. "Astrophysics"@en . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . "Theoretical astrophysics 1-4"@en . . "10" . "Semester 1: Physical foundaions\nThermodynamics: ideal gas, parial ionisaion, Saha equaion. Degeneraion of mater. Nuclear reacions. Basics of luid mechanics and magnetohydrodynamics. Linear perturbaions, waves in homogeneous media, perturbaions in straiied media. Turbulence and convecion. Radiaive transfer equaion\n\nSemester 2: Stellar structure and evoluion\nApplicaion of luid mechanics to stars. Thermodynamics of stellar plasma. Radiaive and convecive transfer of energy. Simpliied models, polytropic spheres. Numerical methods in the modelling of steallr structure and evoluion. Stability of stars: theory of linear pulsaion. Basics of numerical modelling of nonlinear pulsaions. Introducion to asteroseismology. Stellar evoluion: energy producion and nucleosynthesis. Phases of stellar evoluion.\n\nSemester 3: Radiaive transfer\nSaha equaion, Fowler-Milne theory of stellar spectra. Radiaive equilibrium in stellar atmospheres. Transfer equaion. Limb darkening. Theory of Fraunhofer lines. Mechanisms of absorpion, damping, Doppler broadining. Theory of the growth curve, determinaion of stellar composiion. Nontehrmal radiaion processes: synchrotron radiaion, nonthermal bremsstrahlung, comptonisaion.\n\nSemester 4: Difuse matter\nRadiative transfer and raditaive processes in difuse media. Interstellar molecules. The luid dynamics of difuse mater, shock waves. Interstellar dust and gas. Interstellar magneic ields. Interstellar medium in the Milky Way Galaxy. Star formaion. Planetary nebulae and supernove remnants." . . "Presential"@en . "TRUE" . . "Master in Astronomy"@en . . "https://www.elte.hu/en/astronomy-msc" . "120"^^ . "Presential"@en . "The objective of the Astronomy Master's Degree Program is to provide a comprehensive knowledge of astronomy including related interdisciplinary areas. Students will also acquire competencies in the wider field of scientific research, in the use of technical language, in team work and in the communication of scientific results, they will also develop an ability to resolve novel or unusual problems arising in a multidisciplinary context.\n\nThe objective of the Astronomy MSc programme is the formation of fully trained astronomers and astrophysicists capable of supervised observational and theoretical research in astronomy and related fields."@en . . "2"@en . "FALSE" . . "Master"@en . "Thesis" . "8380.00" . "Euro"@en . "8380.00" . "Mandatory" . "Career opportunities\r\nAfter completing the requirements listed above, students are awarded an MSc degree. The MSc degree qualifies its holder to take up positions in the relevant fields and to enlist to a postgraduate (PhD) study programme.\r\n\r\nJob examples\r\nPostgraduate (PhD) studentships at a Hungarian, European or international university research assistant's positions at a Hungarian, European or international research institute industry positions where a strong training in IT, signal processing, physics and electromagnetic wave analysis are an advantage, including telecommunications, computer technology, software companies, air control, satellite communications, etc."@en . "1"^^ . "FALSE" . "Upstream"@en . . . . . . . . . . . . . . . . . . . . . . . . .