Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Federico Lavorenti"'
Autor:
Federico Lavorenti, Elizabeth A. Jensen, Sae Aizawa, Francesco Califano, Mario D’Amore, Deborah Domingue, Pierre Henri, Simon Lindsay, Jim M. Raines, Daniel Wolf Savin
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 9, p 163 (2023)
Mercury is the closest planet to the Sun, possesses a weak intrinsic magnetic field, and has only a very tenuous atmosphere (exosphere). These three conditions result in a direct coupling between the plasma emitted from the Sun (namely, the solar win
Externí odkaz:
https://doaj.org/article/735c4e67d7a547829afd7742433296ab
Autor:
Federico Lavorenti, Pierre Henri, Francesco Califano, Jan Deca, Sae Aizawa, Nicolas André, Simon Lindsay, Johannes Benkhoff
Mercury is the only telluric planet of the solar system, other than Earth, with an intrinsic magnetic field. Thus, the Hermean surface is shielded from the impinging solar wind via an “Earth-like” magnetosphere. This magnetic cavity is however tw
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e9a8492483cadb0cce9be7e3372d3a0d
https://doi.org/10.5194/epsc2022-848
https://doi.org/10.5194/epsc2022-848
Autor:
Pietro Dazzi, Pierre Henri, Luca Bucciantini, Federico Lavorenti, Gaetan Wattieaux, Francesco Califano
Mutual impedance experiments are active electric instruments that provide in situ diagnostic in space plasmas, such as the plasma density and electron temperature. The instrumental technique is based on the coupling between electric antennas embedded
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1b3bacbad2f033bc999be103ee1e53d7
https://doi.org/10.5194/epsc2022-1091
https://doi.org/10.5194/epsc2022-1091
Mercury is the only telluric planet of the solar system, other than Earth, with an intrinsic magnetic field. Thus, the Hermean surface is shielded from the impinging solar wind via the presence of an “Earth-like” magnetosphere. However, this cavi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fe1e35959b707436a0ec96043061a27d
https://doi.org/10.5194/egusphere-egu22-62
https://doi.org/10.5194/egusphere-egu22-62
Publikováno v:
Europlanet Science Congress 2021
Europlanet Science Congress 2021, Sep 2021, Virtual Congress, France. pp.EPSC2021-10
HAL
Europlanet Science Congress 2021, Sep 2021, Virtual Congress, France. pp.EPSC2021-10
HAL
Density inhomogeneities are ubiquitous in space and astrophysical plasmas, in particular at contact boundaries between different media. They often correspond to regions that exhibits strong dynamics on a wide range of spatial and temporal scales. Ind
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6210220d183ac59af447f7fa58b29ec3
https://doi.org/10.5194/epsc2021-10
https://doi.org/10.5194/epsc2021-10
Magnetic reconnexion and Kelvin-Helmholtz (KH) instability are usually recognized as the two main mixing processes along magnetopauses. However, a recent work [Dargent et al., 2019] showed that in Mercury’s conditions, another instability can grow
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bed4ba8c05ab431bc5765225441c6f63
https://doi.org/10.5194/egusphere-egu21-9413
https://doi.org/10.5194/egusphere-egu21-9413
Density inhomogeneities are ubiquitous in space and astrophysical plasmas, in particular at contact boundaries between different media. They often correspond to regions that exhibits strong dynamics on a wide range of spatial and temporal scales. Ind
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ab7aec0d8b504189de89e7c437c068f