X-ray Emission from Charge Exchange of Highly Charged Ions in Atoms and Molecules
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Engineering topics
Publications and source records attributed to Smith, S..
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X-ray emission from a comet was observed for the first time in 1996. One of the mechanisms believed to be contributing to this surprisingly strong emission is the interaction of highly charged solar wind ions with cometary gases.
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Radiative Eistein A-values have been measured for fine structure transistions in the intercombination 2s(sup 2)2p (sup 2p)(sup 0) decay in C(sup +).
Experimental and theoretical collisional excitation cross sections are reported for the 3s square 3p- 3s3p cube 5S to the zero spin-forbidden transition in S square+.
In the experimental approach, use is made of the electron energy-loss method with merged electron and ion beams.
A new 14.0 GHz electron-cyclotron resonance ion source, the so-called Caprice source, has been in operation at JPL/Caltech for over a year.
Experimental cross sections are reported for electron excitation of the allowed 2s (sup 2)S 2p - (sup 2)P transition in C(sup 3+).
During recent high altitude flights, we have tested the aerosol section of the fast flow flight cascade impactor quartz crystal microbalance (QCM) on loan to Howard University from NASA. The aerosol mass collected during these flights was disappointingly small. Increasing the flow through the QCM did not correct the problem. It was clear that the instrument was not being operated under proper conditions for aerosol collect ion primarily because the gas dynamics is not well understood. A laboratory study was therefore undertaken using two different fast flow QCM's in an attempt to establish the gas flow characteristics of the aerosol sections and its effect on particle collection, Some tests were made at low temperatures but most of the work reported here was carried out at room temperature. The QCM is a cascade type impactor originally designed by May (1945) and later modified by Anderson (1966) and Mercer et al (1970) for chemical gas analysis. The QCM has been used extensively for collecting and sizing stratospheric aerosol particles. In this paper all flow rates are given or corrected and referred to in terms of air at STP. All of the flow meters were kept at STP. Although there have been several calibration and evaluation studies of moderate flow cascade impactors of less than or equal to 1 L/rein., there is little experimental information on the gas flow characteristics for fast flow rates greater than 1 L/rein.
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Experimental and theoretical excitation cross sections are reported for the first forbidden transition xxx and the first allowed (resonance) transition xxx in OII. Use is made of electron-energy loss and merged beams methods. The electron energy range covered is 3.33 eV (threshold) to 15 eV for the S->D transition, and 14.9 eV (threshold) to 40 eV for the S->P transition. Care was taken to assess and minimize the metastable fraction of the OII beam. An electron mirror was designed and tested to reflect inelastically back-scattered electrons into the forward direction to account for the full range of polar scattering angles. Comparisons are made between present experiments and 11-state R-Matrix calculations. Calculations are also presented for the xxx transition.
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Psychological and physiological effects of long-term isolation and confinement and project RIM experimental design