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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

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