Results 31 to 40 of about 3,424,751 (303)

Distribution of O+ and \begin{document}${\text{O}}_{\text{2}}^{\text{+}}$\end{document} fluxes and their escape rates in the near-Mars magnetotail: A survey of MAVEN observations

open access: yesEarth and Planetary Physics, 2022
Tailward ion outflows in the Martian-induced magnetotail are known to be one of the major channels for Martian atmospheric escape. On the basis of nearly 6.5 years of observations from the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission, we ...
HengLe Du   +7 more
doaj   +1 more source

The freeze-out mechanism and phase-space density in ultrarelativistic heavy-ion collisions [PDF]

open access: yes, 2002
We explore the consequences of a freeze-out criterion for heavy-ion collisions, based on pion escape probabilities from the hot and dense but rapidly expanding collision region.
B. Tomášik   +26 more
core   +2 more sources

Solar forcing and planetary ion escape from Mars [PDF]

open access: yesGeophysical Research Letters, 2008
The variability of planetary ion escape from Mars is studied using data from the Ion Mass Analyzer, IMA, on Mars Express (MEX). 42 orbits were selected during 17 months for different solar wind conditions, focusing on the low energy (≈30 – 800 eV) heavy ion (e.g. O+, O2+ and CO2+) outflow. A strong correlation is found between solar wind forcing of the
R. Lundin   +6 more
openaire   +1 more source

Observations of fast anisotropic ion heating, ion cooling, and ion recycling in large-amplitude drift waves [PDF]

open access: yes, 1998
Large-amplitude drift wave fluctuations are observed to cause severe ion temperature oscillations in plasmas of the Caltech Encore tokamak [J. M. McChesney, P. M. Bellan, and R. A. Stern, Phys. Fluids B 3, 3370 (1991)]. Experimental investigations of the
Bellan, P. M.   +2 more
core   +2 more sources

IMF-induced escape of molecular ions from the Martian ionosphere [PDF]

open access: yesAnnales Geophysicae, 2013
Since Mars does not possess a significant global intrinsic magnetic field, the solar wind interacts directly with the Martian ionosphere and can induce ion escapes from it.
Y. Kubota   +3 more
doaj   +1 more source

Production and Characterization of Molecular Dications: Experimental and Theoretical Efforts

open access: yesMolecules, 2020
Molecular dications are doubly charged cations of importance in flames, plasma chemistry and physics and in the chemistry of the upper atmosphere of Planets.
Stefano Falcinelli, Marzio Rosi
doaj   +1 more source

Pickup ion measurements by MAVEN: A diagnostic of photochemical oxygen escape from Mars [PDF]

open access: yes, 2014
A key process populating the oxygen exosphere at Mars is the dissociative recombination of ionospheric O 2 + , which produces fast oxygen atoms, some of which have speeds exceeding the escape speed and thus contribute to atmospheric loss.
A. F. Nagy   +52 more
core   +1 more source

Reionization constraints using Principal Component Analysis [PDF]

open access: yes, 2010
Using a semi-analytical model developed by Choudhury & Ferrara (2005) we study the observational constraints on reionization via a principal component analysis (PCA).
Andrea Ferrara   +43 more
core   +7 more sources

Survey of pickup ion signatures in the vicinity of Titan using CAPS/IMS [PDF]

open access: yes, 2016
Pickup ion detection at Titan is challenging because ion cyclotron waves are rarely detected in the vicinity of the moon. In this work, signatures left by freshly produced pickup heavy ions (m/q ∼ 16 to m/q ∼ 28) as detected in the plasma data by the ...
Coates, AJ   +7 more
core   +1 more source

The Venusian Atmospheric Oxygen Ion Escape: Extrapolation to the Early Solar System

open access: yesJournal of Geophysical Research: Planets, 2020
The present atmosphere of Venus contains almost no water, but recent measurements indicate that in its early history, Venus had an Earth‐like ocean. Understanding how the Venusian atmosphere evolved is important not only for Venus itself but also for ...
M. Persson   +7 more
semanticscholar   +1 more source

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