldsten, et al. Ex Luna, Scientia: The Lunar Occultation eXplorer (LOX). Office of Scientific and Technical Information (OSTI), July 2019. http://dx.doi.org/10.2172/1544647.
Full textBarclay, Keith A. Ethnic Violence in Moldolva. Fort Belvoir, VA: Defense Technical Information Center, May 2002. http://dx.doi.org/10.21236/ada403991.
Full textAlesina, Alberto, Salvatore Piccolo, and Paolo Pinotti. Organized Crime, Violence, and Politics. Cambridge, MA: National Bureau of Economic Research, March 2016. http://dx.doi.org/10.3386/w22093.
Full textCastro-Pantoja, John David, José Eduardo Gómez-González, Tatiana Mora-Arbelaez, Daniela Rodriguez-Novoa, and Laura Catalina Díaz-Barreto. Bancarization and Violence in Colombia. Bogotá, Colombia: Banco de la República, September 2018. http://dx.doi.org/10.32468/be.1052.
Full textAizer, Anna. Neighborhood Violence and Urban Youth. Cambridge, MA: National Bureau of Economic Research, February 2008. http://dx.doi.org/10.3386/w13773.
Full textMiguel, Edward, Sebastián Saiegh, and Shanker Satyanath. National Cultures and Soccer Violence. Cambridge, MA: National Bureau of Economic Research, April 2008. http://dx.doi.org/10.3386/w13968.
Full textWilliams, Phil, and Vanda Felbab-Brown. Drug Trafficking, Violence, and Instability. Fort Belvoir, VA: Defense Technical Information Center, April 2012. http://dx.doi.org/10.21236/ada560718.
Full textRogers, Patrick. Domestic Violence and Other Poems. Portland State University Library, January 2000. http://dx.doi.org/10.15760/etd.6345.
Full textBailey, Corin. Crime and Violence in Barbados: IDB Series on Crime and Violence in the Caribbean. Inter-American Development Bank, June 2016. http://dx.doi.org/10.18235/0000332.
Full textHarriott, Anthony D., and Marlyn Jones. Crime and Violence in Jamaica: IDB Series on Crime and Violence in the Caribbean. Inter-American Development Bank, June 2016. http://dx.doi.org/10.18235/0000333.
Full text