Relevant bibliographies by topics / Action Stars

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Action Stars'

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

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Journal articles on the topic "Action Stars"

1

Gray, David F. "Dynamo Action in Evolved Stars." International Astronomical Union Colloquium 130 (1991): 336–41. http://dx.doi.org/10.1017/s0252921100079872.

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AbstractEvolved stars tell us a great deal about dynamos. The granulation boundary shows us where solar-type convection begins. Since activity indicators also start at this boundary, it is a good bet that solar-type convection is an integral part of dynamo activity for all stars. The rotation boundary tells us where the magnetic fields of dynamos become effective in dissipating angular momentum, and rotation beyond the boundary tells us the limiting value needed for a dynamo to function. The observed uniqueness of rotation rates after the rotation boundary is crossed can be understood through the rotostat hypothesis. Quite apart from the reason for the unique rotation rate, its existence can be used to show that magnetic activity of giants is concentrated to the equatorial latitudes, as it is in the solar case. The coronal boundary in the H-R diagram is probably nothing more than a map of where rotation becomes too low to sustain dynamo activity.
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Aerts, Conny. "Massive Star Asteroseismology in Action." Proceedings of the International Astronomical Union 9, S307 (June 2014): 154–64. http://dx.doi.org/10.1017/s1743921314006644.

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AbstractAfter highlighting the principle and power of asteroseismology for stellar physics, we briefly emphasize some recent progress in this research for various types of stars. We give an overview of high-precision high duty-cycle space photometry of OB-type stars. Further, we update the overview of seismic estimates of stellar parameters of OB dwarfs, with specific emphasis on convective core overshoot. We discuss connections between pulsational, rotational, and magnetic variability of massive stars and end with future prospects for asteroseismology of evolved OB stars.
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Augustson, Kyle C., Allan S. Brun, and Juri Toomre. "Convection and dynamo action in B stars." Proceedings of the International Astronomical Union 6, S271 (June 2010): 361–62. http://dx.doi.org/10.1017/s1743921311017790.

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AbstractMain-sequence massive stars possess convective cores that likely harbor strong dynamo action. To assess the role of core convection in building magnetic fields within these stars, we employ the 3-D anelastic spherical harmonic (ASH) code to model turbulent dynamics within a 10 M⊙ main-sequence (MS) B-type star rotating at 4 Ω⊙. We find that strong (900 kG) magnetic fields arise within the turbulence of the core and penetrate into the stably stratified radiative zone. These fields exhibit complex, time-dependent behavior including reversals in magnetic polarity and shifts between which hemisphere dominates the total magnetic energy.
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Bonanno, A., L. Rezzolla, and V. Urpin. "Mean-field dynamo action in protoneutron stars." Astronomy & Astrophysics 410, no. 3 (November 2003): L33—L36. http://dx.doi.org/10.1051/0004-6361:20031459.

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Palouš, Jan, Jim Dale, Richard Wünsch, Sergiy Silich, Guillermo Tenorio-Tagle, and Anthony Whitworth. "Action of Winds Inside and Outside of Star Clusters." Proceedings of the International Astronomical Union 6, S270 (May 2010): 267–74. http://dx.doi.org/10.1017/s1743921311000494.

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AbstractThe feedback form pre-main sequence and young stars influences their vicinity. The stars are formed in clusters, which implies that the winds of individual stars collide with each other. Inside of a star cluster, winds thermalize a fraction of their kinetic energy, forming a very hot medium able to escape from the cluster in the form of a large-scale wind. Outside of the cluster, the cluster wind forms a shock front as it interacts with the ambient medium which is accreted onto the expanding shell. A variety of instabilities may develop in such shells, and in some cases they fragment, triggering second generation of star formation. However, if the cluster surpasses a certain mass (depending on the radius and other parameters) the hot medium starts to be thermally unstable even inside of the cluster, forming dense warm clumps. The formation of next generations of stars may start if the clumps are big enough to self-shield against stellar radiation creating cold dense cores.
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Browning, Matthew K. "Simulations of Dynamo Action in Fully Convective Stars." Astrophysical Journal 676, no. 2 (April 2008): 1262–80. http://dx.doi.org/10.1086/527432.

