about
First observation of a mini-magnetosphere above a lunar magnetic anomaly using energetic neutral atomsMartian atmospheric erosion rates.Cometary science. Birth of a comet magnetosphere: a spring of water ions.Low energy neutral atom imaging on the Moon with the SARA instrument aboard Chandrayaan-1 missionCharacteristics of proton velocity distribution functions in the near-lunar wake from Chandrayaan-1/SWIM observationsEffects of the crustal magnetic fields on the Martian atmospheric ion escape rateEmission of energetic neutral atoms from water ice under Ganymede surface-like conditionsScattering characteristics and imaging of energetic neutral atoms from the Moon in the terrestrial magnetosheathThe electric wind of Venus: A global and persistent “polar wind”-like ambipolar electric field sufficient for the direct escape of heavy ionospheric ionsLow-energy energetic neutral atom imaging of Io plasma and neutral toriThe Martian atmospheric ion escape rate dependence on solar wind and solar EUV conditions: 1. Seven years of Mars Express observationsThe impact of a slow interplanetary coronal mass ejection on VenusBackscattered energetic neutral atoms from the Moon in the Earth's plasma sheet observed by Chandarayaan-1/Sub-keV Atom Reflecting Analyzer instrumentChandrayaan-1 observations of backscattered solar wind protons from the lunar regolith: Dependence on the solar wind speedPhobos 2/ASPERA data revisited: Planetary ion escape rate from Mars near the 1989 solar maximumStatistical properties of planetary heavy-ion precipitations toward the Martian ionosphere obtained from Mars ExpressKinetic simulations of finite gyroradius effects in the lunar plasma environment on global, meso, and microscalesErratum to “Extremely high reflection of solar wind protons as neutral hydrogen atoms from regolith in space” [Planet. Space Sci. 57 (2009) 2132–2134]Heavy ion escape from Mars, influence from solar wind conditions and crustal magnetic fieldsStrong influence of lunar crustal fields on the solar wind flowIon escape from Mars as a function of solar wind conditions: A statistical studyExtremely high reflection of solar wind protons as neutral hydrogen atoms from regolith in spaceEnergetic neutral atom imaging mass spectroscopy of the Moon and Mercury environmentsLow energy neutral atoms imaging of the MoonA new view on the solar wind interaction with the MoonStudying the Lunar—Solar Wind Interaction with the SARA Experiment aboard the Indian Lunar Mission Chandrayaan-1Uranus Pathfinder: exploring the origins and evolution of Ice Giant planetsSolar Wind Interaction and Impact on the Venus AtmosphereHybrid simulations of proton precipitation patterns onto the upper atmosphere of MarsMagnetized Mars: Spatial distribution of oxygen ionsAtmospheric effects of precipitating energetic hydrogen atoms on the Martian atmosphereX-ray imaging of the solar wind-Mars interactionOn the elastic and inelastic collisions between precipitating energetic hydrogen atoms and Martian atmospheric neutralsSELMA mission: How do airless bodies interact with space environment? The Moon as an accessible laboratoryProperties of a large-scale flux rope and current sheet region on the dayside of Mars: MGS MAG/ER and MEX ASPERA-3 ELS observationsElectron optical study of the Venus Express ASPERA-4 Electron Spectrometer (ELS) top-hat electrostatic analyserAn induced global magnetic field looping around the magnetotail of VenusIMF control of the location of Venusian bow shock: The effect of the magnitude of IMF component tangential to the bow shock surfaceCallisto plasma interactions: Hybrid modeling including induction by a subsurface ocean
P50
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P50
name
Stas Barabash
@en
Stas Barabash
@nl
type
label
Stas Barabash
@en
Stas Barabash
@nl
prefLabel
Stas Barabash
@en
Stas Barabash
@nl