Examples of Pressure Gradient. Pressure Gradient Force. Chapter 7: Forces and Force Balances. Forces that Affect Atmospheric Motion 2/7/2019

Similar documents
Examples of Pressure Gradient. Pressure Gradient Force. Chapter 7: Forces and Force Balances. Forces that Affect Atmospheric Motion 2/2/2015

4/29/2011. Frictional force in the boundary layer ultimately destroys extratropical cyclones.

1/18/2011. From the hydrostatic equation, it is clear that a single. pressure and height in each vertical column of the atmosphere.

The atmosphere in motion: forces and wind. AT350 Ahrens Chapter 9

The dynamics of high and low pressure systems

Atmospheric Pressure and Wind Frode Stordal, University of Oslo

True or false: The atmosphere is always in hydrostatic balance. A. True B. False

4/29/2011. Mid-latitude cyclones form along a

p = ρrt p = ρr d = T( q v ) dp dz = ρg

Lecture 5: Atmospheric General Circulation and Climate

Atmospheric pressure tells you how much atmospheric mass is above a particular altitude.

EESC V2100 The Climate System spring 2004 Lecture 4: Laws of Atmospheric Motion and Weather

Dust devils, water spouts, tornados

MIDTERM 1: APPROXIMATE GRADES TOTAL POINTS = 45 AVERAGE = 33 HIGH SCORE = = A = B = C < 20.0 NP

Mid-Latitude Cyclones and Fronts. Lecture 12 AOS 101

1/18/2011. Conservation of Momentum Conservation of Mass Conservation of Energy Scaling Analysis ESS227 Prof. Jin-Yi Yu

warmest (coldest) temperatures at summer heat dispersed upward by vertical motion Prof. Jin-Yi Yu ESS200A heated by solar radiation at the base

EART164: PLANETARY ATMOSPHERES

Balance. in the vertical too

General Atmospheric Circulation

Synoptic Meteorology I: Other Force Balances

Class exercises Chapter 3. Elementary Applications of the Basic Equations

Lecture 10 March 15, 2010, Monday. Atmospheric Pressure & Wind: Part 1

Chapter 10 Atmospheric Forces & Winds

Control Volume. Dynamics and Kinematics. Basic Conservation Laws. Lecture 1: Introduction and Review 1/24/2017

Lecture 1: Introduction and Review

Module 9 Weather Systems

Divergence, Spin, and Tilt. Convergence and Divergence. Midlatitude Cyclones. Large-Scale Setting

CONVERGENCE, DIVERGENCE, AND VORTICITY

Conservation of Mass Conservation of Energy Scaling Analysis. ESS227 Prof. Jin-Yi Yu

Wind: Global Systems Chapter 10

Weather, Air Masses, Fronts and Global Wind Patterns. Meteorology

1/3/2011. This course discusses the physical laws that govern atmosphere/ocean motions.

The Planetary Circulation System

Problem #1: The Gradient Wind in Natural Coordinates (Due Friday, Feb. 28; 20 pts total)

Fundamental Meteo Concepts

Synoptic Meteorology II: Self-Development in the IPV Framework. 5-7 May 2015

d v 2 v = d v d t i n where "in" and "rot" denote the inertial (absolute) and rotating frames. Equation of motion F =

Dynamical Meteorology 1

Introduction to Atmospheric Circulation

Winds and Global Circulation

F = ma. ATS 150 Global Climate Change Winds and Weather. Scott Denning CSU CMMAP 1. Please read Chapter 6 from Archer Textbook

Transient and Eddy. Transient/Eddy Flux. Flux Components. Lecture 3: Weather/Disturbance. Transient: deviations from time mean Time Mean

Precipitation and Wind AOSC 200 Tim Canty. Current Weather

Dynamic Meteorology 1

Circulation and Vorticity

The Transfer of Heat

Measurement of Rotation. Circulation. Example. Lecture 4: Circulation and Vorticity 1/31/2017

Meteorology Lecture 15

General Circulation. Nili Harnik DEES, Lamont-Doherty Earth Observatory

1. Sea Surface Temperatures (SSTs) > 27 and extending to some depth.

The Equations of Motion in a Rotating Coordinate System. Chapter 3

1. The vertical structure of the atmosphere. Temperature profile.

centrifugal acceleration, whose magnitude is r cos, is zero at the poles and maximum at the equator. This distribution of the centrifugal acceleration

Ocean Mixing and Climate Change

Chapter 24 Tropical Cyclones

Air Masses, Fronts, Storm Systems, and the Jet Stream

ENVIRONMENTAL MANAGEMENT I

Chapter 12 Fronts & Air Masses

1/25/2010. Circulation and vorticity are the two primary

Lecture 1. Equations of motion - Newton s second law in three dimensions. Pressure gradient + force force

NWP Equations (Adapted from UCAR/COMET Online Modules)

Atmospheric Circulation

Part-8c Circulation (Cont)

Chapter 24. Tropical Cyclones. Tropical Cyclone Classification 4/19/17

g (z) = 1 (1 + z/a) = 1

GEF 1100 Klimasystemet. Chapter 7: Balanced flow

K32: The Structure of the Earth s Atmosphere

Chapter 10: Mid-latitude Cyclones Mid-Latitude Cyclones

Chapter 10: Mid-latitude Cyclones

Quasi-Geostrophic ω-equation. 1. The atmosphere is approximately hydrostatic. 2. The atmosphere is approximately geostrophic.

