The constraints on dark energy tighten considerably when the cluster measurements are combined with the supernova measurements and others, including observations of the cosmic microwaves left over from the Big Bang, in which the seeds of cosmic structures like galaxy clusters can be seen, yielding a w of minus 0.991, plus or minus.045.
Within a single cluster, measurements should have related thickness and therefore low standard deviation.
We apply our method to Cluster measurements in the Earth's magnetotail.
Previously, we studied several specific features of tangential discontinuities on the basis of Cluster measurements in February April 2003.
Also we derive the conditional sample and conditional sample-complement distributions and the moments of the cluster-specific effects given the cluster measurements.
Each cluster was assigned to one of 18 predefined strata, based on predicted growing stock volume, time consumption for cluster measurements and the slope of the terrain [31].
The first-phase clusters were stratified based on predicted growing stock, time consumption for cluster measurements and slope of the terrain [6].
Although Liang and Wang in [26] presented a methodology to simulate uncertainty on RSSi and to cluster measurements, it was not exploited on localization.
High order spectral analysis is applied to Cluster measurements to assess the strength of various nonlinear processes involved in the dynamics of the turbulence.
We use the unique capability of Cluster measurements in determining gradients to examine the associated current density, Lorentz force, and current dissipation/dynamo term.
This method is applied to Cluster measurements from September 8th, 2002, where a series of Earthward propagating 1-min scale magnetic field and plasma flow variations were observed outside of the plasma sheet, which are consistent with the theoretical picture of NFTEs.
