Engineering and Design Portfolio
Weather 101 Chris Geraci. Imagine a system on a rotating sphere that is 8000 miles wide, consists of different materials, different gases that have different.
Astronomy190 - Topics in Astronomy Astronomy and Astrobiology Lecture 2 : History of Science & Astrobiology Ty Robinson.
CHAPTER 4: ATMOSPHERIC TRANSPORT Forces in the atmosphere: Gravity g Pressure-gradient Coriolis Friction to R of direction of motion (NH) or L (SH) Equilibrium.
Geophysical Modelling: Climate Modelling How advection, diffusion, choice of grids, timesteps etc are defined in state of the art models.
Energy on planet earth Sources of energy on earth? Surface 1. Solar radiation 2. Extra solar radiation (very very small) Very well understood Core.
Numerical weather prediction: current state and perspectives
As interpreted by: Jeff A. Messick Creation. Day 1.
Unstable periodic orbits in models of the low frequency atmospheric variability Andrey Gritsun Institute of Numerical Mathematics/RAS,Moscow ([email protected])
* Height (from trough to crest) * Wavelength (from crest to crest) * Period (time interval between arrival of consecutive crests at a stationary point)
© Crown copyright Met Office Climate predictions – from the coal face Richard Wood, Met Office Hadley Centre (with thanks to many colleagues)
WHAT DETERMINES THE EARTH’S GLOBAL MEAN SURFACE TEMPERATURE (GMST)?