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F. Dorch, S. B. "A Magnetic Betelgeuse? Numerical Simulations of Non-Linear Dynamo Action." Symposium - International Astronomical Union 219 (2004): 656–60. http://dx.doi.org/10.1017/s0074180900182701.

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Betelgeuse is an example of a cool supergiant displaying brightness fluctuations and irregular surface structures. Simulations by Freytag, Steffen, & Dorch (2002) of the convective envelope of the star have shown that the fluctuations in the star's luminosity may be caused by giant cell convection. A related question regarding the nature of Betelgeuse and supergiants in general is whether these stars may be magnetically active. If so, that may in turn also contribute to their variability. By performing detailed numerical simulations, I find that both linear kinematic and non-linear dynamo action are possible and that the non-linear magnetic field saturates at a value somewhat below equipartition: in the linear regime there are two modes of dynamo action.
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Augustson, Kyle C., Allan Sacha Brun, and Juri Toomre. "DYNAMO ACTION AND MAGNETIC CYCLES IN F-TYPE STARS." Astrophysical Journal 777, no. 2 (October 23, 2013): 153. http://dx.doi.org/10.1088/0004-637x/777/2/153.

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Turner, Brandon D. "Changing the Stars: Astrocytes Adapt to Coordinate Action Flexibility." Biological Psychiatry 89, no. 11 (June 2021): e59-e60. http://dx.doi.org/10.1016/j.biopsych.2021.03.028.

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Sanderson, Robyn E., Amina Helmi, and David W. Hogg. "Action-space clustering of tidal streams to map the Galactic potential." Proceedings of the International Astronomical Union 9, S298 (May 2013): 207–12. http://dx.doi.org/10.1017/s1743921313006388.

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AbstractGiven a parametrized model of the Galactic potential, the best-fit parameters can be obtained by maximizing the Kullback-Leibler divergence of the action distribution of a set of stars initially clustered in action space (e.g. stars in tidal streams). This method will allow us to map the Milky Way's gravitational potential by simultaneously fitting multiple tidal streams without requiring stream membership information. With 20 streams of at least 20 stars each, including observational errors consistent with predictions for Gaia, this technique recovers the input potential parameters to a precision of 10-60% and an accuracy of 10%. With all the observed streams in our mock stellar halo (about 40) that fit the error criteria, the precision improves to 10%.
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Dissertations / Theses on the topic "Action Stars"

1

Augustson, K. C. "Convection and Dynamo Action in Massive Stars." Thesis, University of Colorado at Boulder, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=3607276.

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Contact between numerical simulations and observations of stellar magnetism is sought, with an emphasis on those stars that are the most readily observed and those that may have magnetic activity cycles: the Sun, F-type, and B-type stars. Two approaches are taken in studying stellar dynamos and dynamics, utilizing three-dimensional MHD simulations run on massively parallel supercomputers with the full spherical geometry and employing a new compressible code in the spherical wedge geometry. A 3-D MHD simulation of the solar dynamo that utilizes the Anelastic Spherical Harmonic (ASH) code is presented. This simulation self-consistently exhibits four prominent aspects of solar magnetism: activity cycles, polarity cycles, the equatorward field migration, and grand minima. The ASH framework and this simulation's ability to capture many aspects of the solar dynamo represent a first step toward a more complete model of the Sun's global-scale magnetic activity and its cycles. The dynamics and dynamos of F-type stars are studied through global-scale ASH simulations, with significant contact made between the observed differential rotation and magnetic cycle periods of these stars and those achieved in the simulations. Separately, ASH simulations of core convection in the massive B-type stars show that generation of superequipartition magnetic fields with peak strengths above 1 MG is possible within their cores, which has implications for the evolution of these stars as well as for the properties of their remnants. The internal waves excited by overshooting convection and rotation in these star's radiative exteriors are assessed for their asteroseismic signatures. The results of 3-D compressive MHD simulations of the solar near-surface shear layer with the Compressible Spherical Segment (CSS) code are shown, with such layers arising in the coupled dynamics of ASH and CSS as well as in a more rapidly rotating, thin convective envelope of an F-type star.

