Search results for "Individual"
showing 10 items of 1227 documents
Minäkäsitys individualistisessa ja kollektivistisessa kulttuurissa
2001
Study of social self-concept invariance in physical activity individual and collective practitioners
2019
Este estudio tiene como objetivo explorar la invariancia configural, métrica y escalar en función del sexo y de la práctica de actividad física colectiva del AUSO de Fernández-Zabala et al. (2016) y comparar las puntuaciones obtenidas por los subgrupos. La muestra fue de 278 estudiantes universitarios (M = 21. 16 años; DT = 19. 238) divididos de forma equivalente en función del género y de la práctica de actividad física. Tras comprobar la invariancia estricta en ambos supuestos, los resultados demuestran que no existen diferencias significativas en ninguno de los factores en función del sexo, pero sí en función de la práctica de actividad física: aquellos estudiantes que realizan actividad…
Soda noteikšanas teorētiskie un praktiskie aspekti
2020
Vienlaikus ar humānisma ideju un cilvēktiesību principu ieviešanu sodu noteikšanā arvien lielāku nozīmi iegūst arī nepieciešamība nodrošināt efektīvu noziedzīgu nodarījumu novēršanu. Bakalaura darba mērķis ir apzināt soda noteikšanas vispārīgo principu un noteikumu, kas attiecas uz soda noteikšanu par vairākiem noziedzīgiem nodarījumiem, regulējuma un prakses problēmjautājumus. Darba uzdevumi ir izpētīt soda un ar to saistītā taisnīguma izpratnes vēsturisko attīstību, soda būtību un mērķi, soda noteikšanas vispārīgo principu un to ietekmējošo apstākļu regulējumu un piemērošanas praksi, soda noteikšanas par vairākiem noziedzīgiem nodarījumiem regulējumu un piemērošanas praksi. Darba rezultāt…
Personas tiesību ierobežošana Latvijā un Eiropā un ar to saistītā problemātika
2017
Darbā pētīta taisnīga soda un tā atvasināto principu izcelsme un saturs. Darbā analizēta soda individualizācijas ietekme uz soda noteikšanu minimālajām prasībām. Maģistra darba ietvaros izvērtēta divu Krimināllikumā pastāvošu institūtu – sodāmības un personas tiesību ierobežošanas atbilstība taisnīga soda pamatprincipiem. Darbā pētīta aktuālākā personas tiesību ierobežošanas un sodāmības problemātika un šo institūtu atbilstība Satversmes tiesas un Eiropas Cilvēktiesību tiesas judikatūrai. Darbā secināts un izvirzītas tēzes, ka sodāmību un atsevišķi personas tiesību ierobežošanas sodi tiek noteikti, neizvērtējot to atbilstību taisnīgu soda noteikšanas pamatprincipiem, tādēļ likumdevējam šie …
Covid politics : Morality and Solidarities in a State of Exception
2021
Development of microfluidics for sorting of carbon nanotubes
2018
Sorting of carbon nanotubes by their chirality is the current bottleneck in the way to their broad employment based on their exceptional electronic and optical properties. Despite the extensive effort, there is no known method, which would result in really pure chirality ensembles. Previously reported sorting protocols result in enrichment rather than in sorting, alter electronic structure, and suffer from low yield. This is mostly due to the statistical approach, where the nanotubes with mixed chiralities are treated as a set. In this thesis, we propose a new sorting technique based on nanotube-by-nanotube compartmelization, characterization, and sorting in a continuously running droplet-b…
Computational Rationality as a Theory of Interaction
2022
Funding Information: This work was funded by the Finnish Center for AI and Academy of Finland (“BAD” and “Human Automata”). We thank our reviewers, Xiuli Chen, Joerg Mueller, Christian Guckelsberger, Sebastiaan de Peuter, Samuel Kaski, Pierre-Alexandre Murena, Antti Keuru-lainen, Suyog Chandramouli, and Roderick Murray-Smith for their comments. Publisher Copyright: © 2022 ACM. How do people interact with computers? This fundamental question was asked by Card, Moran, and Newell in 1983 with a proposition to frame it as a question about human cognition - in other words, as a matter of how information is processed in the mind. Recently, the question has been reframed as one of adaptation: how …
Coronal properties of active G-type stars in different evolutionary phases
2005
We report on the analysis of XMM-Newton observations of three G-type stars in very different evolutionary phases: the "weak-line" T Tauri star HD 283572, the Zero Age Main Sequence star EK Dra and the Hertzsprung-gap giant star 31 Corn. The X-ray luminosities of the three stars are all in the range 10(30) - 10(31) erg/s. We compare the Emission Measure Distributions of these bright sources, derived from high-resolution X-ray spectra, as well as the pattern of elemental abundances vs. First Ionization Potential (FIP). The results of our analysis suggest that the coronae of these stars are very similar in terms of dominant coronal magnetic structures, in spite of differences in their evolutio…
Stochastic gravito-inertial modes discovered by CoRoT in the hot Be star HD 51452
2012
International audience; Context. Be stars are rapidly rotating stars with a circumstellar decretion disk. They usually undergo pressure and/or gravity pulsation modes excited by the κ-mechanism, i.e. an effect of the opacity of iron-peak elements in the envelope of the star. In the Milky Way, p-modes are observed in stars that are hotter than or equal to the B3 spectral type, while g-modes are observed at the B2 spectral type and cooler. Aims. We observed a B0IVe star, HD 51452, with the high-precision, high-cadence photometric CoRoT satellite and high-resolution, ground-based HARPS and SOPHIE spectrographs to study its pulsations in great detail. We also used the lower resolution spectra a…
X-ray emission from the old CTTS MP Muscae
2007
We study the properties of X-ray emitting plasma of MP Mus, an old classical T Tauri star. XMM-Newton/RGS spectra allow us to measure the plasma electron density, which probes whether X-ray emission is produced in the accretion process. X-ray emission from MP Mus originates from high density cool plasma but a hot flaring component is also present, suggesting that both coronal magnetic activity and accretion contribute to the observed X-ray emission. From the soft part of the X-ray emission from MP Mus, mostly produced by plasma heated in the accretion shock, we derive the accretion parameters and the characteristics of the shock-heated plasma.