Solar Wind Charge Exchange Studies Of Highly Charged Ions On Atomic Hydrogen

Accurate studies of low-energy charge exchange (CX) are critical to understanding underlying soft X-ray radiation processes in the interaction of highly charged ions from the solar wind with the neutral atoms and molecules in the heliosphere, cometary comas, planetary atmospheres, interstellar winds...

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Bibliographic Details
Published in:AIP conference proceedings 2011-06, Vol.1336 (1)
Main Authors: Draganic, I. N., Havener, C. C., Seely, D. G., McCammon, D.
Format: Article
Language:English
Subjects:
ATMOSPHERES
ATOM COLLISIONS
ATOMIC AND MOLECULAR PHYSICS
BEAMS
CAPTURE
CHARGE EXCHANGE
CHARGE STATES
CHARGED PARTICLES
COLLISIONS
CROSS SECTIONS
ECR ION SOURCES
ELECTROMAGNETIC RADIATION
ELECTRON CAPTURE
ELEMENTS
ENERGY RANGE
EV RANGE
FREQUENCY RANGE
GHZ RANGE
HELIOSPHERE
HYDROGEN
INTERACTIONS
ION BEAMS
ION COLLISIONS
ION SOURCES
ION-ATOM COLLISIONS
ION-MOLECULE COLLISIONS
IONIZING RADIATIONS
IONS
KEV RANGE
KEV RANGE 01-10
MOLECULE COLLISIONS
NATIONAL ORGANIZATIONS
NONMETALS
ORNL
OXYGEN IONS
PLANETARY ATMOSPHERES
RADIATIONS
SOFT X RADIATION
SOLAR ACTIVITY
SOLAR ATMOSPHERE
SOLAR WIND
STELLAR ACTIVITY
STELLAR ATMOSPHERES
STELLAR WINDS
TOTAL CROSS SECTIONS
US AEC
US DOE
US ERDA
US ORGANIZATIONS
X RADIATION
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Summary:Accurate studies of low-energy charge exchange (CX) are critical to understanding underlying soft X-ray radiation processes in the interaction of highly charged ions from the solar wind with the neutral atoms and molecules in the heliosphere, cometary comas, planetary atmospheres, interstellar winds, etc.. Particularly important are the CX cross sections for bare, H-like, and He-like ions of C, N, O and Ne, which are the dominant charge states for these heavier elements in the solar wind. Absolute total cross sections for single electron capture by H-like ions of C, N, O and fully-stripped O ions from atomic hydrogen have been measured in an expanded range of relative collision energies (5 eV/u-20 keV/u) and compared to previous H-oven measurements. The present measurements are performed using a merged-beams technique with intense highly charged ion beams extracted from a 14.5 GHz ECR ion source installed on a high voltage platform at the Oak Ridge National Laboratory. For the collision energy range of 0.3 keV/u-3.3 keV/u, which corresponds to typical ion velocities in the solar wind, the new measurements are in good agreement with previous H-oven measurements. The experimental results are discussed in detail and compared with theoretical calculations where available.
ISSN:0094-243X
1551-7616
DOI:10.1063/1.3586067