Validation of stratospheric and mesospheric ozone observed by SMILES from International Space Station

@inproceedings{Kasai2013ValidationOS,
  title={Validation of stratospheric and mesospheric ozone observed by SMILES from International Space Station},
  author={Yasuko Kasai and Hiroyuki Sagawa and Daniel Kreyling and Eric Dupuy and Philippe Baron and Jana Mendrok and Kentaroh Suzuki and Tatiana de Oliveira Sato and Toshiyuki Nishibori and Satoko Mizobuchi and Kenichi Kikuchi and Takeshi Manabe and Hiroyuki Ozeki and Takafumi Sugita and Masatomo Fujiwara and Yoshihisa Irimajiri and Kaley A. Walker and Peter F. Bernath and Chris D. Boone and Gabriele P. Stiller and Thomas von Clarmann and Johannes Orphal and Joachim Urban and Donal Murtagh and Edward J. Llewellyn and D. A. DegensteinD.A. Degenstein and Adam E. Bourassa and N. D. LloydN.D. Lloyd and Lucien Froidevaux and Manfred Birk and Georg Wagner and Franz Schreier and Jianwen Xu and Peter Vogt and Thomas Trautmann and Motoaki Yasui},
  year={2013}
}
We observed ozone (O3) in the vertical region between 250 and 0.0005 hPa (~12-96 km) using the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on the Japanese Experiment Module (JEM) of the International Space Station (ISS) between 12 October 2009 and 21 April 2010. The new 4K superconducting heterodyne receiver technology of SMILES allowed us to obtain a one order of magnitude better signal-to-noise ratio for the O3 line observation compared to past spaceborne microwave… CONTINUE READING

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