Добірка наукової літератури з теми "Cosmic-ray diffusion"
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Статті в журналах з теми "Cosmic-ray diffusion"
Duffy, Peter. "Bohm Diffusion and Cosmic-Ray-Modified Shocks." International Astronomical Union Colloquium 142 (1994): 981–83. http://dx.doi.org/10.1017/s0252921100078428.
Повний текст джерелаZhang, Yiran, Siming Liu, and Dejin Wu. "Cosmic-Ray Convection–Diffusion Anisotropy." Astrophysical Journal 938, no. 2 (October 1, 2022): 106. http://dx.doi.org/10.3847/1538-4357/ac8f28.
Повний текст джерелаReichherzer, P., J. Becker Tjus, E. G. Zweibel, L. Merten, and M. J. Pueschel. "Turbulence-level dependence of cosmic ray parallel diffusion." Monthly Notices of the Royal Astronomical Society 498, no. 4 (August 21, 2020): 5051–64. http://dx.doi.org/10.1093/mnras/staa2533.
Повний текст джерелаSchlickeiser, Reinhard. "Cosmic-Ray Transport and Acceleration." International Astronomical Union Colloquium 142 (1994): 926–36. http://dx.doi.org/10.1017/s0252921100078337.
Повний текст джерелаCommerçon, Benoît, Alexandre Marcowith, and Yohan Dubois. "Cosmic-ray propagation in the bi-stable interstellar medium." Astronomy & Astrophysics 622 (February 2019): A143. http://dx.doi.org/10.1051/0004-6361/201833809.
Повний текст джерелаArmillotta, Lucia, Eve C. Ostriker, and Yan-Fei Jiang. "Cosmic-Ray Transport in Simulations of Star-forming Galactic Disks." Astrophysical Journal 922, no. 1 (November 1, 2021): 11. http://dx.doi.org/10.3847/1538-4357/ac1db2.
Повний текст джерелаMaiti, Snehanshu, Kirit Makwana, Heshou Zhang, and Huirong Yan. "Cosmic-ray Transport in Magnetohydrodynamic Turbulence." Astrophysical Journal 926, no. 1 (February 1, 2022): 94. http://dx.doi.org/10.3847/1538-4357/ac46c8.
Повний текст джерелаZIRAKASHVILI, VLADIMIR N. "COSMIC RAY ANISOTROPY PROBLEM." International Journal of Modern Physics A 20, no. 29 (November 20, 2005): 6858–60. http://dx.doi.org/10.1142/s0217751x05030314.
Повний текст джерелаChan, T. K., D. Kereš, P. F. Hopkins, E. Quataert, K.-Y. Su, C. C. Hayward та C.-A. Faucher-Giguère. "Cosmic ray feedback in the FIRE simulations: constraining cosmic ray propagation with GeV γ-ray emission". Monthly Notices of the Royal Astronomical Society 488, № 3 (10 липня 2019): 3716–44. http://dx.doi.org/10.1093/mnras/stz1895.
Повний текст джерелаExarhos, G., and X. Moussas. "On the heliolatitudinal variation of the galactic cosmic-ray intensity. Comparison with Ulysses measurements." Annales Geophysicae 21, no. 6 (June 30, 2003): 1341–45. http://dx.doi.org/10.5194/angeo-21-1341-2003.
Повний текст джерелаДисертації з теми "Cosmic-ray diffusion"
Cea, del Pozo Elsa de. "Some observational and theoretical aspects of cosmic-ray diffusion." Doctoral thesis, Universitat Autònoma de Barcelona, 2011. http://hdl.handle.net/10803/51003.
