Simultaneous observations of neutral and ionic magnesium in the thermosphere

Earth‐limb observations by the GLO instrument aboard space shuttle mission STS‐53 include the first simultaneous resonant‐scattering detection of Mg+ (279.6–280.3 nm) and neutral Mg (285.2 nm) in the thermosphere. Although Mg+ emissions are observed in approximately 45% of GLO scans over a wide geog...

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Published inGeophysical research letters Vol. 22; no. 16; pp. 2119 - 2122
Main Authors Gardner, James A., Viereck, Rodney A., Murad, Edmond, Knecht, David J., Pike, C. P., Broadfoot, A. Lyle, Anderson, Emmet R.
Format Journal Article
LanguageEnglish
Published Washington, DC Blackwell Publishing Ltd 15.08.1995
American Geophysical Union
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Summary:Earth‐limb observations by the GLO instrument aboard space shuttle mission STS‐53 include the first simultaneous resonant‐scattering detection of Mg+ (279.6–280.3 nm) and neutral Mg (285.2 nm) in the thermosphere. Although Mg+ emissions are observed in approximately 45% of GLO scans over a wide geographic and local‐time range, neutral Mg is observed in fewer than 1% of the measurements, and most of these sightings occur on two consecutive orbits in a near‐equatorial patch at local dusk. Neutral Mg is observed at tangent heights between 150 and 230 km, with an instrument‐view‐column density of 0.4–1.4 × 108 cm−2, compared with simultaneous Mg+ values of 1.4–5.8 × 109 cm−2. Calculated in‐cloud densities are [Mg+] ∼250 cm−3 and [Mg] ∼5 cm−3, and the average ratio of [Mg+] to [Mg] in the individual measurements is 34:1.
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ISSN:0094-8276
1944-8007
DOI:10.1029/95GL01769