Hallgren, K.; Hartogh, P.; Jarchow, C.: A new microwave spectrometer for ground-based observations of water vapour. Atmos. Meas. Tech. Discuss 6, pp. 4677 - 4703 (2013)
Hallgren, K.; Hartogh, P.: First detection of tidal behaviour in polar mesospheric water vapour by ground based microwave spectroscopy. Atmos. Chem. Phys. 12, pp. 3753 - 3759 (2012)
Stevens, M. H.; Lossow, S.; Fiedler, J.; Baumgarten, G.; Lübken, F.-J.; Hallgren, K.; Hartogh, P.; Randall, C. E.; Lumpe, J.; Bailey, S. M.et al.; Niciejewski, R.; Meier, R. R.; Plane, J. M. C.; Kochenash, A. J.; Murtagh, D. P.; Englert, C. R.: Bright polar mesospheric clouds formed by main engine exhaust from the space shuttles final launch. Journal Geophysical Research 117, D19206 (2012)
Hallgren, K.; Hartogh, P.: First detection of tidal behaviour in polar mesospheric water vapour by ground-based microwave spectroscopy. Atmospheric Chemistry and Physics Discussions 11, pp. 31265 - 31281 (2011)
Straub, C.; Kämpfer, N.; Golchert, S. H. W.; Hochschild, G.; Hallgren, K.; Hartogh, P.: ARIS-Campaign: intercomparison of three ground based 22 GHz radiometers for middle atmospheric water vapor at the Zugspitze in winter 2009. Atmospheric Measurement Techniques 4, pp. 1979 - 1994 (2011)
Straub, C.; Murk, A.; Kämpfer, N.; Golchert, S. H. W.; Hochschild, G.; Hallgren, K.; Hartogh, P.: ARIS-Campaign: intercomparison of three ground based 22 GHz radiometers for middle atmospheric water vapor at the Zugspitze in winter 2009. Atmospheric Measurement Techniques Discussions 4 (3), pp. 3359 - 3400 (2011)
Hartogh, P.; Jarchow, C.; Hallgren, K.: Investigations of the Solar Influence on Middle Atmospheric Water Vapour and Ozone During the Last Solar Cycle - Analysis of the MPS Data Set. In: Climate and Weather of the Sun-Earth System (CAWSES) Highlights from a Priority Program, pp. 109 - 124 (Ed. Lübken, F.-J.). Springer, Dordrecht (2012)
Hallgren, K.; Hartogh, P.; Jarchow, C.: A New, High-performance, Heterodyne Spectrometer for Ground-based Remote Sensing of Mesospheric Water Vapour. In: Advances in Geosciences, pp. 569 - 578 (Eds. Bhardwaj, A.; Haider, S. A.; Hartogh, P.; Ip, W.-H.; Ito, T. et al.). World Scientific Publishing Co., Singapore (2010)
Hallgren, K.: Mesospheric water vapor - Variability at different timescales observed by ground-based microwave spectroscopy. Dissertation, Mathematisch-Naturwiss. Fak. Univ., at Rostock (2011)
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.