CASES-99: a comprehensive investigation of the stable nocturnal boundary layer

Government policy varies between nations and this guidance sets out the need for balanced decision-making about ways of working, and the ongoing safety considerations

Astrometric and photometric star cata- logues derived from the ESA HIPPARCOS Space Astrometry Mission.

Then, it is applied to the investigation of waves and instabilities in several layers and structures of the solar atmosphere, such as the fully ionized solar corona and solar wind,

In addition to traffic and noise exposure data, the calculation method requires the following inputs: noise costs per day per person exposed to road traffic

In the previous sections we have shown how astronomical alignments and solar hierophanies – with a common interest in the solstices − were substantiated in the

The objective of this study was to describe the relationships between mean daytime and nighttime ambulatory BP, BP variability, and nocturnal decline in BP with subjects

Because of the physical and topological similarity of events in the selected and fiducial phase spaces, new physics contributions are expected to affect both in approximately the

Now the numerical solution is possible today if suitable models are used to solve the equations and simulate the turbulence eect and boundary layer.... 8.5.- Parabolic models of