21 resultados para Criminal histories.
Resumo:
La dimensión real de la actual política criminal española carece de adecuados niveles de racionalidad, entre sus múltiples causas, podemos mencionar el fenómeno de la creciente dinámica punitivista, la ausencia de una adecuada cultura de evaluación, el menosprecio a la criminología, la escasa consideración de los responsables políticos hacia las opiniones expertas de la dogmática, y la constante indiferencia de ésta hacia la realidad que debe enfrentar. Se configura así un decepcionante panorama donde la política criminal real aparece como carente de una sólida base empírica. La dimensión teórica de la política criminal, no puede soslayar el aporte de las investigaciones criminológicas, ya que aquellos tendrían la virtualidad de ser condición necesaria aunque no suficiente de la utilización racional del sistema punitivo. Hay que optar por una reducción de la privación de libertad y promover otras sanciones en cuyo contenido se armonicen los conceptos de incapacitación y responsabilización. Además, se requiere el desarrollo de una victimología que se dirija a inhibir los impulsos punitivos de las víctimas en función de orientar la política criminal hacia una cultura jurídica reparatoria que enfrente la actual expansión del derecho penal.
Resumo:
We present a sample of three large near-relativistic (>50 keV) electron events observed in 2001 by both the ACE and the Ulysses spacecraft, when Ulysses was at high-northern latitudes (>60◦) and close to 2 AU. Despite the large latitudinal distance between the two spacecraft, electrons injected near the Sun reached both heliospheric locations. All three events were associated with large solar flares, strong decametric type II radio bursts and accompanied by wide (>212◦) and fast (>1400 km s−1) coronal mass ejections (CMEs). We use advanced interplanetary transport simulations and make use of the directional intensities observed in situ by the spacecraft to infer the electron injection profile close to the Sun and the interplanetary transport conditions at both low and high latitudes. For the three selected events, we find similar interplanetary transport conditions at different heliolatitudes for a given event, with values of the mean free path ranging from 0.04 AU to 0.27 AU. We find differences in the injection profiles inferred for each spacecraft. We investigate the role that sector boundaries of the heliospheric current sheet (HCS) have on determining the characteristics of the electron injection profiles. Extended injection profiles, associated with coronal shocks, are found if the magnetic footpoints of the spacecraft lay in the same magnetic sector as the associated flare, while intermittent sparse injection episodes appear when the spacecraft footpoints are in the opposite sector or a wrap in the HCS bounded the CME structure.
Resumo:
In recent years, new analytical tools have allowed researchers to extract historical information contained in molecular data, which has fundamentally transformed our understanding of processes ruling biological invasions. However, the use of these new analytical tools has been largely restricted to studies of terrestrial organisms despite the growing recognition that the sea contains ecosystems that are amongst the most heavily affected by biological invasions, and that marine invasion histories are often remarkably complex. Here, we studied the routes of invasion and colonisation histories of an invasive marine invertebrate Microcosmus squamiger (Ascidiacea) using microsatellite loci, mitochondrial DNA sequence data and 11 worldwide populations. Discriminant analysis of principal components, clustering methods and approximate Bayesian computation (ABC) methods showed that the most likely source of the introduced populations was a single admixture event that involved populations from two genetically differentiated ancestral regions - the western and eastern coasts of Australia. The ABC analyses revealed that colonisation of the introduced range of M. squamiger consisted of a series of non-independent introductions along the coastlines of Africa, North America and Europe. Furthermore, we inferred that the sequence of colonisation across continents was in line with historical taxonomic records - first the Mediterranean Sea and South Africa from an unsampled ancestral population, followed by sequential introductions in California and, more recently, the NE Atlantic Ocean. We revealed the most likely invasion history for world populations of M. squamiger, which is broadly characterized by the presence of multiple ancestral sources and non-independent introductions within the introduced range. The results presented here illustrate the complexity of marine invasion routes and identify a cause-effect relationship between human-mediated transport and the success of widespread marine non-indigenous species, which benefit from stepping-stone invasions and admixture processes involving different sources for the spread and expansion of their range.
Resumo:
We present a sample of three large near-relativistic (>50 keV) electron events observed in 2001 by both the ACE and the Ulysses spacecraft, when Ulysses was at high-northern latitudes (>60°) and close to 2 AU. Despite the large latitudinal distance between the two spacecraft, electrons injected near the Sun reached both heliospheric locations. All three events were associated with large solar flares, strong decametric type II radio bursts and accompanied by wide (>212°) and fast (>1400 km s-1) coronal mass ejections (CMEs). We use advanced interplanetary transport simulations and make use of the directional intensities observed in situ by the spacecraft to infer the electron injection profile close to the Sun and the interplanetary transport conditions at both low and high latitudes. For the three selected events, we find similar interplanetary transport conditions at different heliolatitudes for a given event, with values of the mean free path ranging from 0.04 AU to 0.27 AU. We find differences in the injection profiles inferred for each spacecraft. We investigate the role that sector boundaries of the heliospheric current sheet (HCS) have on determining the characteristics of the electron injection profiles. Extended injection profiles, associated with coronal shocks, are found if the magnetic footpoints of the spacecraft lay in the same magnetic sector as the associated flare, while intermittent sparse injection episodes appear when the spacecraft footpoints are in the opposite sector or a wrap in the HCS bounded the CME structure.
Resumo:
El present treball pretén oferir al lector un estudi sobre el nou Codi Processal Penal com esborrany d'avantprojecte de Llei, realitzant un anàlisis dels aspectes més rellevants i innovadors que introdueix el citat Codi així com l’adaptació d’aquests a les realitats socials de cada temps. A més, la idea per la qual neix el treball és analitzar les raons per les quals s’ha vist necessari i important realitzar una modificació total de la actual LECrim, estudiant la forma en què el legislador enfoca el nou Codi així com el seu contingut, destacant les principals diferències que conté l’actual LECrim amb aquelles que el nou Codi pretén instaurar.
Resumo:
El artículo se propone reflexionar sobre dos cuestiones: ¿la «novela de favela» es novela criminal? y ¿es posible detectar aspectos de género en las «novelas de favela» de Patrícia Melo? En nuestra opinión, la «novela de favela» es literatura de la violencia, para ser más exactos de la representación de la violencia, pero, aunque a veces la frontera sea muy tenue, no responde a los paradigmas de la novela criminal. Por otra parte, y a partir del análisis de la construcción de los personajes Máiquel y Reizinho (O Matador e Inferno), creemos que sí es posible afirmar un sesgo de género en los textos de Patrícia Melo.