On the Saturation of Astrophysical Dynamos: Numerical Experiments with the No-Cosines Flow

In the context of astrophysical dynamos we illustrate that the no-cosines flow, with zero mean helicity, can drive fast dynamo action and we study the dynamo’s mode of operation during both the linear and non-linear saturation regimes. It turns out that in addition to a high growth rate in the linear regime, the dynamo saturates at a level significantly higher than normal turbulent dynamos, namely at exact equipartition when the magnetic Prandtl number Pr_m∼ 1. Visualization of the magnetic and velocity fields at saturation will help us to understand some of the aspects of the non-linear dynamo problem.     

Coastal research and policy integration in northwest Europe. The COREPOINT project

The COREPOINT (COastal REsearch and POlicy INTegration) project aimed to advance integrated coastal zone management (ICZM) in northwest Europe through a network of local authorities, research organisations and NGOs. It involved 12 partners from Ireland, the United Kingdom, France, Netherlands and Belgium. The project enabled a comparison of approaches to ICZM at the northwest Europe scale and a series of workshops was hosted to promote the principles contained in the European Union's recommendation on ICZM. At the local level, linkages were formed between research organisations and coastal management practitioners in local authorities in an attempt to bridge the science-management divide. This special edition contains several papers that deal with different facets of the project's results.     

Spectroscopic far ultraviolet observations of transition zone instabilities and their possible role in a pre-flare energy build-up

(1) Highly flare-productive new emerging active regions are characterized by numerous small low-lying loops which frequently show a chaotic pattern. (2) Flare activity in such a region subsides as the chaotic loop structures relax and expand into a bipolar configuration. (3) The transition zone in such an active region is highly unstable as shown by broadened and shifted non-thermal line profiles of medium ionized elements like Si iii, Si iv, C iv, etc. (4) These transition zone instabilities which occur as isolated events in active regions of low flare productivity are often observed prior to flares. (5) Transition zone instabilities can be traced to the footpoints of active loops, and seem to be accompanied by heating of the loop. (6) The loops vary in size and show differing degrees of activity, with the brightest and most compact ones seemingly being in a pre-flare state which results in the catastrophic energy release along the loop during a flare.     

Observations and interpretation of solar decameter type IIIb radio bursts

Solar decameter bursts of Type IIIb are observed with a multichannel radiometer at wavelengths around 12m. The time and frequency resolutions were 10 ms and 100 kHz. Observations on the time structure of these bursts are presented. A theoretical model which accounts for various aspects of these bursts is proposed.     

Spatio-temporal variations of density of the particles generating the optical emission of meteor plasma

The data of absolute spectrophotometry of meteors permit to determine number densities of particles of different elements.It is possible to solve mathematically the problem on space-time structure of the meteor with the model of a spherically symmetrical flare.The space distribution of radiating matter can be estimated by the integral equation of Abel type.Variation of density of particles in time can be found from the differential equations of kinetics.