Yamada, T.; Baron, P.; Neary, L.; Nishibori, T.; Larsson, R.; Kuroda, T.; Daerden, F.; Kasai, Y.: Observation Capability of a Ground-Based Terahertz Radiometer for Vertical Profiles of Oxygen and Water Abundances in Martian Atmosphere. IEEE Transactions on Geoscience and Remote Sensing 60, p. 3152271 (2022)
Kuroda, T.; Medvedev, A. S.; Yiğit, E.; Hartogh, P.: Global distribution of gravity wave sources and fields in the Martian atmosphere during equinox and solstice inferred from a high-resolution general circulation model. Journal of the Atmospheric Sciences 73, pp. 4895 - 4909 (2016)
Medvedev, A. S.; Nakagawa, H.; Mockel, C.; Yiğit, E.; Kuroda, T.; Hartogh, P.; Terada, K.; Terada, N.; Seki, K.; Schneider, N. M.et al.; Jain, S. K.; Evans, J. S.; Deighan, J. I.; McClintock, W. E.; Lo, D.; Jakosky, B. M.: Comparison of the Martian thermospheric density and temperature from IUVS/MAVEN data and general circulation modeling. Geophysical Research Letters 43, pp. 3095 - 3104 (2016)
Kuroda, T.; Medvedev, A. S.; Yiğit, E.; Hartogh, P.: A global view of gravity waves in the Martian atmosphere inferred from a high-resolution general circulation model. Geophysical Research Letters 42, pp. 9213 - 9222 (2015)
Medvedev, A. S.; Kuroda, T.; Hartogh, P.: Influence of dust on the dynamics of the martian atmosphere above the first scale height. Aeolian Research 3, pp. 145 - 156 (2011)
Yamashita, Y.; Kuroda, T.; Takahashi, M.: Maintainance of zonal wind variability associated with the annular mode on Mars. Geophysical Research Letters 34, L16819 (2007)
Kuroda, T.; Hashimoto, N.; Sakai, D.; Takahashi, M.: Simulation of the Martian atmosphere using a CCSR/NIES AGCM. J. Meteorol. Soc. Japan 83, pp. 1 - 19 (2005)
Kuroda, T.; Kasaba, Y.; Medvedev, A. S.; Hartogh, P.: CO2 snowfalls modulated by the baroclinic waves in the northern winter polar atmosphere of Mars. Fifth international workshop on the Mars Atmosphere: Modelling and observations, Oxford, UK (2014)
Kuroda, T.; Medvedev, A. S.; Hartogh, P.: Radiative forcing by molecules in the stratosphere of Jupiter. 11th Annual Meeting, Asia Oceania Geosciences Society, Sapporo, Japan (2014)
Kuroda, T.; Medvedev, A. S.; Hartogh, P.: Parameterization of the radiative forcing in the stratosphere of Jupiter. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Kuroda, T.; Medvedev, A. S.; Kasaba, Y.; Hartogh, P.: CO2 snowfalls, seasonal ice cap formations and baroclinic waves in the winter polar atmosphere of Mars. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Kuroda, T.; Medvedev, A. S.; Kasaba, Y.; Hartogh, P.: Weather Forecasts on Mars: CO2 Snowfalls Related to the Baroclinic Waves in the Northern Winter Polar Atmosphere. Eighth International Conference on Mars, Pasadena, USA (2014)
Medvedev, A. S.; Yiğit, E.; Kuroda, T.; Hartogh, P.: Response of the Martian upper atmosphere to lower atmospheric dust storms: GCM study. Fifth international workshop on the Mars Atmosphere: Modelling and observations, Oxford, UK (2014)
Medvedev, A. S.; Yiğit, E.; Kuroda, T.; Hartogh, P.: Dynamical coupling between the lower Martian atmosphere and thermosphere. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Medvedev, A.; Yiğit, E.; Kuroda, T.; Hartogh, P.: Influence of global dust storms on the mesosphere and lower thermosphere of Mars. European Planetary Science Congress 2014, Cascais, Portugal (2014)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...