Non-thermal escape of the martian CO2 atmosphere over time: Constrained by Ar isotopes by Lichtenegger, H.I.M., Dyadechkin, S., Scherf, M., Lammer, H., Adam, R., Kallio, E., Amerstorfer, U.V., Jarvinen, R.

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Machine Learning for Predicting the Bz Magnetic Field Component From Upstream in Situ Observations of Solar Coronal Mass Ejections by Reiss, M. A., Möstl, C., Bailey, R. L., Rüdisser, H. T., Amerstorfer, U. V., Amerstorfer, T., Weiss, A. J., Hinterreiter, J., Windisch, A.

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Non-thermal escape of the martian CO 2 atmosphere over time: Constrained by Ar isotopes by Lichtenegger, H.I.M., Dyadechkin, S., Scherf, M., Lammer, H., Adam, R., Kallio, E., Amerstorfer, U.V., Jarvinen, R.

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Automatic Detection of Interplanetary Coronal Mass Ejections in Solar Wind In Situ Data by Rüdisser, H. T., Windisch, A., Amerstorfer, U. V., Möstl, C., Amerstorfer, T., Bailey, R. L., Reiss, M. A.

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Estimation of the past and present Martian water-ice reservoirs by isotopic constraints on exchange between the atmosphere and the surface by Lammer, H., Kolb, C., Penz, T., Amerstorfer, U.V., Biernat, H.K., Bodiselitsch, B.

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On Kelvin–Helmholtz instability due to the solar wind interaction with unmagnetized planets by Amerstorfer, U.V., Erkaev, N.V., Langmayr, D., Biernat, H.K.

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The Kelvin–Helmholtz instability in magnetohydrodynamics with finite Larmor radius effects and application to Venus by Amerstorfer, U.V.

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Ion loss on Mars caused by the Kelvin–Helmholtz instability by Penz, T., Erkaev, N.V., Biernat, H.K., Lammer, H., Amerstorfer, U.V., Gunell, H., Kallio, E., Barabash, S., Orsini, S., Milillo, A., Baumjohann, W.

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Solar wind flow past Venus and its implications for the occurrence of the Kelvin–Helmholtz instability by Biernat, H.K., Erkaev, N.V., Amerstorfer, U.V., Penz, T., Lichtenegger, H.I.M.

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