990 likes | 1.15k Views
Material Based on Chapter 5. The Planetary Boundary Layer. The Planetary Boundary Layer. Class Slide. Class Slide. Class Slide. Class Slide. Class Slide. Class Slide. Class Slide. Class Slide. Red = w ’ (t) Blue = q ’ (t). Class Slide. Class Slide. Class Slide. Class Slide.
E N D
Material Based on Chapter 5 The Planetary Boundary Layer MT 454
The Planetary Boundary Layer Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Red = w’(t) Blue = q’(t) Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide is the radiative heating rate. Note: MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Derive TKE Equation Similarly for v’ and w’
Class Slide MT 454
Class Slide • = Frictional dissipation (molecular diffusion) • > 0 TR = Redistribution by transport & pressure forces (no new TKE created) MT 454
Class Slide MT 454
Class Slide MT 454
Analogue in large-scale flow: Class Slide How does this circulation lower center of mass? MT 454
If PBL heated from below, then (z): BPL - TKE increase for unstable PBL BPL > 0 Primary energy source for unstable PBL (In stable PBL, BPL term gives energy loss) w’ < 0 ’ < 0 w’ > 0 ’ > 0 z
More precise (z) when well-mixed PBL is fully developed. Homogeneous, well-mixed layer Unstable layer maintained near surface by surface heating BPL - Side Note z
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide (See figures) MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide MT 454
Class Slide (Add friction? See Figure 5.3 in Holton.) MT 454