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)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.