Zobrazeno 1 - 10
of 47
pro vyhledávání: '"I. B. Miroshnichenko"'
Autor:
A. G. Berezutsky, A. A. Chibranov, M. A. Efimov, V. G. Posukh, M. S. Rumenskikh, P. A. Trushin, I. B. Miroshnichenko, Yu. P. Zakharov, V. A. Terekhin, I. F. Shaikhislamov
Publikováno v:
Plasma Physics Reports. 49:351-361
Publikováno v:
Astronomy Reports. 67:272-279
Autor:
A G Berezutsky, I F Shaikhislamov, M S Rumenskikh, M L Khodachenko, H Lammer, I B Miroshnichenko
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 515:706-715
We simulate with a global 3D aeronomy code two warm Neptunes in the TOI-421 system and show that both planets experience significant escape of their upper atmospheres. The double shock structures, generated around the planets in course of their inter
Autor:
A. A. Chibranov, A. G. Berezutsky, M. A. Efimov, Y. P. Zakharov, I. B. Miroshnichenko, V. G. Posukh, M. S. Rumenskikh, P. A. Trushin, I. F. Shaikhislamov
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 86:830-832
Autor:
M. S. Rumenskikh, M. A. Efimov, I. F. Shaikhislamov, V. G. Posukh, A. A. Chibranov, P. A. Trushin, Yu. P. Zakharov, I. B. Miroshnichenko, A. G. Berezutsky, E. V. Smolina, E. L. Boyarintsev
Publikováno v:
Quantum Electronics. 51:222-227
We describe an experiment on the interaction of a dipolar magnetic field with the laser plasma flow produced inside of a laboratory magnetosphere. This interaction is found to exhibit two dynamic stages: after a prompt displacement of the dipole fiel
Autor:
I. F. Shaikhislamov, Luca Fossati, Maxim L. Khodachenko, I. B. Miroshnichenko, Helmut Lammer, A. G. Berezutsky, M. A. Efimof, M. S. Rumenskikh
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 503:L23-L27
Transmission spectroscopy of WASP-107b revealed 7-8% absorption at the position of metastable HeI triplet at 10830 {\AA} in Doppler velocity range of [-20; 10] km/s, which is stronger than that measured in other exoplanets. With a dedicated 3D self-c
Autor:
I. F. Shaikhislamov, I. B. Miroshnichenko, M. S. Rumenskikh, A. G. Berezutskii, E. S. Vetrova
Publikováno v:
Astronomy Reports. 65:61-69
Simulation results are presented for the Lyα flux impact from the parent star on the Hα absorption spectrum in the atmospheres of the hot Jupiters HD189733b and HD 209458b. The atmosphere is simulated using a three-dimensional hydrodynamic code. Se
Autor:
L. Fossati, G. Guilluy, I. F. Shaikhislamov, I. Carleo, F. Borsa, A. S. Bonomo, P. Giacobbe, M. Rainer, C. Cecchi-Pestellini, M. L. Khodachenko, M. A. Efimov, M. S. Rumenskikh, I. B. Miroshnichenko, A. G. Berezutsky, V. Nascimbeni, M. Brogi, A. F. Lanza, L. Mancini, L. Affer, S. Benatti, K. Biazzo, A. Bignamini, D. Carosati, R. Claudi, R. Cosentino, E. Covino, S. Desidera, A. Fiorenzano, A. Harutyunyan, A. Maggio, L. Malavolta, J. Maldonado, G. Micela, E. Molinari, I. Pagano, M. Pedani, G. Piotto, E. Poretti, G. Scandariato, A. Sozzetti, H. Stoev
The hot Jupiter WASP-80b has been identified as a possible excellent target for detecting and measuring HeI absorption in the upper atmosphere. We observed 4 primary transits of WASP-80b in the optical and near-IR using the HARPS-N and GIANO-B high-r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e244505d36cd197ca22ff26ac81b1566
http://wrap.warwick.ac.uk/163997/1/WRAP-The-GAPS-Programme-TNG-2022.pdf
http://wrap.warwick.ac.uk/163997/1/WRAP-The-GAPS-Programme-TNG-2022.pdf
Autor:
M. S. Rumenskikh, I. F. Shaikhislamov, M. L. Khodachenko, H. Lammer, I. B. Miroshnichenko, A. G. Berezutsky, L. Fossati
A 3D fully self-consistent multifluid hydrodynamic aeronomy model is applied to simulate the hydrogen-helium expanding upper atmosphere of the hot Jupiter HD189733b, and related absorption in the Lyα line and the 10830 Å line of metastable helium.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e6901feedda02d44b6af6c00fcdc08c1
Autor:
A. G. Berezutsky, A. G. Ponomarenko, A. A. Chibranov, V. N. Tischenko, M. A. Efimov, V. G. Posukh, Yu. P. Zakharov, I. B. Miroshnichenko, I. F. Shaikhislamov
Publikováno v:
Bulletin of the Russian Academy of Sciences: Physics. 84:803-806
The limiting mode of the generation of low-frequency torsional whistlers is obtained for the first time. Laser plasma clouds create only weak whistlers in a weakly magnetized laboratory plasma (argon), allowing the whistler magnetic field to reach re