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Petrov, Pavel. "Effect of Curvature Squared Corrections to Gravitational Action on Viscosity-to-Entropy Ratio of the Dual Gauge Theory." Thesis, Harvard University, 2012. http://dissertations.umi.com/gsas.harvard:10549.

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In this thesis we study the properties of strongly-coupled large-N conformal field theories (CFT’s) using AdS/CFT correspondence. Chapter 1 serves as an introduction. In Chapter 2 we study the shear viscosity of strongly-coupled large-N conformal field theories. We find that it is affected by \(R^2\) corrections to the AdS action and present an example of 4D theory in which the the conjectured universal lower bound on viscosity-to-entropy ratio \(\eta/s > 1/4 \pi\) is violated by 1/N corrections. This fact proves that there is no universal lower bound of \(1/4 \pi\) on viscosity-to-entropy ratio and may be relevant for the studies of QCD quark-gluon plasma for which this ratio is experimentally found to be close to \(1/4 \pi\). In Chapter 3 we study the formation of the electron star in 4D AdS space. We show that in a gravity theory with charged fermions a layer of charged fermion fluid may form at a finite distance from the charged black hole. We show that these “electron stars” are candidate gravity duals for strongly interacting fermion systems at finite density and finite temperature. Entropy density for such systems scales as \(s \sim T^{2/z}\) at low temperatures as expected from IR criticality of electron stars solutions.
Physics
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Scott, John F. "Theoretical atmospheres of stars in the broad line regions of active galaxies /." The Ohio State University, 1987. http://rave.ohiolink.edu/etdc/view?acc_num=osu1487585645578035.

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Bingham, Dennis. "Male spectatorship and Hollywood star acting /." The Ohio State University, 1990. http://rave.ohiolink.edu/etdc/view?acc_num=osu1487684245465453.

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Nieding, Michael, and Brechtje Postema. "Degrowth: From Utopia to Reality : An action research approach to start the Degrowth dialogue." Thesis, Uppsala universitet, Företagsekonomiska institutionen, 2021. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-447345.

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How can an idea that critiques the global capitalist system persist? How can a concept that opposes growth as indicator of wealth gather more and more supporters inside and outside of academia? How can a radical theory that challenges almost any societal structure convince us that it is something we must pursue? The Degrowth movement is often referred to as utopia, and not without good reason, as it is a relatively new concept that certainly still has its flaws. This thesis aims to start the Degrowth dialogue outside the ivory tower of academia. We use qualitative data gained from five focus groups to determine which components of Degrowth need the most clarification to make a movement evolve into a genuine theory. Our findings, brought forward by engaged discussions during the focus groups, showed potential for improvements of the Degrowth theory in the areas of education, societal norms and values as well as governmental policies and regulations. These insights allowed us to more specifically address the ambiguities of degrowth and counter them with opinions from experts to make Degrowth more accessible.
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Ekdiha, Mohamed. "Actions bi-hamiltoniennes et star-produits sur une variété bi-hamiltonienne." Grenoble 2 : ANRT, 1987. http://catalogue.bnf.fr/ark:/12148/cb37604825w.

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Ekdiha, Mohamed. "Actions bi-hamiltoniennes et star-produits sur une variété bi-hamiltonnienne." Lyon 1, 1987. http://www.theses.fr/1987LYO11747.

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Dans le 1er chapitre nous etudions l'action hamiltonien ne d'un goupe de lie g sur une variete de jacobi (m. Lambda ,e) en donnant des exemples d'actions admettant des applications moments coadjoints equivariants. Dans le 2eme chapitre, nous etudions l'action d'un groupe de lie g, connexe sur une variete bi-hamiltonienne (m,lambda ,lambda ). L'homomorphisme r : tm -> tm associe a la structure (m,lambda ,lambda ) est un operateur de recursion pour les systemes dynamiques dx/dt = x::(m)(x) ou x::(m) est un champ fondamental de l'action de g sur (m,lambda ,lambda ). Le dernier chapitre est consacre a l'etude des *-produits sur la variete bi-hamiltonienne (m,lambda ,lambda ). Apres avoir donne un theoreme d'existence, nous determinons un lien entre les *-produits d'un point sur (m,lambda ,lambda ), (m,lambda ) et d'autre part sur (m,lambda ) dans un cas particulier de structures bi-hamiltonienne que nous appelons c-tangentiellement exacte. Enfin nous considerons une variete de poisson reguliere tangentiellement exacte et nous donnons une condition d'existence de *-produits tangentiels invariants par l'action d'un groupe de lie
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Eriksson, Joel, Niclas Krantz, and Jonas Ivarsson. "The strategic path in a creative start-up process : Action research within the fashion industry." Thesis, Jönköping University, JIBS, Business Administration, 2006. http://urn.kb.se/resolve?urn=urn:nbn:se:hj:diva-322.