Повний текст джерелаThis Thesis deals with certain aspects on cosmic-ray diffusion. It is divided in two parts, one describes phenomenological models of cosmic-ray diffusion, and the other presents observations taken with the MAGIC experiments and simulations of the future Cherenkov Telescope Array (CTA). In the first part, the generally accepted theory for cosmic-ray diffusion is introduced. Supernova remnants (SNRs) are believed to be the more likely scenarios of cosmic-ray acceleration, considering both hadronic and leptonic processes. The mechanism for particle acceleration in each SNR is assumed to be diffusive shock acceleration (DSA). To obtain the observational confirmation of proton and nuclei acceleration, and distinguish it from leptonic emission, the effects of multiple messengers produced by secondary particles must be isolated. Following this, a model for the neighborhood of the SNR IC443 is developed, explaining the high energy phenomenology: cosmic rays escape from the remnant, the most energetic ones reach first the molecular cloud located in front of it and the least energetic ones still remain confined on the shell of the SNR. The results are confronted with the latest observations that are obtained from this source. The apparent displacement between high and very high energy detected sources is explained thanks to this model. Moreover, a multi-frequency and multi-messenger model (i.e., photons from the whole electromagnetic spectrum and neutrinos) for the diffuse emission coming from the starburst galaxy M82 is presented. The gamma-ray predictions are compared to the posterior detections in the energy range between the giga- and the tera-electronvolts of the starburst galaxies M82 and NGC 253, observed by the satellite Fermi and the ground-based experiments H.E.S.S. and VERITAS. The model explains rather satisfactorily these detections at high and very high energy. In the second part of the Thesis, the technique for the gamma-ray detection at ground level through Cherenkov radiation is described. This Cherenkov technique is used in the MAGIC experiment, among others. Some of the observations taken by the student with this telescope facility are presented as part of this Thesis. First, the upper limits to the gamma-ray flux coming from two sources in the region of the SNR G65.1+0.6 when observed with MAGIC-I are shown. These two sources were previously detected by the Milagro experiment and are associated with two bright sources in the Fermi catalog. One of the possible explanations is that these sources are two pulsars powering the pulsar wind nebula that surrounds them. Furthermore, preliminar results of the stereo observations (using the two MAGIC telescopes) of the SNR IC443 are presented. The goal for these observations is performing an energy-dependent morphological study. So far, the obtained number of hours is not enough, although new observations are planned for the near future. Finally, some simulations for the future CTA are presented for the first time, together with several spectral studies regarding interesting scientific cases. In particular, those studies are focused on objects that have been already mentioned in this Thesis, like the SNR IC443 and the starburst galaxies M82 and NGC 253, and also on molecular clouds that are illuminated by cosmic rays which escaped from nearby SNRs. The CTA observatory represents the future of the ground-based gamma-ray observations, and it is likely to include every collaboration from the existing telescope facilities nowadays. The energy range will be widened, the sensitivity will be one order of magnitude improved and the angular resolution will be enhanced respect to the existing experiments up to now. Thus, the present Thesis is just the tip of the iceberg of what is yet to come.
KO, CHUNG-MING. "COSMIC-RAY MODIFIED STELLAR WINDS (ACCELERATION, MODULATION, DIFFUSION, TRANSONIC SOLUTION)." Diss., The University of Arizona, 1986. http://hdl.handle.net/10150/183980.
Повний текст джерелаVos, Etienne Eben. "Cosmic ray modulation processes in the heliosphere / Vos E.E." Thesis, North-West University, 2011. http://hdl.handle.net/10394/7266.
Повний текст джерелаThesis (M.Sc. (Physics))--North-West University, Potchefstroom Campus, 2012.
Engelbrecht, Nicholas Eugéne. "On the heliospheric diffusion tensor and its effect on 26-day recurrent cosmic-ray variations / N.E. Engelbrecht." Thesis, North-West University, 2008. http://hdl.handle.net/10394/2052.
Повний текст джерелаNkosi, Godfrey Sibusiso. "A study of cosmic ray anisotropies in the heliosphere / Godfrey Sibusiso Nkosi." Thesis, North-West University, 2006. http://hdl.handle.net/10394/1627.
Повний текст джерелаEngelbrecht, Nicholas Eugéne. "On the development and applications of a three-dimensional ab initio cosmic-ray modulation model / Nicholas Eugéne Engelbrecht." Thesis, North-West University, 2012. http://hdl.handle.net/10394/8735.
Повний текст джерелаThesis (PhD (Physics))--North-West University, Potchefstroom Campus, 2013
Giesen, Gaelle. "Dark Matter Indirect Detection with charged cosmic rays." Thesis, Paris 11, 2015. http://www.theses.fr/2015PA112160/document.
