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dc.contributor.authorNicolet, M.
dc.date1975
dc.date.accessioned2017-08-31T12:18:32Z
dc.date.available2017-08-31T12:18:32Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/6065
dc.descriptionNitric oxide is formed in the atmosphere through the ionization and dissociation of molecular nitrogen by galactic cosmic rays. One NO molecule is formed for each ion pair produced by cosmic ray ionization. The height-integrated input (day and night) to the lower stratosphere is of the order of 6 × 107 NO molecules cm-2/sec in the auroral zone (geomagnetic latitude Φ ≥ 60°) during the minimum of the sunspot cycle and 4 × 107 NO molecules cm-2/sec in the subauroral belt and auroral region (Φ≥ 45°) at the maximum of solar activity. The tropical production is less than 10-7 NO molecules cm-2/sec above 17 km and at the equator the production is only 3 × 106NO molecules cm-2/sec.
dc.languageeng
dc.titleOn the production of nitric oxide by cosmic rays in the mesosphere and stratosphere
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.source.titlePlanetary and Space Science
dc.source.volume23
dc.source.issue4
dc.source.page637-649
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/0032-0633(75)90104-X
dc.identifier.scopus2-s2.0-0001538194


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