An evaluation of COSMIC radio occultation data in the lower atmosphere over the Southern Ocean

In spite of the differences in global mean SST, major changes to the pattern and magnitude of SST biases are only seen with both high atmosphere and ocean resolution (Fig. 3): the

A high resolution climatology of precipitation and deep convection over the Mediterranean region from operational satellite microwave data: development and application to the

Our analysis of COSMIC mutations and other cancer mutations did not find an enrichment for high B-SIFT scores in COSMIC (Fig. 4A), implying that the majority of

The COSMIC RO data obtained for each day during the cyclone period are separated based on the IMD cyclone best track data, and the tropopause parameters for each individ-

The wetPrf water vapor pressure was much smaller com- pared to radiosonde in the layers above 200 hPa. Figure 3 shows the mean water vapor pressure profile of wetPrf, back- ground

Making use of the extrema bounds for the soft pomeron intercept, recently determined by fits to pp and pp ¯ data (from both accelerator and cosmic-ray experiments), we investigate

We analyze the cosmic ray arrival direction map that would be observed if the source of ultra high energy cosmic rays were the decay of dark matter particles in the halos of our

The correction, calculated from the optimally an- alyzed hydrographic data in the Southern Ocean, results in an increased ACC total baroclinic volume transport and in a shift in