Response of Cloud Condensation Nuclei (> 50 nm) to changes in ion-nucleation
arXiv:1202.5156 · doi:10.1016/j.physleta.2013.07.004
Abstract
In experiments where ultraviolet light produces aerosols from trace amounts of ozone, sulphur dioxide, and water vapour, the number of additional small particles produced by ionization by gamma sources all grow up to diameters larger than 50 nm, appropriate for cloud condensation nuclei. This result contradicts both ion-free control experiments and also theoretical models that predict a decline in the response of larger particles due to an insufficiency of condensable gases (which leads to slower growth) and to larger losses by coagulation between the particles. This unpredicted experimental finding points to a process not included in current theoretical models, possibly an ion-induced formation of sulphuric acid in small clusters.
4 pages, 3 figures
References in corpus (1)
Cited by in corpus (6)
- Discussion on climate oscillations: CMIP5 general circulation models versus a semi empirical harmonic model based on astronomical cycles
- How much has the Sun influenced Northern Hemisphere temperature trends? An ongoing debate
- Dust in brown dwarfs and extra-solar planets. VIII. TiO seed formation: 3D Monte Carlo versus kinetic approach
- Approximate analytical solutions to the condensation-coagulation equation of aerosols
- The Ion and Charged Aerosol Growth Enhancement (ION-CAGE) code: A numerical model for the growth of charged and neutral aerosols
- Evidence of two different types of short term solar modulation of regional surface temperature and cloud