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Baleg, Abd Almonam Abd Alsalam. "Synthesis and electrochemistry of novel conducting dendrimeric star copolymers on poly(propylene imine) dendrimer." Thesis, University of the Western Cape, 2011. http://etd.uwc.ac.za/index.php?module=etd&action=viewtitle&id=gen8Srv25Nme4_1288_1365583651.

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One of the most powerful aspects of conducting polymers is their ability to be nanostructured through innovative, synthetically manipulated, transformations, such as to tailor-make the polymers for specialized applications. In the exponentially increasing wide field of nanotechnology, some special attention is being paid to innovative hybrid dendrimer-core based polymeric smart materials. Star copolymers are a class of branched macromolecules having a central core with multiple linear polymer chains extending from the core. This intrinsic structural feature yields a unique 3D structure with extended conjugated linear polymer chains, resulting in star copolymers, which have higher ionic conductivities than their corresponding non-star conducting polymer counterparts. In this study an in-depth investigation was carried out into the preparation and characterization of specialized electronic &lsquo
smart materials&rsquo
. In particular, the preparation and characterization of novel conducting dendrimeric star copolymers which have a central poly(propylene imine) (PPI) dendrimer core with conducting polypyrrole (PPy) chains extending from the core was carried out. This involved, first, the preparation of a series of dendrimeric polypyrrole poly(propylene imine) star copolymers (PPI-co-PPy), using generations 1 to 4 (G1 to G4) PPI dendrimer precursors. The experimental approach involved the use of both chemical and electrochemical synthesis methods. The basic procedure involved a condensation reaction between the primary amine of a diamino functional PPI dendrimer surface and 2-pyrrole aldehyde, to afford the pyrrole functionalized PPI dendrimer (PPI-2Py). Polymerization of the intrinsically contained monomeric Py units situated within the dendrimer backbone was achieved via two distinctly different routes: the first involved chemical polymerization and the second was based on potentiodynamic oxidative electrochemical polymerization. The star copolymers were then characterized using various sophisticated analytical techniques, in-situ and ex-situ. Proton nuclear magnetic resonance spectroscopy (1HNMR) and Fourier transform infrared spectroscopy (FTIR) were used to determine the structures. Scanning electron microscopy (SEM) was used to determine the morphology. Themogravimetric analysis (TGA) was used to study the thermal stability of the prepared materials. X-ray diffraction analysis (XRD) was used to study the structural make-up of phases, crystallinity and amorphous content. Hall effect measurements were carried out to determine the electrical conductivity of the chemically prepared star copolymers. The PPI-co-PPy exhibited improved thermal stability compared to PPI-2Py, as confirmed by TGA. SEM results showed that the surface morphology of the functionalized dendrimer and star copolymer differed. The surface morphology of the chemically prepared star copolymers resembled that of a flaky, waxy material, compared to the ordered morphology of the electrochemically grown star copolymers, which resembled that of whelk-like helixes. In the case the electrochemically grown star copolymers, SEM images recorded at higher magnifications showed that the whelk-like helixes of the star copolymers were hollow tubes with openings at their tapered ends, and had an average base diameter of 2.0 &mu
m. X-ray diffraction analysis of the first generation star copolymer G1PPI-co-PPy revealed a broadly amorphous structure associated with PPy, and crystalline peaks for PPI. Cyclic voltammetry (CV), square wave voltammetry (SWV) and electrochemical impedance spectroscopy (EIS) techniques were used to study and model the electrochemical reactivity of the star copolymer materials. Electrochemical impedance spectroscopy data showed that the G1PPI-co-PPy exhibited slightly higher ionic conductivity than pristine PPy in lithium perchlorate. The second generation star copolymer G2PPI-co-PPy electrochemically deposited on a platinum (Pt) electrode had a lower electrochemical charge transfer resistance compared to electrodeposited polypyrrole (PPy) on a Pt electrode, and bare Pt. The decrease in charge transfer resistance was attributed to an increase in the conjugation length of the polymer as a result of the linking of the highly conjugated PPy to the PPI dendrimer. Bode impedimetric analysis indicated that G2PPI-co-PPI was a semiconductor, with a maximum phase angle shift of 45.3°
at 100 MHz. The star copolymer exhibited a 2- electron electrochemistry and a surface coverage of 99%. Results of Hall effect measurements showed that the star copolymer is a semiconducting material, having a conductivity of 0.7 S cm-1, in comparison to the 1.5 S cm-1 of PPy. To the best of my knowledge, these new star copolymers have not been reported in the open literature. Their properties make them potentially applicable for use in biosensors.

