Analysis of Particle Precipitation and Development of the Atmospheric Ionization Module OSnabrück - AIMOS

• Main Author: Wissing, Jan Maik
• Other Authors: Prof. Dr. May-Britt Kallenrode, Prof. Dr. Bernd Heber, Prof. Dr. Karl-Heinz Glaßmeier
• Format: Doctoral or Postdoctoral Thesis
• Language: English
• Published: 2011
• Subjects: atmospheric ionization; ionosphere; solar energetic particles; magnetospheric particles; EISCAT; POES; GOES; AIMOS; ozone depletion; polar cap; auroral oval; 33.46 - Hochenergie-Kernphysik; 38.81 - Atmosphäre; 39.54 - Interplanetare Materie; M50 - Physics. Astronomy. Technology. Engineering. Computer science. Earth sciences; 65Z05 - Applications to physics; J.2 - PHYSICAL SCIENCES AND ENGINEERING; 94.20.Qq - Particle precipitation; 94.30.Lr - Magnetic storms; substorms; 94.10.Rk - Aurora and airglow; 94.20.Kj - Polar cap ionosphere; 94.20.Yx - Interaction between ionosphere and magnetosphere; ddc:530; ddc:550; Jackman; Randall
• Online Access: https://osnadocs.ub.uni-osnabrueck.de/bitstream/urn:nbn:de:gbv:700-201108318300/2/thesis_wissing.pdf

The goal of this thesis is to improve our knowledge on energetic particle precipitation into the Earth’s atmosphere from the thermosphere to the surface. The particles origin from the Sun or from temporarily trapped populations inside the magnetosphere. The best documented influence of solar (high-) energetic particles on the atmosphere is the Ozone depletion in high latitudes, attributed to the generation of HOx and NOx by precipitating particles (Crutzen et al., 1975; Solomon et al., 1981; Reid et al., 1991). In addition Callis et al. (1996b, 2001) and Randall et al. (2005, 2006) point out the importance of low-energetic precipitating particles of magnetospheric origin, creating NOx in the lower thermosphere, which may be transported downwards where it also contributes to Ozone depletion. The incoming particle flux is dramatically changing as a function of auroral/geomagnetical activity and in particular during solar particle events. As a result, the degree of ionization and the chemical composition of the atmosphere are substantially affected by the state of the Sun. Therefore the direct energetic or dynamical influences of ions on the upper atmosphere depend on solar variability at different time scales. Influences on chemistry have been considered so far with simplified precipitation patterns, limited energy range and restrictions to certain particle species, see e.g. Jackman et al. (2000); Sinnhuber et al. (2003b, for solar energetic protons and no spatial differentiation), and Callis et al. (1996b, 2001, for magnetospheric electrons only). A comprehensive atmospheric ionization model with spatially resolved particle precipitation including a wide energy range and all main particle species as well as a dynamic magnetosphere was missing. In the scope of this work, a 3-D precipitation model of solar and magnetospheric particles has been developed. Temporal as well as spatial ionization patterns will be discussed. Apart from that, the ionization data are used in different climate models, allowing (a) ...