Browsing Fakultät für Physik (inkl. GAUSS) by Advisor & Referee "Reiners, Ansgar Prof. Dr."
Now showing items 21-35 of 35
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Solar Variability over the Last 9000 Years
(2018-08-31)The solar activity has been observed to vary at various time scales, of which the 11-year solar cycle is the most prominent one. Since the Sun provides the main external energy to the Earth, knowledge of solar variability ... -
Dynamics of Suspended Dust Grains: Experimental Investigations and Implications for Protoplanetary Discs
(2018-05-29)The collective interaction of solid particulate matter with flowing gas is one of the fundamental processes occurring in planet-forming discs. Small dust grains and pebbles are comparable to or smaller than the mean ... -
Radial velocities in low mass stars: improving the wavelength solution of astronomical spectrographs and understanding stellar noise
(2017-11-10)The radial velocity method has been used to discover hundreds of extrasolar planets in the past two decades. The continuous improvements in radial velocity precision have revealed several rocky planets in the habitable ... -
Modelling turbulent effects of stellar feedback in cosmological simulations
(2017-10-30)In order to study the influence of turbulence on star formation, stellar feedback, and the mixing of metals into the circumgalactic medium (CGM), we implemented a model for star formation and stellar feedback and employ ... -
Nanoscale Waveguiding Studied by Lensless Coherent Diffractive Imaging using EUV High-Harmonic Generation Source
(2017-07-24)The challenge of nanometric imaging drives intense efforts in applied sciences and fundamental research. Following the physical law of diffraction, the utilization of extreme ultraviolet (EUV) or X-ray radiation for imaging ... -
Characterisation of star-planet systems
(2017-07-05)After the first confirmed detection of an exoplanet in 1995, their number has significantly increased to 3 557 confirmed planets around other stars (www.exoplanet.eu, Dec. 2016). The most successful techniques for planet ... -
3-D Modeling of Coronal Mass Ejections with STEREO/SECCHI Data
(2017-02-28)This thesis reports on the three-dimensional analysis of coronal mass ejections (CMEs) in order to answer questions about their morphology and to derive their three-dimensional geometry. The questions are about the ... -
Construction and Analysis of a Microwave-induced Plasma Lamp for Precision Spectroscopy
(2016-06-09)Spectroscopy is one of the most powerful techniques to analyze light of astronomical objects. New instrumentation strives to extend high-precision spectroscopy from the optical to the near-infrared spectral range. This ... -
Simulating the signature of starspots in stellar oscillations
(2016-04-14)It has been known for a few decades that acoustic oscillations are affected by stellar activity. In the case of the Sun global acoustic modes show a variation with the 11-year cycle and a similar phenomenon has been observed ... -
Coronal dynamics driven by magnetic flux emergence
(2015-11-09)The corona is the Sun’s outer atmosphere which is more than 100 times hotter than the solar surface. It can be brilliantly observed in the extreme-ultraviolent (EUV) and soft X-ray passbands. What heats the corona is one ... -
Effect of density stratification on dynamos in gas planets and low-mass stars
(2015-05-29)Numerical simulations of the Geodynamo have reproduced many of the features of the Earth's magnetic field. An ensemble of these simulations has been used to formulate a predictive scaling law which agrees with the Earth's ... -
High-resolution spectroscopy of low-mass stars
(2015-03-23)High-resolution spectroscopy is employed to investigate a large sample of open cluster low-mass stars. The stellar rotation and magnetic activity of these stars are measured and their correlation is studied. I find in ... -
Fabry-Pérot etalons for high precision radial velocity calibration
(2014-06-24)The current generation of astronomical spectrographs can measure radial velocity signals of exoplanets down to a few m/s, in ideal cases even 60 cm/s can be achieved. This led to the discovery of rocky planets with masses ... -
Simulations of magnetoconvection in cool main-sequence stars
(2014-05-26)In this thesis, the magnetoconvective processes in the nearsurface layers of cool main-sequence stars were studied in 24 three-dimensional local “box-in-a-star” simulations. For each of six sets of stellar parameters ... -
Photometric variability in the Kepler field
(2013-09-23)Measurements of rotation and differential rotation for more than 20,000 active Kepler stars.