Bhatt, M.; Mall, U.; Wöhler, C.; Grumpe, A.; Bugiolacchi, R.: A comparative study of iron abundance estimation methods: Application to the western nearside of the Moon. Icarus 248, pp. 72 - 88 (2015)
Mall, U.; Wöhler, C.; Grumpe, A.; Bugiolacchi, R.; Bhatt, M.: Characterization of lunar soils through spectral features extraction in the NIR. Advances in Space Research 54 (10), pp. 2029 - 2040 (2014)
Wöhler, C.; Grumpe, A.; Berezhnoy, A.; Bhatt, M. U.; Mall, U.: Integrated topographic, photometric and spectral analysis of the lunar surface: Application to impact melt flows and ponds. Icarus 235, pp. 86 - 122 (2014)
Bugiolacchi, R.; Mall, U.; Bhatt, M.; McKenna-Lawlor, S.; Ullaland, K.: From the Imbrium Basin to crater Tycho: The first regional spectral distribution map derived from SIR-2 near-infrared data. Icarus 223, pp. 804 - 818 (2013)
Reddy, V.; Le Corre, L.; O'Brien, D. P.; Nathues, A.; Cloutis, E. A.; Durda, D. D.; Bottke, W. F.; Bhatt, M. U.; Nesvorny, D.; Buczkowski, D.et al.; Scully, J. E. C.; Palmer, E. M.; Sierks, H.; Mann, P. J.; Becker, K. J.; Beck, A. W.; Mittlefehldt, D.; Li, J.-Y.; Gaskell, R.; Russell, C. T.; Gaffey, M. J.; McSween, H. Y.; McCord, T. B.; Combe, J.-P.; Blewett, D.: Corrigendum to ``Delivery of dark material to Vesta via carbonaceous chondritic impacts'' [Icarus 221, pg 544, 2012]. Icarus 223 (1), p. 632 - 632 (2013)
Bhatt, M.; Mall, U.; Bugiolacchi, R.; McKenna-Lawlor, S.; Banaszkiewicz, M.; Nathues, A.; Ullaland, K.: Lunar iron abundance determination using the 2-μm absorption band parameters. Icarus 220 (1), pp. 51 - 64 (2012)
Bugiolacchi, R.; Mall, U.; Bhatt, M.: A near-infrared reflectance survey across lunar crater Aristoteles. In: Proceedings of the 42nd Lunar and Planetary Science Conference. (2011)
Bugiolacchi, R.; Mall, U.; Bhatt, M.: NIR spectral investigation of the Delisle/Diophantus crater region by the SIR-2 instrument. In: Proceedings of the 42nd Lunar and Planetary Science Conference. (2011)
Bhatt, M. U.: Mineralogical analysis and iron abundance estimation of the Moon using the SIR-2 and other VIS-NIR spectrometers on-board the lunar orbiter Chandrayaan-1. Dissertation, Technische Universität Clausthal (2012)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.