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相关论文: Neutral particle release from Europa's surface

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The Neutral beam Injectors of the ITER experiment will be based on negative ion sources for the generation of beams composed by 1 MeV H/D particles. The prototype of these sources is currently under testing in the SPIDER experiment, part of…

等离子体物理 · 物理学 2023-08-30 M. Barbisan , R. Agnello , G. Casati , R. Pasqualotto , E. Sartori , G. Serianni

Ionizing stellar photons heat the upper regions of planetary atmospheres, driving atmospheric mass loss. Gas escaping from several hot, hydrogen-rich planets has been detected using UV and X-ray transmission spectroscopy. Because these…

太阳与恒星天体物理 · 物理学 2015-08-05 Anjali Tripathi , Kaitlin M. Kratter , Ruth A. Murray-Clay , Mark R. Krumholz

The SPIDER experiment, part of the Neutral Beam Test Facility (NBTF) at Consorzio RFX (Padua, Italy), is the prototype of the negative ion source for the ITER neutral beam injectors; the source is coupled to a 100 kV three-grid acceleration…

等离子体物理 · 物理学 2023-04-07 M. Barbisan , B. Zaniol , R. Pasqualotto , G. Serianni , M. Ugoletti

H$_3^+$ emission is the dominant cooling mechanism in Jupiter's thermosphere and a useful probe of temperature and ion densities. The H$_3^+$ ion is predicted to form in the thermospheres of close-in `hot Jupiters' where its emission would…

天体物理学 · 物理学 2008-11-26 Evgenya Shkolnik , Eric Gaidos , Nick Moskovitz

Jupiter's moon Io hosts a dynamic atmosphere that is continually stripped off and replenished through frost sublimation and volcanic outgassing. We observed an emission band at 1.707 $\mu$m thought to be produced by hot SO molecules…

地球与行星天体物理 · 物理学 2018-08-13 Katherine de Kleer , Imke de Pater , Máté Ádámkovics

We have studied molecular hydrogen emission in a sample of 21 YSOs using spectra obtained with the Infrared Space Observatory (ISO). H2 emission was detected in 12 sources and can be explained as arising in either a shock, caused by the…

天体物理学 · 物理学 2007-05-23 M. E. van den Ancker , P. R. Wesselius , A. G. G. M. Tielens

Direct and statistical observational evidences suggest that photoevaporation is important in eroding the atmosphere of sub-Neptune planets. We construct full hydrodynamic simulations, coupled with consistent thermochemistry and ray-tracing…

地球与行星天体物理 · 物理学 2018-07-11 Lile Wang , Fei Dai

Ion Beam Sputtering (IBS) is a cost-effective technique able to produce ordered nanopatterns on the surfaces of different materials. To date, most theoretical studies of this process have focused on systems which become amorphous under…

介观与纳米尺度物理 · 物理学 2016-05-04 Javier Renedo , Javier Muñoz-García , Mario Castro , Rodolfo Cuerno

Europa has been modified by a variety of geologic processes, exposing internally-derived materials that are heavily irradiated by charged particles trapped in Jupiter's magnetosphere. Prior spectral analysis of H2O ice on Europa relied on…

Low energy ion scattering is a technique to detect the energy of ions which are scattered from a surface. For noble gas ions, it is predominantly sensitive to the topmost surface layer due to strong neutralisation processes. Depending on…

材料科学 · 物理学 2021-09-07 H. R. Koslowski , Ch. Linsmeier

A multiphysics simulation model incorporating a sintering model coupled with the MultIHeaTS thermal solver was developed to study the evolution of icy moons' microstructure. The sintering process is highly dependent on temperature, and this…

地球与行星天体物理 · 物理学 2024-10-22 Cyril Mergny , Frédéric Schmidt

Io is the most volcanically active body in the Solar System. This volcanic activity results in the ejection of material into Io's atmosphere, which may then escape from the atmosphere to form various structures in the jovian magnetosphere,…

The ion energy distribution functions (IEDF) have been measured for a helium atmospheric pressure dielectric barrier discharge jet expanding into the air and impacting a metal or ceramic surface. The plasma jet produces ionization waves as…

等离子体物理 · 物理学 2025-05-13 Daniel Henze , Laura Chauvet , Achim von Keudell

The detections of atomic hydrogen, heavy atoms and ions surrounding the extrasolar giant planet (EGP) HD209458b constrain the composition, temperature and density profiles in its upper atmosphere. Thus the observations provide guidance for…

地球与行星天体物理 · 物理学 2015-06-11 T. T. Koskinen , M. J. Harris , R. V. Yelle , P. Lavvas

Diamond is a promising candidate for enhancing the negative-ion surface production in the ion sources for neutral injection in fusion reactors; hence evaluation of its reactivity towards hydrogen plasma is of high importance. High quality…

等离子体物理 · 物理学 2019-10-14 D. Kogut , D. Aussems , N. Ning , K. Bystrov , A. Gicquel , J. Achard , O. Brinza , Y. Addab , C. Martin , C. Pardanaud , S. Khrapak , G. Cartry

Thanks to the \textit{Cassini} spacecraft onboard instruments, it has been known that Titan's ionospheric chemistry is complex and the molecular growth is initiated through the photolysis of the most abundant species directly in the upper…

地球与行星天体物理 · 物理学 2020-01-08 Jérémy Bourgalais , Nathalie Carraso , Ludovic Vettier , Pascal Pernot

The evolution of Europa's water-product exosphere over its 85-hour day, based on current models, has not been shown to exhibit any diurnal asymmetries. Here we simulate Europa's exosphere using a 3-D Monte Carlo routine including, for the…

We constrain Europa's tenuous atmosphere on the subsolar hemisphere by combining two sets of observations: oxygen emissions at 1304 {\AA} and 1356 {\AA} from Hubble Space Telescope (HST) spectral images, and Galileo magnetic field…

空间物理 · 物理学 2022-11-16 Sebastian Cervantes , Joachim Saur

The dynamics of H atom recombination on materials of interest for a EUV lithographer was studied under a longterm low-pressure H2 plasma exposure. The similarity of the experimental plasma with the typical EUV-induced plasma over the…

等离子体物理 · 物理学 2022-11-30 V. Gubarev , D. Lopayev , A. Zotovich , M. A. Blauw , V. Medvedev , P. Krainov , D. Astakhov , S. Zyryanov

The measured neutron flux from the Moons south polar region shows evidence of locally enhanced hydrogen concentrations, likely in the form of water ice, within most permanently shadowed regions (PSR), poleward of 77 deg S latitude. Results…