Shaheen, F.; Scariah, N. V.; Lala, M. G. N.; Krishna, A. P.; Jeganathan, C.; Hoekzema, N. M.: Shadow method retrievals of the atmospheric optical depth above Gale crater on Mars using HRSC images. Icarus 388, p. 115229 (2022)
Gwinner, K.; Jaumann, R.; Hauber, E.; Hoffmann, H.; Heipke, C.; Oberst, J.; Neukum, G.; Ansan, V.; Bostelmann, J.; Dumke, A.et al.; Elgner, S.; Erkeling, G.; Fueten, F.; Hiesinger, H.; Hoekzema, N. M.; Kersten, E.; Loizeau, D.; Matz, K.-D.; McGuire, P. C.; Mertens, V.; Michael, G.; Pasewaldt, A.; Pinet, P.; Preusker, F.; Reiss, D.; Roatsch, T.; Schmidt, R.; Scholten, F.; Spiegel, M.; Stesky, R.; Tirsch, D.; van Gasselt, S.; Walter, S.; Waehlisch, M.; Willner, K.: The High Resolution Stereo Camera (HRSC) of Mars Express and its approach to science analysis and mapping for Mars and its satellites. Planetary and Space Science 126, pp. 93 - 138 (2016)
Reiss, D.; Hoekzema, N. M.; Stenzel, O. J.: Dust deflation by dust devils on Mars derived from optical depth measurements using the shadow method in HiRISE images. Planetary and Space Science 93-94, pp. 54 - 64 (2014)
Petrova, E. V.; Hoekzema, N. M.; Markiewicz, W. J.; Thomas, N.; Stenzel, O. J.: Optical depth of the Martian atmosphere and surface albedo from high-resolution orbiter images. Planetary and Space Science 60, pp. 287 - 296 (2012)
Hoekzema, N. M.; Garcia-Comas, M.; Stenzel, O. J.; Grieger, B.; Markiewicz, W. J.; Gwinner, K.; Keller, H. U.: Optical depth and its scale-height in Valles Marineris from HRSC stereo images. Earth and Planetary Science Letters 294 (3-4), pp. 534 - 540 (2010)
Hoekzema, N. M.; Rimmele, T. R.; Rutten, R. J.: Small-scale topology of solar atmosphere dynamics V. Acoustic events and internetwork grains. Astronomy and Astrophysics 390, pp. 681 - 690 (2002)
Reiss, D.; Hoekzema, N. M.; Stenzel, O. J.: Dust Deflation by Dust Devils on Mars Derived from Optical Depth Measurements Using the Shadow Method in HiRISE Images. 45th Lunar and Planetary Science Conference, The Woodlands, Texas (2014)
Stenzel, O. J.; Hoekzema, N. M.; Markiewicz, W. J.: Mars' Atmospheric Optical Depth from Mars Express HRSC and Mars Exploration Rovers A Comparison. 45th Lunar and Planetary Science Conference, The Woodlands, Texas (2014)
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.