Zobrazeno 1 - 10
of 555
pro vyhledávání: '"Grott, M."'
Autor:
Spohn, T., Hudson, T. L., Marteau, E., Golombek, M., Grott, M., Wippermann, T., Ali, K. S., Schmelzbach, C., Kedar, S., Hurst, K., Trebi-Ollennu, A., Ansan, V., Garvin, J., Knollenberg, J., Mueller, N., Piqeux, S., Lichtenheldt, R., Krause, C., Fantinati, C., Brinkman, N., Sollberger, D., Delage, P., Vrettos, C., Reershemius, S., Wisniewski, L., Grygorczuk, J., Robertsson, J., Edme, P., Andersson, F., Kroemer, O., Lognonne, P., Giardini, D., Smrekar, S. E., Banerdt, W. B.
Publikováno v:
Space Science Reviews (2022) 218: 72
The NASA InSight Lander on Mars includes the Heat Flow and Physical Properties Package HP$^3$ to measure the surface heat flow of the planet. The package uses temperature sensors that would have been brought to the target depth of 3--5 m by a small p
Externí odkaz:
http://arxiv.org/abs/2112.04438
Autor:
Spohn, T., Hudson, T. L., Witte, L., Wippermann, T., Wisniewski, L., Kediziora, B., Vrettos, C., Lorenz, R. D., Golombek, M., Lichtenfeld, R., Grott, M., Knollenberg, J., Krause, C., Fantinati, C., Nagihara, S., Grygorczuk, J.
Publikováno v:
Advances in Space Research, 69 (2022) 3140-3163
The NASA InSight mission payload includes the Heat Flow and Physical Properties Package HP$^3$ to measure the surface heat flow. The package was designed to use a small penetrator -- nicknamed the mole -- to implement a string of temperature sensors
Externí odkaz:
http://arxiv.org/abs/2112.03234
Thermophysical modelling and parameter estimation of small solar system bodies via data assimilation
Deriving thermophysical properties such as thermal inertia from thermal infrared observations provides useful insights into the structure of the surface material on planetary bodies. The estimation of these properties is usually done by fitting tempe
Externí odkaz:
http://arxiv.org/abs/2003.13804
Autor:
Ho, T.M., Kührt, E., Zhang, X.J., Auster, U., Biele, J., Grott, M., Grundmann, J.T., He, H., Hördt, A., Huang, J.C., Ma, T., Mottola, S., Otto, K., Plettemeier, D., Qin, L., Rubin, M., Schmitz, N., Ulamec, S., Vincent, J.B.
Publikováno v:
In Acta Astronautica December 2023 213:49-70
Autor:
Spohn, T., Müller, N., Knollenberg, J., Grott, M., Golombek, M. P., Plesa, A.‐C., Bickel, V. T., Morgan, P., Krause, C., Breuer, D., Smrekar, S. E., Banerdt, W. B.
Publikováno v:
Geophysical Research Letters; 9/28/2024, Vol. 51 Issue 18, p1-10, 10p
Autor:
Lammer, H., Chassefière, E., Karatekin, Ö., Morschhauser, A., Niles, P. B., Mousis, O., Odert, P., Möstl, U. V., Breuer, D., Dehant, V., Grott, M., Gröller, H., Hauber, E., Pham, L. B. S.
Publikováno v:
Space Sci Rev (2013) 174:113-154
The evolution and escape of the martian atmosphere and the planet's water inventory can be separated into an early and late evolutionary epoch. The first epoch started from the planet's origin and lasted $\sim$500 Myr. Because of the high EUV flux of
Externí odkaz:
http://arxiv.org/abs/1506.06569
Autor:
Wippermann, T., Hudson, T.L., Spohn, T., Witte, L., Scharringhausen, M., Tsakyridis, G., Fittock, M., Krömer, O., Hense, S., Grott, M., Knollenberg, J., Lichtenheldt, R.
Publikováno v:
In Planetary and Space Science February 2020 181
Publikováno v:
In Planetary and Space Science January 2020 180
Publikováno v:
Mon.Not.Roy.Astron.Soc.344:1119,2003
Strange mode instabilities in the envelopes of massive stars lead to shock waves, which can oscillate on a much shorter timescale than that associated with the primary instability. The phenomenon is studied by direct numerical simulation using a, wit
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309706
Publikováno v:
Mon.Not.Roy.Astron.Soc.347:481,2004
The evolution of strange mode instabilities into the non linear regime has been followed by numerical simulation for an envelope model of a massive star having solar chemical composition, M=50M_sun, T_eff=10^4K and L=1.17*10^6 L_sun. Contrary to prev
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309708