Fundamentals of Atmospheric Modeling

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Formation of Martian Gullies by the Action of Liquid Water Flowing Under Current Martian Environmental Conditions (2005, background): “015, vh is the horizontal wind velocity (assumed to be 1 m/s), and rv is the total atmospheric density at the surface (zo) and at a reference height (zr) of typically 10 m [Jacobson, 1999].”
The International Urban Energy Balance Models Comparison Project: First Results from Phase 1 (2010, background): “…is poorest for those models that assume a separate tile (Vs; median RMSE 5 19 W m 2 2 , MBE 5 17 W m 2 2 ) and best for Vi models (Willmott 1981; Jacobson 1999): P i and O i 5 predicted and observed values; n 5 number of data points; e i 5 P i 2 O i ^ P i 5 a 1 bO i (where a and b are the…”
Assessing the ability of numerical ice sheet models to simulate grounding line migration (2005, background): “where D5a is the fifth-order asymmetric backward-difference approximation of the thickness slope at the grounding line (following Jacobson [1999, p. 161] ) given by”