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dc.contributor.authorVan Zyl, Bert
dc.date.accessioned2024-10-07T22:37:06Z
dc.date.available2024-10-07T22:37:06Z
dc.date.issued1978-11
dc.identifier.urihttp://hdl.handle.net/11122/15449
dc.descriptionUAG R-265en_US
dc.description.abstractAn analysis of the hydrogen aurora begins with a determination of the charge-state-equilibrium fractions of the proton/hydrogen atom flux traversing the atmosphere. Charge-exchange and ionization-stripping cross sections are compiled. Where no data exist, estimates of the required cross sections are made. Charge-state-equilibrium flux fractions are computed for N2, O2, and O targets. Net atmospheric charge-state-equilibrium flux fractions are then calculated as a function of altitude using the appropriate atmospheric constituent density ratios for these species.en_US
dc.description.sponsorshipPublication of this report has been made possible by the support of National Science Foundation Grant ATM76-17409 to the University of Alaska.en_US
dc.language.isoen_USen_US
dc.publisherGeophysical Institute at the University of Alaska Fairbanksen_US
dc.subjectAurorasen_US
dc.titleCharge-state-equilibrated H+/H flux fractions for analysis of the hydrogen auroraen_US
dc.typeReporten_US
refterms.dateFOA2024-10-07T22:37:08Z


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