To the development of the mechanism of interaction of galactic comets with the terrestrial planets the physical processes at once. At that, with a decrease of power of
gaseous envelope of
planet, the action
To the development of the mechanism of interaction of galactic comets with the terrestrial planets the physical processes at once. At that, with a decrease of power of
gaseous envelope of
planet, the action
Overcoming the Limitations of the Energy-limited Approximation for Planet Atmospheric EscapeKubyshkina, D.,
Fossati, L.,
Erkaev, N. V.,
Cubillos, P. E.,
Johnstone, C. P.,
Kislyakova, K. G.,
Lammer, H.,
Lendl, M.,
Odert, P. -atmosphere hydrodynamic models computed for a wide range of
planets with hydrogen-dominated atmospheres from which we
Modeling the Ly alpha transit absorption of the hot Jupiter HD 189733bOdert4, P.,
Erkaev, N. V.,
Kislyakova, K. G.,
Lammer, H.,
Mezentsev, A. V.,
Ivanov, V. A.,
Fossati, L.,
Leitzinger, M.,
Kubyshkina, D.,
Holmström, M. absorption of neutral hydrogen has been observed in the Lyα line during transits of several close-in
gaseous Modeling the Lyα transit absorption of the hot Jupiter HD 189733b=Modeling the Ly alpha transit absorption of the hot Jupiter HD 189733bOdert, P.,
Erkaev, N. V.,
Kislyakova, K. G.,
Lammer, H.,
Mezentsev, A. V.,
Ivanov, V. A.,
Fossati, L.,
Leitzinger, M.,
Kubyshkina, D.,
Holmström, M. absorption of neutral hydrogen has been observed in the
Lyα line during transits of several close-in
gaseous Effect of changes in gaseous environment and temperature on animals with diabetesIn contrast to normal environmental conditions (normal temperature and
gaseous composition
Novel position-sensitive gaseous detectors with solid photocathodesCurrently, a revolution is happening in the development of
gaseous detectors of photons
Grid of upper atmosphere models for 1-40 M⊕ planets: application to CoRoT-7 b and HD 219134 b,cKubyshkina, D.,
Fossati, L.,
Erkaev, N. V.,
Johnstone, C. P.,
Cubillos P. E. La,
Kislyakova, K. G.,
Lammer, H.,
Lendl, M.,
Odert, P. to produce a large grid of about 7000 models covering
planets with masses 1-39 M⊕ with hydrogen