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Watson, Casey Richard. "The cosmological X-ray evolution of stars, AGN, and galaxies." The Ohio State University, 2006. http://rave.ohiolink.edu/etdc/view?acc_num=osu1148410557.

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Books on the topic "Action Stars"

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O'Brien, Sean. Vale of stars. San Francisco: JournalStone, 2012.

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The stars askew. New York, NY: Tor, 2016.

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Isaac Asimov. The stars, like dust. New York: Tor, 2008.

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Isaac Asimov. The Stars, Like Dust. London, UK: Grafton HarperCollins UK, 1986.

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Isaac Asimov. The Stars, Like Dust. London: HarperCollins, 1993.

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Isaac Asimov. The Stars, Like Dust. New York, NY: Spectra/Bantam Books, 1992.

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Copyright Paperback Collection (Library of Congress), ed. The sea is full of stars. New York: Ballantine Pub. Group, 1999.

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Isaac Asimov. Fan xing ruo chen: The stars, like dust. Taibei Shi: Mao tou ying chu ban she, 2006.

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Boys and toys: Ultimate action-adventure movies. New York, NY: Citadel Press, 2002.

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Brode, Douglas. Boys and Toys: Ulitmate Action-Adventure Movies. New York, usa: Citadel, 2003.

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Book chapters on the topic "Action Stars"

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Donnar, Glen. "Redundancy and Ageing: Sylvester Stallone’s Enduring Action Star Image." In Lasting Screen Stars, 245–58. London: Palgrave Macmillan UK, 2016. http://dx.doi.org/10.1057/978-1-137-40733-7_18.

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Gulam, Joshua. "From Action Babe to Mature Actress: The Place of Humanitarianism in Angelina Jolie’s Lasting Screen Career." In Lasting Screen Stars, 277–90. London: Palgrave Macmillan UK, 2016. http://dx.doi.org/10.1057/978-1-137-40733-7_20.

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Lee, Nikki J. Y. "Pop-orientalism and the Asian Star Body: Rain and the Transnational Hollywood Action Movie." In East Asian Film Stars, 35–48. London: Palgrave Macmillan UK, 2014. http://dx.doi.org/10.1057/9781137029195_3.

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Morris, Mark. "A Genealogy of the South Korean Action ‘Star’: Jang Dong-hwi, Hwang Jeong-ri, Jeong Du-hong." In East Asian Film Stars, 205–21. London: Palgrave Macmillan UK, 2014. http://dx.doi.org/10.1057/9781137029195_14.

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Martin, Daniel. "Body of Action, Face of Authenticity: Symbolic Stars in the Transnational Marketing and Reception of East Asian Cinema." In East Asian Film Stars, 19–34. London: Palgrave Macmillan UK, 2014. http://dx.doi.org/10.1057/9781137029195_2.

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Kawaler, Steven D. "Asteroseismology in Action: Pulsating Hot White Dwarfs." In New Eyes to See Inside the Sun and Stars, 261–68. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4982-2_58.

