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Le prix d’une petite pizza est la moitié du prix d’une grande pizza. Combien coûte une
Combien de moutons blancs y- a-t-il dans ce troupeau.. 23
on obtient un nouveau nombre de six chiffres, qui est le triple du nombre
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L’objectif de cette étude est de montrer si la protection des tubuli dentinaires et plus particulièrement celle du collagène qu’ils contiennent, a un impact sur le collage
On the application of the classic Kessler and Berry schemes in Large Eddy Simulation models with a particular emphasis on cloud autoconversion, the onset time of precipitation
The spatial scales of the APVC systems observed during this interval have been determined by studying the reduced- time resolution scans over all beams in use (in this case 16). All
interesting feature that the annual component dominates the variation in northern hemisphere (the maxima at December solstice and the minima around the July sol- stice) and
The question of generation mechanisms for the travelling convection vortices (TCV) signatures which are closely related to the magnetic impulsive events observed, most often, in
4 it appears that the error in the eective pointing angle arising from the aspect sensitivity of echoes observed at a nominal zenith angle of 6° is largely responsible
Phase functions have been calculated using the Monte Carlo/geometric ray tracing method for single hexagonal pyramidal ice crystals (such as solid and hollow bullets) randomly
Two of the examples (December 21, 1997; March 5, 1998) are low- to intermediate-shear cross- ings; one contains two magnetopause crossings under conditions of exceptionally high
We present a linear clustering model of cosmic infrared background (CIB) anisotropies at large scales that is used to measure the cosmic star formation rate density up to redshift
stratosphere and lower mesosphere is presented in Figure 3 for the October 2003 – April 2004 period, using both MIPAS and GOMOS data for latitudes higher than 65°N.. The daily-
The height-latitude contour plots of monthly mean zonal and meridional winds for all months of the year, and of annual mean wind, amplitudes and phases of annual and
The results obtained from the model when the neutral wind is given by HWM90 reproduce the observations that the electron density at 600 km altitude is higher in the summer
In this case we can expect variation of the energetic particle source amplitude (which is proportional to the electron density in a cloud), pitch-angle anisotropy, and
In the second, the observed aurora are interpreted as the ionospheric footprint of the region 1 current system, and the OCFLB is placed near the poleward edge of the radar
Comparing seasonal variations of k for (M +m) years with those at the stations considered by Danilov and Mikhailov (1999a), we see that the k variations during a year (or, to be
Title Page Abstract Introduction Conclusions References Tables Figures J I J I Back Close Full Screen / Esc.. Printer-friendly Version Interactive Discussion lies that were di
correlations of PC1 with the boreal winter northern Red Sea coral data (Felis et al., 2000), ice core data (Vinther et al., 2003), and some modulations in the strength of
MIPAS-E observations provide the first dataset with sufficient coverage of the polar vortex in mid-winter which enables a reason- able estimate of the timing of onset and
