Results 31 to 40 of about 3,054,495 (336)
Impact of accounting of 238U chemical toxicity on its permissible release level to atmosphere
Радиационная гигиена, 2021 At present, the permissible atmospheric release levels of 238U are evaluated only on a basis of its radiation impact on population. At the same time, uranium belongs to the 1st hazard class (extremely dangerous chemicals) by its toxic effect.
A. I. Kryshev +2 more
doaj +1 more source
Atmosphere, 2015 The published date in the paper [1] should be 23 November 2015. We apologize to the authors of the paper and readers of Atmosphere for any inconvenience caused. [...]
Atmosphere Editorial Office
doaj +1 more source
Atmospheric Correction for High-Resolution Shape from Shading on Mars
Journal of Imaging, 2022 Digital Elevation Models (DEMs) of planet Mars are crucial for many remote sensing applications and for landing site characterization of rover missions.
Marcel Hess +3 more
doaj +1 more source
Correction: Recent Advances in Atmospheric Chemistry of Mercury
Atmosphere, 2018 The published paper [1] has been updated to remove instances of copied text from other publications [2–6].[...]
Lin Si +2 more
doaj +1 more source
Mars Exploration Using Sailplanes
Aerospace, 2022 We present the preliminary design of sailplanes, used for Mars exploration. The sailplanes mitigate the weight and energy storage limitations traditionally associated with powered flight by instead exploiting atmospheric wind gradients for dynamic ...
Adrien Bouskela +5 more
doaj +1 more source
Helium Atmospheres on Warm Neptune- and Sub-Neptune-Sized Exoplanets and Applications to GJ 436 b [PDF]
, 2015 Warm Neptune- and sub-Neptune-sized exoplanets in orbits smaller than Mercury's are thought to have experienced extensive atmospheric evolution. Here we propose that a potential outcome of this atmospheric evolution is the formation of helium-dominated ...
Hu, Renyu, Seager, Sara, Yung, Yuk L.
core +3 more sources
New Journal of Physics, 2004 Atmospheric neutrinos are produced as decay products in hadronic showers resulting from collisions of cosmic rays with nuclei in the atmosphere. Electron-neutrinos and muon-neutrinos are produced mainly by the decay chain of charged pions to muons to electrons.
openaire +2 more sources
Dependence of cosmic ray component in background of atmosphere surface from solar magnetic activity
Vestnik KRAUNC: Fiziko-Matematičeskie Nauki, 2021 Using Geant4 toolkit the changes of the flux density and of the dose rates of the secondary cosmic radiation at the heights up to 50 m from the land surface (at a depth of atmosphere about 1030 g/cm²) and depending on solar magnetic activity were ...
Zelinskiy, A.S., Yakovlev, G.A.
doaj +1 more source
Detection of CO in Triton's atmosphere and the nature of surface-atmosphere interactions
, 2010 Triton possesses a thin atmosphere, primarily composed of nitrogen, sustained by the sublimation of surface ices. The goal is to determine the composition of Triton's atmosphere and to constrain the nature of surface-atmosphere interactions.
de Bergh, C. +4 more
core +2 more sources
Nuclear Physics B - Proceedings Supplements, 2000 To be published in the proceedings of TAUP99 Conference College de France - Paris 6-10 September 1999 11 pages 12 ...
openaire +2 more sources