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Context. Ceres is the most massive body of the asteroid belt and contains about 25 wt.% (weight percent) of water. Understanding its thermal evolution and assessing its current state are major goals o...
Satellite-based cloud top effective radius retrieved by the CERES Science Team were combined with simulated aerosol concentrations from CCCma CanAM4 to examine relationships between aerosol and cloud ...
The dust aerosol radiative forcing and heating rate over the Taklimakan Desert in Northwestern China in July 2006 are estimated using the Fu-Liou radiative transfer model along with satellite observat...
This paper describes a numerical interpretation of the April 2007, CarboEurope Regional Experiment Strategy (CERES) campaign, devoted to the study of the CO2 cycle at the regional scale. Four consecut...
Mutual perturbing effects between (1) Ceres and (2) Pallas are presented by using differences in their right ascensions and declinations. These differences are obtained as the result of two integrat...
The technique of asteroid mass determination from perturbation during close approach requires as many as possible di erent close approaches in order to derive reliable mass of a perturber. Here are ...
The impact of Asian dust on cloud radiative forcing during 2003–2006 is studied by using the Clouds and Earth's Radiant Energy Budget Scanner (CERES) data and the Fu-Liou radiative transfer model.
Pervasivemetasomatismthatinvolvedtheformationoftourmaline-richrocksandin?ux ofLi,F,andCsintoOrdovicianpsammo-peliticmetasedimentsoccurredintheValde?ores area(Ca!ceres,Spain).NumerousLi-andSn-bearing...

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