63 results on '"Lammer H"'
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2. Escape of rock-forming volatile elements and noble gases from planetary embryos
3. Constraining the early evolution of Venus and Earth through atmospheric Ar, Ne isotope and bulk K/U ratios
4. A mathematical model of quasistationary electric field penetration from ground to the ionosphere with inclined magnetic field
5. Escape and fractionation of volatiles and noble gases from Mars-sized planetary embryos and growing protoplanets
6. Water-rich planets: How habitable is a water layer deeper than on Earth?
7. Monte-Carlo simulation of Callisto’s exosphere
8. 3D-modeling of Mercury's solar wind sputtered surface-exosphere environment
9. Hot oxygen and carbon escape from the martian atmosphere
10. Escape of the martian protoatmosphere and initial water inventory
11. A neutral gas mass spectrometer for the investigation of lunar volatiles
12. Is hydrodynamic escape from Titan possible?
13. Could CoRoT-7b and Kepler-10b be remnants of evaporated gas or ice giants?
14. Comet-like tail-formation of exospheres of hot rocky exoplanets: Possible implications for CoRoT-7b
15. Non-thermal water loss of the early Mars: 3D multi-ion hybrid simulations
16. Self-consistent modelling of Mercury’s exosphere by sputtering, micro-meteorite impact and photon-stimulated desorption
17. Aeronomical evidence for higher CO 2 levels during Earth’s Hadean epoch
18. Titan’s atomic hydrogen corona
19. A comparison of global models for the solar wind interaction with Mars
20. Hybrid simulations of the O + ion escape from Venus: Influence of the solar wind density and the IMF x component
21. On the protection of extrasolar Earth-like planets around K/M stars against galactic cosmic rays
22. On the impact of multiply charged heavy solar wind ions on the surface of Mercury, the Moon and Ceres
23. Mass loss from “Hot Jupiters”—Implications for CoRoT discoveries, Part II: Long time thermal atmospheric evaporation modeling
24. The Venusian induced magnetosphere: A case study of plasma and magnetic field measurements on the Venus Express mission
25. Mars Express and Venus Express multi-point observations of geoeffective solar flare events in December 2006
26. Comparative analysis of Venus and Mars magnetotails
27. First observation of energetic neutral atoms in the Venus environment
28. Location of the bow shock and ion composition boundaries at Venus—initial determinations from Venus Express ASPERA-4
29. Response of bacteriophage T7 biological dosimeter to dehydration and extraterrestrial solar UV radiation
30. Mass loss of “Hot Jupiters”—Implications for CoRoT discoveries. Part I: The importance of magnetospheric protection of a planet against ion loss caused by coronal mass ejections
31. The lunar exosphere: The sputtering contribution
32. Could we identify hot ocean-planets with CoRoT, Kepler and Doppler velocimetry?
33. Loss of hydrogen and oxygen from the upper atmosphere of Venus
34. Atmospheric and water loss from early Venus
35. Magnetic field investigation of the Venus plasma environment: Expected new results from Venus Express
36. A comparison of magnetohydrodynamic instabilities at the Martian ionopause
37. DNA damage under simulated extraterrestrial conditions in bacteriophage T7
38. The influence of the solar particle and radiation environment on Titan’s atmosphere evolution
39. Energy dissipation of possible Titan lightning strokes
40. Annual solar UV exposure and biological effective dose rates on the Martian surface
41. Simulation experiments of the effect of space environment on bacteriophage and DNA thin films
42. Biological UV dosimeters in simulated space conditions
43. Possible temperature effects of energetic neutral hydrogen atoms on the Martian exosphere
44. Ion loss on Mars caused by the Kelvin–Helmholtz instability
45. The variability of Mercury's exosphere by particle and radiation induced surface release processes
46. Mapping of the cusp plasma precipitation on the surface of Mercury
47. Loss of water from Mars:: Implications for the oxidation of the soil
48. Modelling of thunderclouds and lightning generation on Titan
49. Lightning activity on Titan: can Cassini detect it?
50. Ionospheric layer induced by meteoric ionization in Titan's atmosphere
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