'Cloud size' diaporamas de présentation

ISM Lecture 10

ISM Lecture 10. The Three-Phase Interstellar Medium. 10.1 Why necessary?. Two-phase model (see Sect. 8.3) FGH model: Heating by cosmic rays => p.e. effect UV from stars: G ( T ) Cooling by [C II] fine-structure emission: L ( T )

622 views • 42 slides

Universal thermodynamics of a strongly interacting Fermi gas

Universal thermodynamics of a strongly interacting Fermi gas. Hui Hu 1,2 , Peter D. Drummond 2 , and Xia-Ji Liu 2. Physics Department, Renmin University of China ; ACQAO , Physics Department, University of Queensland. Why strongly interacting Fermi gases?.

488 views • 35 slides

Ulrich Schneider

470 views • 26 slides

Validation of CFD Calculations Against Impinging Jet Experiments

Validation of CFD Calculations Against Impinging Jet Experiments. Prankul Middha and Olav R. Hansen, GexCon, Norway Joachim Grune, ProScience, Karlsruhe, Germany Alexei Kotchourko, FZK, Karlsruhe, Germany September 11, 2007. Motivation.

372 views • 24 slides

Precipitation Intensity and Cloud Physics

Precipitation Intensity and Cloud Physics. Brad Eck April 26, 2007. Data Sources. Precipitation Intensity North American Regional Reanalysis (NARR) netCDF (thanks to Cedric) Units: kg/m^2/s ? mm/s Cloud Physics Moderate Resolution Imaging Spectrometer (MODIS) Optical Thickness.

270 views • 10 slides

Introduction

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