2013
DOI: 10.1002/2012jd019420
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SMILES zonal and diurnal variation climatology of stratospheric and mesospheric trace gasses: O3, HCl, HNO3, ClO, BrO, HOCl, HO2, and temperature

Abstract: [1] We present a climatology of the diurnal variation of short-lived atmospheric compounds, such as ClO, BrO, HO 2 , and HOCl, as well as longer-lived species: O 3 , the hydrogen chloride isotopes H 35 Cl and H 37 Cl, and HNO 3 . Measurements were taken by the Superconducting Submillimeter-wave Limb-Emission Sounder (SMILES). This spectrally resolving radiometer, with very low observation noise and altitude range from the lower stratosphere to the lower thermosphere (20-100 km), was measuring vertical profiles… Show more

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Cited by 18 publications
(14 citation statements)
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“…This feature is valid for all the quantities measured by SMILES (e.g. Kreyling et al, 2013). For a particular region, there is not an instantaneous complete coverage in local time and only seasonal mean variations can be derived.…”
Section: Diurnal Variationsmentioning
confidence: 73%
“…This feature is valid for all the quantities measured by SMILES (e.g. Kreyling et al, 2013). For a particular region, there is not an instantaneous complete coverage in local time and only seasonal mean variations can be derived.…”
Section: Diurnal Variationsmentioning
confidence: 73%
“…This instrument measured about 1600 profiles per day (both daytime and nighttime) within the latitude range of 38 • S-65 • N. Owing to the non-sun-synchronous orbit of the ISS, measurements of the atmosphere are taken at different local times. This data set provides unprecedented opportunities to study diurnal ozone variations throughout the stratosphere Sakazaki et al, 2013;Kasai et al, 2013;Kreyling et al, 2013).…”
Section: Smilesmentioning
confidence: 99%
“…Although solar proton and energetic electron precipitation events are known to enhance the nighttime abundance of HO x (H, OH, and HO 2) in the high‐latitude region owing to the reaction between electrons and hydrated cluster ions (Jackman et al, , ; Solomon et al, ), their activity was quite low at the low‐latitude region and during the SMILES observations that took place from 12 October 2009 to 21 April 2010 (Andersson et al, ). The diurnal variation in mesospheric HO 2 is mostly controlled by the photolysis of H 2O by sunlight (Kreyling et al, ), which only depends on the local time and lifetime of HO x species, making it incapable of producing the local enhancement. Horizontal transportation by zonal winds may impact the estimated HO 2 productions as demonstrated in Arnone et al () for nitrogen oxides.…”
Section: Ho 2 Spectral Enhancements Above Sprite‐producing Thunderstomentioning
confidence: 99%
“…The atmospheric profiles include the volume mixing ratio of HO 2, temperature, and pressure. Vertical atmospheric profiles are obtained from the averaged values of the SMILES Level‐2 research (L2r) product data Version 3.0.0, an updated version of Version 2.1.5 (Baron et al, ; Kasai et al, ; Kreyling et al, ), at adjacent observation scans. The calculated spectra are convoluted with frequency response functions of acousto‐optic spectrometers (Mizobuchi et al, ).…”
Section: Estimation Of Ho 2 Amount Produced By Sprite Eventsmentioning
confidence: 99%