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Lau, Dorothy Wai Sim. "Voices of Mulan in Animated and Live-Action Cinematic Spaces." In Reorienting Chinese Stars in Global Polyphonic Networks, 155–78. Singapore: Springer Singapore, 2021. http://dx.doi.org/10.1007/978-981-16-0313-6_8.

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Thorpe, Holly. "Digital Media and the Transnational Imaginary: Virtual Memorialization of Global Action Sport Stars." In Transnational Mobilities in Action Sport Cultures, 68–103. London: Palgrave Macmillan UK, 2014. http://dx.doi.org/10.1057/9780230390744_3.

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Lau, Dorothy Wai Sim. "Mediating Action and Speech: Michelle Yeoh’s Star Discourse in Pan-Pacific Connections." In Reorienting Chinese Stars in Global Polyphonic Networks, 25–44. Singapore: Springer Singapore, 2021. http://dx.doi.org/10.1007/978-981-16-0313-6_2.

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Shaw, J. Scott. "Near-Contact Binary Stars." In Active Close Binaries, 241–51. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0679-2_20.

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Conference papers on the topic "Action Stars"

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MONTELONGO GARCIA, N., and T. ZANNIAS. "DYNAMO ACTION ON RELATIVISTIC SPHERICAL STARS." In Proceedings of the MG11 Meeting on General Relativity. World Scientific Publishing Company, 2008. http://dx.doi.org/10.1142/9789812834300_0330.

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Browning, Matthew K., Gibor Basri, Richard J. Stancliffe, Guenter Houdek, Rebecca G. Martin, and Christopher A. Tout. "Dynamo Action in Fully Convective Low-Mass Stars." In UNSOLVED PROBLEMS IN STELLAR PHYSICS: A Conference in Honor of Douglas Gough. AIP, 2007. http://dx.doi.org/10.1063/1.2818964.

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Oishi, Jeffrey S., Matthew J. Turk, Tom Abel, and Greg Bryan. "Turbulence and small scale dynamo action in population III star formation." In FIRST STARS IV – FROM HAYASHI TO THE FUTURE –. AIP, 2012. http://dx.doi.org/10.1063/1.4754334.

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Pei, Songwen, Xianrong Wang, Wei Qin, and Sheng Liang. "STARS: Spatial Temporal Graph Convolution Network for Action Recognition System on FPGAs." In 2021 IEEE 45th Annual Computers, Software, and Applications Conference (COMPSAC). IEEE, 2021. http://dx.doi.org/10.1109/compsac51774.2021.00218.

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Petitdemange, Ludovic, Martin Schrinner, and Emmanuel Dormy. "Action of differential rotation on the large-scale magnetic field of stars and planets." In WAVES AND INSTABILITIES IN SPACE AND ASTROPHYSICAL PLASMAS. AIP, 2012. http://dx.doi.org/10.1063/1.3701356.

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Osten, Rachel. "Transient Emissions from Radio-Active Stars." In Bursts, Pulses and Flickering: wide-field monitoring of the dynamic radio sky. Trieste, Italy: Sissa Medialab, 2008. http://dx.doi.org/10.22323/1.056.0005.

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Kochukhov, O., N. Piskunov, I. Ilyin, I. Tuominen, and Eric Stempels. "Magnetic Doppler Imaging of Active Stars." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099216.

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Chen, Hsuan-Sheng, Hua-Tsung Chen, Yi-Wen Chen, and Suh-Yin Lee. "Human action recognition using star skeleton." In the 4th ACM international workshop. New York, New York, USA: ACM Press, 2006. http://dx.doi.org/10.1145/1178782.1178808.

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Leitzinger, M., P. Odert, A. Hanslmeier, A. A. Konovalenko, M. Vanko, M. L. Khodachenko, H. Lammer, H. O. Rucker, and Eric Stempels. "Decametric observations of active M-dwarfs." In COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP, 2009. http://dx.doi.org/10.1063/1.3099205.

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Yuuki, Hayato, Takeharu Ito, and Seiji Kawamura. "Active Star Coupler." In International Congress & Exposition. 400 Commonwealth Drive, Warrendale, PA, United States: SAE International, 1992. http://dx.doi.org/10.4271/920619.