Dynamics Rotating Tank

The Boundary Layer and Related Phenomena

MET 3502 Synoptic Meteorology. Lecture 8: September 16, AIRMASSES, FRONTS and FRONTAL ANALYSIS (2)

Lecture 2. Lecture 1. Forces on a rotating planet. We will describe the atmosphere and ocean in terms of their:

Chapter 1 Anatomy of a Cyclone

Using simplified vorticity equation,* by assumption 1 above: *Metr 430 handout on Circulation and Vorticity. Equations (4) and (5) on that handout

Global Wind Patterns

Lecture 14. Equations of Motion Currents With Friction Sverdrup, Stommel, and Munk Solutions Remember that Ekman's solution for wind-induced transport

Note that Rossby waves are tranverse waves, that is the particles move perpendicular to the direction of propagation. f up, down (clockwise)

Chapter 1. Introduction

Physical Oceanography, MSCI 3001 Oceanographic Processes, MSCI Dr. Katrin Meissner Ocean Dynamics.

Solution to Problems #1. I. Information Given or Otherwise Known. = 28 m/s. Heading of the ultralight aircraft!! h

Tropical Meridional Circulations: The Hadley Cell

Equatorial Superrotation on Tidally Locked Exoplanets

g (z) = 1 (1 + z/a) = 1 1 ( km/10 4 km) 2

Air Masses, Weather Systems and Hurricanes

4. Atmospheric transport. Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017

not to be republished NCERT ATMOSPHERIC CIRCULATION AND WEATHER SYSTEMS ATMOSPHERIC PRESSURE

ATMOSPHERIC CIRCULATION

Balanced Flow Geostrophic, Inertial, Gradient, and Cyclostrophic Flow

SIO 210 Introduction to Physical Oceanography Mid-term examination November 3, 2014; 1 hour 20 minutes

2. Meridional atmospheric structure; heat and water transport. Recall that the most primitive equilibrium climate model can be written

Temperature (T) degrees Celsius ( o C) arbitrary scale from 0 o C at melting point of ice to 100 o C at boiling point of water Also (Kelvin, K) = o C

Unit 2 Meteorology Test **Please do not write on this test** 5. El Nino & La Nina 6. Photosynthesis 7. Coriolis Effect 8.

1. Which weather map symbol is associated with extremely low air pressure? A) B) C) D) 2. The diagram below represents a weather instrument.

Vertical Structure of Atmosphere

Unit Three Worksheet Meteorology/Oceanography 2 WS GE U3 2

2. What are the four most common gasses in the atmosphere and their percentages?

X Y. Equator. Question 1

Transcription:

Chapter 7: Forces and Force Balances Forces that Affect Atmospheric Motion Fundamental force - Apparent force - Pressure gradient force Gravitational force Frictional force Centrifugal force Forces that Affect Atmospheric Motion Force Balance Geostrophic Balance and Jetstream Newton s second law of motion states that the rate of change of momentum (i.e., the acceleration) of an object, as measured relative to coordinates fixed in space, equals the sum of all the forces acting. For atmospheric motions of meteorological interest, the forces that are of primary concern are the pressure gradient force, the gravitational force, and friction. These are the fundamental forces. For a coordinate system rotating with the earth, Newton s second law may still be applied provided that certain apparent forces, the centrifugal force and the, are included among the forces acting. Pressure Gradient Force Examples of Pressure Gradient Hurricane Andrew, 1992 Extratropical Cyclone (from Meteorology Today) PG = (pressure difference) / distance Pressure gradient force goes from high pressure to low pressure. Closely spaced isobars on a weather map indicate steep pressure gradient. 1

