The Atmospheric Response to Solar Variability: Simulations with a General Circulation and Chemistry Model for the Entire Atmosphere

• Applicant: Dr. Hauke Schmidt
• Subject Area: Atmospheric Science
• Term: from 2005 to 2012
• Project identifier: Deutsche Forschungsgemeinschaft (DFG) - Project number 5454793

• Final Report Year: 2013

Final Report Abstract

No abstract available

Publications

• Seasonal variations of semidiurnal tidal perturbations in mesopause region temperature, zonal and meridional winds above fort collins, co (40.6◦ N, 105◦ W). J. Geophys. Res., 113, 2008
  T. Yuan, H. Schmidt, C. Y. She, D. A. Krueger, and S. Reising
  
• Variation of energetic particle precipitation with local magnetic time. Adv. Space Res., 41:1274–1278, 2008
  J. M. Wissing, J. P. Bornebusch, and M.-B. Kallenrode
  
• Atmospheric Ionization Module OSnabrück (AIMOS): A 3-d model to determine atmospheric ionization by energetic charged particles from different populations. J. Geophys. Res., 114, 2009
  J. M. Wissing and M.-B. Kallenrode
  
• The effect of the solar rotational irradiance variation on the middle and upper atmosphere calculated by a three-dimensional chemistryclimate model. Atmos. Chem. Phys., 9:595–614, 2009
  A. N. Gruzdev, H. Schmidt, and G. P. Brasseur
  
• Atmospheric ionisation module Osnabrück (AIMOS) 2: Total particle inventory in the October / November 2003 event and ozone. J. Geophys. Res., 115, 2010
  J.-M. Wissing, M.-B. Kallenrode, N. Wieters, H. Winkler, and M. Sinnhuber
  
• Qbo modulation of the semiannual oscillation in MAECHAM5 and HAMMONIA. J. Geophys. Res., 115(D14), 2010
  C. Peña-Ortiz, H. Schmidt, M. A. Giorgetta, and M. Keller
  
• Solar cycle signal in a general circulation and chemistry model with internally generated quasi-biennial oscillation. J. Geophys. Res., 115(D14), 2010
  H. Schmidt, G. P. Brasseur, and M. A. Giorgetta
  
• Atmospheric Ionization Module OSnabrück (AIMOS)3: Comparison of electron density simulations by AIMOS-HAMMONIA and incoherent scatter radar measurements. J. Geophys. Res., 116, 2011
  J. M. Wissing, M.-B. Kallenrode, J. Kieser, H. Schmidt, M. Rietveld, A. Strømme, and P. Erickson
  
• Composition changes after the ” halloween“ solar proton event: the High-Energy Particle Precipitation in the atmosphere (HEPPA) model versus (MIPAS) data intercomparison study. Atmos. Chem. Phys., 11:9089–9139, 2011
  B. Funke, A. J. G. Baumgaertner, M. Calisto, T. Egorova, C. H. Jackman, J. Kieser, A. Krivolutsky, M. López-Puertas, D. R. Marsh, T. Reddmann, E. Rozanov, S.-M. Salm, M. Sinnhuber, G. Stiller, P. T. Verronen, S. Versick, T. von Clarmann, T. Y. Vyushkova, N. Wieters, and J.-M. Wissing
  
• Inter-comparison of 11-year solar cycle response in mesospheric ozone and temperature obtained by HALOE satellite data and HAMMONIA model. J. Geophys. Res., 117, 2012
  G. Beig, S. Fadnavis, H. Schmidt, and G. P. Brasseur
  
• Mechanisms involved in the amplification of the 11-yr solar cycle signal in the Tropical Pacific Ocean. Journal of Climate, 25:5102–5118, 2012
  S. Misios and H. Schmidt
  (See online at https://doi.org/10.1175/JCLI-D-11-00261.1)
• The atmospheric response to solar variability: Simulations with a general circulation and chemistry model for the entire atmosphere. In F.-J. Lübken, editor, Climate And Weather of the Sun-Earth System (CAWSES): Highlights from a priority program, pages 585–604. Springer, Dordrecht, The Netherlands, 2013
  H. Schmidt, J. Kieser, S. Misios, and A. N. Gruzdev