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Reports on the topic "Action Stars"

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Lang, Kenneth R. Radio Wavelength Observations of Magnetic Fields on Active Dwarf-M, RS CVN and Magnetic Stars,. Fort Belvoir, VA: Defense Technical Information Center, January 1986. http://dx.doi.org/10.21236/ada171985.

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S. Abdellatif, Omar, Ali Behbehani, and Mauricio Landin. Luxembourg COVID-19 Governmental Response. UN Compliance Research Group, August 2021. http://dx.doi.org/10.52008/lux0501.

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The UN Compliance Research Group is a global organization which specializes in monitoring the work of the United Nations (UN). Through our professional team of academics, scholars, researchers and students we aim to serve as the world's leading independent source of information on members' compliance to UN resolutions and guidelines. Our scope of activity is broad, including assessing the compliance of member states to UN resolutions and plan of actions, adherence to judgments of the International Court of Justice (ICJ), World Health Organization (WHO) guidelines and commitments made at UN pledging conferences. We’re proud to present the international community and global governments with our native research findings on states’ annual compliance with the commitments of the UN and its affiliated agencies. Our goal as world citizens is to foster a global change towards a sustainable future; one which starts with ensuring that the words of delegates are transformed into action and that UN initiatives don’t remain ink on paper. Hence, we offer policy analysis and provide advice on fostering accountability and transparency in UN governance as well as tracing the connection between the UN policy-makers and Non-governmental organizations (NGOs). Yet, we aim to adopt a neutral path and do not engage in advocacy for issues or actions taken by the UN or member states. Acting as such, for the sake of transparency. The UN Compliance Research Group dedicates all its effort to inform the public and scholars about the issues and agenda of the UN and its affiliated agencies.
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3

Snijder, Mieke, and Marina Apgar, J. How Does Participatory Action Research Generate Innovation? Findings from a Rapid Realist Review. Institute of Development Studies (IDS), July 2021. http://dx.doi.org/10.19088/clarissa.2021.009.

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This Emerging Evidence Report shares evidence of how, for whom, and under what circumstances, Participatory Action Research (PAR) leads to innovative actions. A rapid realist review was undertaken to develop programme theories that explain how PAR generates innovation. The methodology included peer-reviewed and grey literature and moments of engagement with programme staff, such that their input supported the development and refinement of three resulting initial programme theories (IPTs) that we present in this report. Across all three IPTs, safe relational space, group facilitation, and the abilities of facilitators, are essential context and intervention components through which PAR can generate innovation. Implications from the three IPTs for evaluation design of the CLARISSA programme are identified and discussed. The report finishes with opportunities for the CLARISSA programme to start building an evidence base of how PAR works as an intervention modality, such as evidencing group-level conscientisation, the influence of intersecting inequalities, and influence of diverse perspectives coming together in a PAR process.
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Vonk, Jaynie. Women's Empowerment in the Philippines: Impact evaluation of the ‘BASIC START’ project. Oxfam GB, February 2021. http://dx.doi.org/10.21201/2020.6935.

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This evaluation is presented as part of the Effectiveness Review Series 2018/19 on women’s empowerment. The BASIC START (Building Autonomous and Stable Institutions and Communities through Socially Cohesive, Transparent, Accountable and Responsive Transition) in the Bangsamoro' project was carried out in the Autonomous Region in Muslim Mindanao (ARMM) in the Philippines between April 2015 and August 2017, by Oxfam together with four implementing partners: Al Mujadilah Development Foundation (AMDF), United Youth of the Philippines Women (UnYPhil-Women), Tarbilang Foundation, and Women Engaged in Action on 1325 (WE Act 1325). The project aimed to promote women's empowerment and peacebuilding in the region. A quasi-experimental approach was used to assess the impact of the project activities in strengthening women’s empowerment. The evaluation used Oxfam's Women's Empowerment (WE) index. Overall, the evaluation found that the BASIC START project had a positive impact on Women's Empowerment in all three levels investigated – personal, relational and environmental. Find out more by reading the evaluation brief or the full report.
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Harris, Jody, Sarah Gibbons, O’Brien Kaaba, Tabitha Hrynick, and Ruth Stirton. A ‘Right to Nutrition’ in Zambia: Linking Rhetoric, Law and Practice. Institute of Development Studies (IDS), August 2021. http://dx.doi.org/10.19088/ids.2021.051.