Pressure Gradients Pressure Gradients The pressure gradient force initiates movement of atmospheric mass, wind, from areas of higher to areas of lower pressure Horizontal Pressure Gradients Typically only small gradients exist across large spatial scales (1mb/100km) Smaller scale weather features, such as hurricanes and tornadoes, display larger pressure gradients across small areas (1mb/6km) Vertical Pressure Gradients Average vertical pressure gradients are usually greater than extreme examples of horizontal pressure gradients as pressure always decreases with altitude (1mb/10m) Balance of Force in the Vertical: Hydrostatic Balance (from Climate System Modeling) Vertical pressure force = Gravitational force - (dp) x (da) = x (dz) x (da) x g dp = - gdz Since P= RT, dp = -P/RT x gdz dp/p = -g/rt x dz P = P s exp(-gz/rt) Gravitational Force For meteorological applications, (a: earth radius; z: height above surface) Frictional Force Frictional force (drag) is strongest near the Earth s surface and decreases rapidly with height. The atmospheric layer in which frictional force is important is call thed boundary layer, whose depth can vary from a few hundred meters to a few thousand meters. There are three sources to generate turbulence eddies to give rise to the frictional force: (1) mechanical turbulence (airs encounter surface roughness), (2) thermal turbulence (air near Earth s surface get heated, and (3) wind-shear induced turbulence. 2

Example on a Merry-Go-Around Coriolis Force Conservation of Angular Momentum U B U A (from The Earth System) Absolute angular momentum at A = Absolute angular momentum at B U A * (radius at A) = U B * (radius at B) U A * (Earth s Radius * Cos(latitude at A) = U B * (Earth s Radius * Cos(latitude at B) U A = U B * [ cos(latitude at B) / cos(latitude at A) ] U A > U B A northward motion starting at A will arrive to the east of B due to the conservation of angular momentum An apparent force (Coriolis Force) = f V, where f = 2* *Sin(lat) where =7.292x10-5 rad s -1 To the right (left) of the motion in Northern (Southern) Hemisphere Coriolis Force Coriolis Force U B U A (from The Earth System) First, Point A rotates faster than Point B (U A > U B ) U A > U B A northward motion starting at A will arrive to the east of B It looks like there is a force pushing the northward motion toward right This apparent force is called : Coriolis Force = f V where f = 2* *Sin(lat) and =7.292x10-5 rad s -1 causes the wind to deflect to the right of its intent path in the Northern Hemisphere and to the left in the Southern Hemisphere. The magnitude of depends on (1) the rotation of the Earth, (2) the speed of the moving object, and (3) its latitudinal location. The stronger the speed (such as wind speed), the stronger the. The higher the latitude, the stronger the. The Corioils force is zero at the equator. is one major factor that determine weather pattern. 3

Coriolis Force Change with latitudes How Does Coriolis Force Affect Wind Motion? (from The Atmosphere) (from Weather & Climate) Geostrophic Balance Scales of Motions in the Atmosphere H L pressure gradient force By doing scale analysis, it has been shown that largescale and synoptic-scale weather system are in geostropic balance. Geostrophic winds always follow the constant pressure lines (isobar). Therefore, we can figure out flow motion by looking at the pressure distribution. (from Meteorology Today by C. Donald Ahrens 1994 West Publishing Company) 4

Example: Winds and Height on 500mb Frictional Effect on Surface Flow H H Surface friction Surface friction L pressure gradient force L pressure gradient force Surface friction force slows down the geostrophic flow. The flow turns into (out of) the low (high) press sides. Convergence (divergence) is produced with the flow. Surface Friction Surface Geostrophic Flow Cyclonic Flow Anticyclonic Flow Friction Force = c * V c = friction coefficient V = wind speed (figures from Weather & Climate) 5

Surface High and Low Pressure Systems (from The Atmosphere) (from The Atmosphere) Super- and Sub-Geostrophic Wind Gradient Wind Balance For high pressure system gradient wind > geostrophic wind supergeostropic. The three-way balance of horizontal pressure gradient,, and the centrifugal force is call the gradient wind balance. (from Meteorology: Understanding the Atmosphere) For low pressure system gradient wind < geostrophic wind subgeostropic. The gradient wind is an excellent approximation to the actual wind observed above the Earth s surface, especially at the middle latitudes. 6

Upper Tropospheric Flow Pattern Convergence/Divergence and Vertical Motion Upper tropospheric flows are characterized by trough (low pressure; isobars dip southward) and ridge (high pressure; isobars bulge northward). The winds are in gradient wind balance at the bases of the trough and ridge and are slower and faster, respectively, than the geostrophic winds. Therefore, convergence and divergence are created at different parts of the flow patterns, which contribute to the development of the low and high systems. Convergence in the upper tropospheric flow pattern can cause descending motion in the air column. surface pressure increase (high pressure) clear sky Divergence in the upper troposphric flow pattern ca cause ascending motion in the air column. surface pressure decreases (low pressure) cloudy weather Convergence/Divergence in Jetstreak Combined Curvature and Jetstreak Effects Surface low will develop ahead of the upper-level trough. The convergence/divergence produced by the curvature and jetstreak effects cancels each other to the south of the jetstream axis but enhances each other to the north of the jetsream. The strongest divergence aloft occurs on the northeast side of the trough, where a surface low pressure tens to develop. The strongest convergence aloft occurs on the northwest side of the trough, where a surface high pressure tends to develop. However, other processes are more important that this upperlevel convergence in affecting the development of high pressure system. 7