Повний текст джерелаOverwhelming evidence for the existence of Dark Matter (DM), in the form of an unknownparticle filling the galactic halos, originates from many observations in astrophysics and cosmology: its gravitational effects are apparent on galactic rotations, in galaxy clusters and in shaping the large scale structure of the Universe. On the other hand, a non-gravitational manifestation of its presence is yet to be unveiled. One of the most promising techniques is the one of indirect detection, aimed at identifying excesses in cosmic ray fluxes which could possibly be produced by DM annihilations or decays in the Milky Way halo. The current experimental efforts mainly focus in the GeV to TeV energy range, which is also where signals from WIMPs (Weakly Interacting Massive Particles) are expected. Focussing on charged cosmic rays, in particular antiprotons, electrons and positrons, as well as their secondary emissions, an analysis of current and forseen cosmic ray measurements and improvements on astrophysical models are presented. Antiproton data from PAMELA imposes contraints on annihilating and decaying DM which are similar to (or even slightly stronger than) the most stringent bounds from gamma ray experiments, even when kinetic energies below 10 GeV are discarded. However, choosing different sets of astrophysical parameters, in the form of propagation models and halo profiles, allows the contraints to span over one or two orders of magnitude. In order to exploit fully the power of antiprotons to constrain or discover DM, effects which were previously perceived as subleading turn out to be relevant especially for the analysis of the newly released AMS-02 data. In fact, including energy losses, diffusive reaccelleration and solar modulation can somewhat modify the current bounds, even at large DM masses. A wrong interpretation of the data may arise if they are not taken into account. Finally, using the updated proton and helium fluxes just released by the AMS-02 experiment, the astrophysical antiproton to proton ratio and its uncertainties are reevaluated and compared to the preliminarly reported AMS-02 measurements. No unambiguous evidence for a significant excess with respect to expectations is found. Yet, some preference for thicker halos and a flatter energy dependence of the diffusion coefficient starts to emerge. New stringed constraints on DM annihilation and decay are derived. Secondary emissions from electrons and positrons can also be used to constrain DM annihilation or decay in the galactic halo. The radio signal due to synchrotron radiation of electrons and positrons on the galactic magnetic field, gamma rays from bremsstrahlung processes on the galactic gas densities and from Inverse Compton scattering processes on the interstellar radiation field are considered. With several magnetic field configurations, propagation scenarios and improved gas density maps and interstellar radiation field, state-of-art tools allowing the computaion of synchrotron and bremssttrahlung radiation for any WIMP DM model are provided. All numerical results for DM are incorporated in the release of the Poor Particle Physicist Coookbook for DM Indirect Detection (PPPC4DMID). Finally, the possible GeV gamma-ray excess identified in the Fermi-LAT data from the Galactic Center in terms of DM annihilation, either in hadronic or leptonic channels is studied. In order to test this tantalizing interprestation, a multi-messenger approach is used: first, the computation of secondary emisison from DM with respect to previous works confirms it to be relevant for determining the DM spectrum in leptonic channels. Second, limits from antiprotons severely constrain the DM interpretation of the excess in the hadronic channel, for standard assumptions on the Galactic propagation parameters and solar modulation. However, they considerably relax if more conservative choices are adopted
Antecki, Thorsten [Verfasser], Reinhard [Gutachter] Schlickeiser, and Horst [Gutachter] Fichtner. "Effects of a finite downstream medium in diffusive cosmic ray acceleration at relativistic shock waves / Thorsten Antecki. Gutachter: Reinhard Schlickeiser ; Horst Fichtner." Bochum : Ruhr-Universität Bochum, 2016. http://d-nb.info/110905159X/34.
Повний текст джерелаVoisin, Fabien. "Environment Studies of Pulsar Wind Nebulae and Their Interactions with the Interstellar Medium." Thesis, 2017. http://hdl.handle.net/2440/119266.
Повний текст джерелаThesis (Ph.D.) -- University of Adelaide, School of Physical Sciences, 2017
Raath, Jan Louis. "A comparative study of cosmic ray modulation models / Jan Louis Raath." Thesis, 2015. http://hdl.handle.net/10394/15516.
Повний текст джерелаMSc (Space Physics), North-West University, Potchefstroom Campus, 2015
Книги з теми "Cosmic-ray diffusion"
Shalchi, Andreas. Nonlinear Cosmic Ray Diffusion Theories. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00309-7.
Повний текст джерелаGaggero, Daniele. Cosmic Ray Diffusion in the Galaxy and Diffuse Gamma Emission. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-29949-0.
Повний текст джерелаservice), SpringerLink (Online, ed. Cosmic Ray Diffusion in the Galaxy and Diffuse Gamma Emission. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012.
Знайти повний текст джерелаShalchi, Andreas. Nonlinear Cosmic Ray Diffusion Theories. Springer, 2009.