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Zambians in all walks of life are affected by malnutrition, and working through human rights is one key way to address this injustice. Based on research aiming to understand how a ‘right to nutrition’ is perceived by different actors globally and in Zambia, this brief presents a clear framework for a rights-based approach to nutrition in Zambia. This framework identifies rhetorical, legal and practical functions of human rights, and offers a way to think through clearly how different actors might work on the different aspects of rights. Addressing these three aspects of a right to nutrition all together – instead of by very separate constituencies as happens now – is fundamental to a coherent rights-based approach to nutrition. This brief outlines which actors need to come together – from law and policy, activism and communities, across global, national and local levels – and suggests how to start. It lays out the Zambian policy, legal and practical environment as it stands, and suggests actions to move forward in each of these areas in ways that are consistent with the different aspects of rights. Through these steps, Zambia can become known as a hub of action on a right to nutrition, to join with others in using human rights to address the injustice of malnutrition.
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Sheridan, Anne. Annual report on migration and asylum 2016: Ireland. ESRI, November 2017. http://dx.doi.org/10.26504/sustat65.

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The Annual Report on Migration and Asylum 2016 provides an overview of trends, policy developments and significant debates in the area of asylum and migration during 2016 in Ireland. Some important developments in 2016 included: The International Protection Act 2015 was commenced throughout 2016. The single application procedure under the Act came into operation from 31 December 2016. The International Protection Office (IPO) replaced the Office of the Refugee Applications Commissioner (ORAC) from 31 December 2016. The first instance appeals body, the International Protection Appeals Tribunal (IPAT), replacing the Refugee Appeals Tribunal (RAT), was established on 31 December 2016. An online appointments system for all registrations at the Registration Office in Dublin was introduced. An electronic Employment Permits Online System (EPOS) was introduced. The Irish Short Stay Visa Waiver Programme was extended for a further five years to October 2021. The Second National Action Plan to Prevent and Combat Human Trafficking was published. 2016 was the first full year of implementation of the Irish Refugee Protection Programme (IRPP). A total of 240 persons were relocated to Ireland from Greece under the relocation strand of the programme and 356 persons were resettled to Ireland. Following an Oireachtas motion, the Government agreed to allocate up to 200 places to unaccompanied minors who had been living in the former migrant camp in Calais and who expressed a wish to come to Ireland. This figure is included in the overall total under the IRPP. Ireland and Jordan were appointed as co-facilitators in February 2016 to conduct preparatory negotiations for the UN high level Summit for Refugees and Migrants. The New York Declaration, of September 2016, sets out plans to start negotiations for a global compact for safe, orderly and regular migration and a global compact for refugees to be adopted in 2018. Key figures for 2016: There were approximately 115,000 non-EEA nationals with permission to remain in Ireland in 2016 compared to 114,000 at the end of 2015. Net inward migration for non-EU nationals is estimated to be 15,700. The number of newly arriving immigrants increased year-on-year to 84,600 at April 2017 from 82,300 at end April 2016. Non-EU nationals represented 34.8 per cent of this total at end April 2017. A total of 104,572 visas, both long stay and short stay, were issued in 2016. Approximately 4,127 persons were refused entry to Ireland at the external borders. Of these, 396 were subsequently admitted to pursue a protection application. 428 persons were returned from Ireland as part of forced return measures, with 187 availing of voluntary return, of which 143 were assisted by the International Organization for Migration Assisted Voluntary Return Programme. There were 532 permissions of leave to remain granted under section 3 of the Immigration Act 1999 during 2016. A total of 2,244 applications for refugee status were received in 2016, a drop of 32 per cent from 2015 (3,276). 641 subsidiary protection cases were processed and 431 new applications for subsidiary protection were submitted. 358 applications for family reunification in respect of recognised refugees were received. A total of 95 alleged trafficking victims were identified, compared with 78 in 2015.
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