Hannover 2010 – scientific programme
Parts | Days | Selection | Search | Downloads | Help
UP: Fachverband Umweltphysik
UP 4: Remote Sensing
UP 4.7: Talk
Wednesday, March 10, 2010, 15:45–16:00, M 11
Impact of solar proton events on noctilucent clouds — •Nabiz Rahpoe1, Christian von Savigny1, Charles E. Robert1, John P. Burrows1, and M. DeLand2 — 1IEP, University of Bremen, Germany — 2Science Systems and Applications Inc. (SSAI),Maryland, USA
The impact of SPEs (Solar Proton Events) on NLCs (Noctilucent Clouds) is studied using the 23-year NLC data set based on measurements with SBUV instruments on NIMBUS 7 and the NOAA 9-17 satellites. We analyzed the GOES proton flux and NLC time series in order to find significant anti-correlations between proton fluxes and NLC occurrence rates and albedo. We focused on the analysis of the years when SPEs occurred during the core NLC season. For several cases anti-correlations of NLC and proton fluxes were found. For an increase of the proton flux of several orders of magnitude (with proton energies E > 5 MeV) during the NLC season we find a NLC reduction in NLC occurence rate or albedo of up to 50 % (relative to maximum).