Знайти повний текст джерелаShalchi, Andreas. Nonlinear Cosmic Ray Diffusion Theories. Springer Berlin / Heidelberg, 2010.
Знайти повний текст джерелаNonlinear Cosmic Ray Diffusion Theories. Springer, 2009.
Знайти повний текст джерелаCosmic Ray Diffusion In The Galaxy And Diffuse Gamma Emission. Springer, 2012.
Знайти повний текст джерелаGaggero, Daniele. Cosmic Ray Diffusion in the Galaxy and Diffuse Gamma Emission. Springer, 2016.
Знайти повний текст джерелаЧастини книг з теми "Cosmic-ray diffusion"
Shalchi, Andreas. "The General scenario." In Nonlinear Cosmic Ray Diffusion Theories, 1–28. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00309-7_1.
Повний текст джерелаShalchi, Andreas. "On Astrophysical Turbulence." In Nonlinear Cosmic Ray Diffusion Theories, 29–56. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00309-7_2.
Повний текст джерелаShalchi, Andreas. "The Quasilinear Theory." In Nonlinear Cosmic Ray Diffusion Theories, 57–81. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00309-7_3.
Повний текст джерелаShalchi, Andreas. "The Nonlinear Guiding Center Theory." In Nonlinear Cosmic Ray Diffusion Theories, 83–97. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00309-7_4.
Повний текст джерелаShalchi, Andreas. "The Weakly Nonlinear Theory." In Nonlinear Cosmic Ray Diffusion Theories, 99–114. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00309-7_5.
Повний текст джерелаShalchi, Andreas. "The Second-Order QLT." In Nonlinear Cosmic Ray Diffusion Theories, 115–34. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00309-7_6.
Повний текст джерелаShalchi, Andreas. "The Extended Nonlinear Guiding Center Theory." In Nonlinear Cosmic Ray Diffusion Theories, 135–53. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00309-7_7.
Повний текст джерелаShalchi, Andreas. "Applications." In Nonlinear Cosmic Ray Diffusion Theories, 155–78. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00309-7_8.
Повний текст джерелаShalchi, Andreas. "Summary and Outlook." In Nonlinear Cosmic Ray Diffusion Theories, 179–86. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00309-7_9.
Повний текст джерелаGaggero, Daniele. "Cosmic Ray Diffusion in the Galaxy." In Cosmic Ray Diffusion in the Galaxy and Diffuse Gamma Emission, 7–28. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-29949-0_2.
Повний текст джерелаТези доповідей конференцій з теми "Cosmic-ray diffusion"
Tautz, Robert. "Cosmic-ray diffusion in magnetized turbulence." In Cosmic Rays and the InterStellar Medium. Trieste, Italy: Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.221.0050.
Повний текст джерелаXu, Siyao. "Diffusion of cosmic rays in MHD turbulence." In 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0041.
Повний текст джерелаFang, Kun, Xiao-Jun Bi, and Peng-Fei Yin. "Possible origin of the Geminga slow-diffusion halo." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0670.
Повний текст джерелаGiacinti, Gwenael. "Cosmic-Ray Diffusion and Galactic Magnetic Field Models." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0075.
Повний текст джерелаReimer, Olaf, Ralf Kissmann, Felix Niederwanger, and Andrew W. Strong. "Anisotropic Diffusion in Galactic Cosmic Ray transport using PICARD." In 35th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0480.
Повний текст джерелаBrisbois, Chad, and Hao Zhou. "First Galactic Survey of Energy-Dependent Diffusion by HAWC." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0640.
Повний текст джерелаIlolov, Mamadsho. "Equations of anomalous diffusion of cosmic rays." In The 34th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.236.0510.
Повний текст джерелаKollamparambil Paul, Arun Babu, S. K. Gupta, S. R. Dugad, B. Hariharan, Y. Hayashi, P. Jagadeesan, A. Jain, et al. "Diffusion of cosmic rays in heliosphere, observations from GRAPES-3." In 35th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0011.
Повний текст джерелаChirkin, Dmitry, and Martin Rongen. "Light diffusion in birefringent polycrystals and the IceCube ice anisotropy." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0854.
Повний текст джерелаStrauss, Du Toit, and Horst Fichtner. "On the perpendicular diffusion of solar energetic particles." In The 34th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.236.0195.
Повний текст джерела