Observational Cosmology - astro845 Course Observational Cosmology Course No. astro845 Category Type Language Teaching hours CP Semester Elective Lecture with exercises English 2+1 4 ST Requirements for Participation: Preparation: Form of Testing and Examination: Requirements for the examination (written or oral): successful work with the exercises Length of Course: 1 semester Aims of the Course: Students with B.
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Wave Optics and Astronomical Applications - astro846 Course Wave Optics and Astronomical Applications Course No. astro846 Category Type Language Teaching hours CP Semester Elective Lecture English 2 3 ST Requirements: Preparation: Form of Testing and Examination: Written or oral examination Length of Course: 1 semester Aims of the Course: Acquire the fundamentals necessary to carry out research projects in the field of wave optics and astronomical infrared interferometry Contents of the Course: Fundamentals of wave optics; Fourier mathematics; digital image processing; Michelson interferometry; speckle interferometry; speckle holography; Knox-Thompson method; bispectrum-speckle interferometry; interferometric spectroscopy; infrared-long-baseline interferometry; optical phase-closure method; infrared interferometry of young stars and stars in late evolutionary stages and in nuclei of galaxies Recommended Literature: Lecture Notes
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Wave Optics and Astronomical Applications - astro846 Course Wave Optics and Astronomical Applications Course No. astro846 Category Type Language Teaching hours CP Semester Elective Lecture English 2 3 ST Requirements for Participation: Preparation: Form of Testing and Examination: Written or oral examination Length of Course: 1 semester Aims of the Course: Acquire the fundamentals necessary to carry out research projects in the field of wave optics and astronomical infrared interferometry Contents of the Course: Fundamentals of wave optics; Fourier mathematics; digital image processing; Michelson interferometry; speckle interferometry; speckle holography; Knox-Thompson method; bispectrum-speckle interferometry; interferometric spectroscopy; infrared-long-baseline interferometry; optical phase-closure method; infrared interferometry of young stars and stars in late evolutionary stages and in nuclei of galaxies Recommended Literature: Lecture Notes
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Optical Observations - astro847 Course Optical Observations Course No. astro847 Category Type Language Teaching hours CP Semester Elective Lecture with exercises English 2+1 4 ST Requirements: Preparation: Astronomy introduction classes Form of Testing and Examination: Requirements for the examination (written or oral exam): successful work with exercises Length of Course: 1 semester Aims of the Course: The students should get familiar with major aspects of optical astronomical observations, data reduction, and image analysis.
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Optical Observations - astro847 Course Optical Observations Course No. astro847 Category Type Language Teaching hours CP Semester Elective Lecture with exercises English 2+1 4 ST Requirements for Participation: Preparation: Astronomy introduction classes Form of Testing and Examination: Requirements for the examination (written or oral exam): successful work with exercises Length of Course: 1 semester Aims of the Course: The students should get familiar with major aspects of optical astronomical observations, data reduction, and image analysis.
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Galactic and Intergalactic Magnetic Fields - astro848 Course Galactic and Intergalactic Magnetic Fields Course No. astro848 Category Type Language Teaching hours CP Semester Elective Lecture with exercises English 2+1 4 ST Requirements: Preparation: Good knowledge of electrodynamics and astronomy Form of Testing and Examination: Requirements for examination (written or oral): successful work with the exercises Length of Course: 1 semester Aims of the Course: The students shall become familiar with relativistic plasmas in astrophysics.
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Galactic and Intergalactic Magnetic Fields - astro848 Course Galactic and Intergalactic Magnetic Fields Course No. astro848 Category Type Language Teaching hours CP Semester Elective Lecture with exercises English 2+1 4 ST Requirements for Participation: Preparation: Good knowledge of electrodynamics and astronomy Form of Testing and Examination: Requirements for examination (written or oral): successful work with the exercises Length of Course: 1 semester Aims of the Course: The students shall become familiar with relativistic plasmas in astrophysics.
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Multiwavelength Observations of Galaxy Clusters - astro849 Course Multiwavelength Observations of Galaxy Clusters Course No. astro849 Category Type Language Teaching hours CP Semester Elective Lecture with exercises English 2+1 4 ST Requirements: Preparation: Introductory Astronomy lectures Form of Testing and Examination: Written or oral examination, successful exercise work Length of Course: 1 semester Aims of the Course: To introduce the students into the largest clearly defined structures in the Universe, clusters of galaxies.
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Multiwavelength Observations of Galaxy Clusters - astro849 Course Multiwavelength Observations of Galaxy Clusters Course No. astro849 Category Type Language Teaching hours CP Semester Elective Lecture with exercises English 2+1 4 ST Requirements for Participation: Preparation: Introductory Astronomy lectures Form of Testing and Examination: Written or oral examination, successful exercise work Length of Course: 1 semester Aims of the Course: To introduce the students into the largest clearly defined structures in the Universe, clusters of galaxies.
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Introduction to Hydro- and Magnetohydrodynamics - astro8401 Course Introduction to Hydro- and Magnetohydrodynamics Course No. astro8401 Category Type Language Teaching hours CP Semester Elective Lecture English 2 3 ST Requirements: Preparation: Revision of vectors and vector calculus, electromagnetism, basic thermodynamics Form of Testing and Examination: Written or oral examination Length of Course: 1 semester Aims of the Course: The students will become familiar with the basic laws of hydrodynamics and magnetohydrodynamics and will understand their universal applicability and importance in many varied contexts.
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