Miriam Sinnhuber

TL;DR: In this paper, the authors provided the recommended solar forcing dataset for CMIP6 and highlighted changes with respect to CMIP5, which is the first time that a recommendation for solar-driven particle forcing has been provided for a CMIP exercise.

TL;DR: In this article, the impact of particle precipitation on the chemical composition of the atmosphere has been studied, and there are a number of observations as well as model studies concerning especially the auroral impact and large solar particle events.

TL;DR: The large solar storms in October-November 2003 caused solar proton events (SPEs) at the Earth and impacted the middle atmospheric polar cap regions, which led to the production of odd hydrogen (HO(sub x)) and odd nitrogen (NO(sub y)).

TL;DR: In this paper, the authors compared the performance of the Bremen 2-D model (B2dM) and B3dCTM, the Central Aerological Observatory (CAO) model, FinROSE, the Hamburg Model of the Neutral and Ionized Atmosphere (HAMMONIA), the KASIMA, the ECHAM5/MESSy Atmospheric Chemistry (EMAC), the modeling tool for SOlar Climate Ozone Links studies (SOCOL and SOCOLi), and the Whole Atmosphere Community Climate Model (WACCM

TL;DR: The authors calculated the changes in stratospheric ozone in response to changes in the halogen loading over the past decades, using a two-dimensional (latitude/height) model constrained by source gas mixing ratios at the surface.