Why is the Winter Hemisphere Hadley Circulation stronger than the Summer Hemisphere Hadley Circulation? ATS 553.

Slides:



Advertisements
Similar presentations
Chapter 10 Wind: Global Systems.
Advertisements

Global Average Barometric Pressure: January
Global Winds Eric Angat Teacher.
Somali Current TYLER JANOSKI. First, let’s talk about the South-Asian Monsoon  Monsoon develops because of temperature differences between land and sea.
General Atmospheric Circulation V Science and Society.
The General Circulation of the Atmosphere
Introduction to Oceanography
Topic: Ocean Systems Essential Question: How does energy from the Sun drive wind and ocean currents?
Visualizing Physical Geography Copyright © 2008 John Wiley and Sons Publishers Inc. Chapter 5 Winds and Global Circulation.
Recitation Geostrophic Balance Thermal Wind Effect of Friction.
Unit 4 – Atmospheric Processes. Winds… Earth’s atmospheric circulation is an important transfer mechanism for both energy and mass The imbalance between.
General Circulation and Kinetic Energy
1-Question for Debate: Think of Earth as a different planet with a single continent (more or less like an island) as indicated below. Discuss with your.
MET 61 1 MET 61 Introduction to Meteorology MET 61 Introduction to Meteorology - Lecture 10 Atmospheric Dynamics Dr. Eugene Cordero Ahrens: Chapter 9 W&H:
Air movement ENVS what makes air move ? air moves from areas of high atmospheric pressure to areas of low atmospheric pressure low pressure.
Outline Further Reading: Chapter 07 of the text book - Surface Winds on an Ideal Earth - Subtropical High-Pressure Belts - Wind and Pressure Features at.
Ocean & Atmospheric circulation redux 1) Unequal planetary heating creates pressure gradients which make winds blow on ocean surface in trade-wind & westerly.
General Circulation and Climate Zones Martin Visbeck DEES, Lamont-Doherty Earth Observatory
The Atmosphere Wind Field –Drives upper layer flows of the major gyres Net Heat & Freshwater Exchanges –Drives buoyancy flows (like the conveyor belt)
MET 61 1 MET 61 Introduction to Meteorology. MET 61 2 MET 61 Introduction to Meteorology MET 61 Introduction to Meteorology - Lecture 11 Global Circulation.
1 Weather and Climate Bay Area Earth Science Institute (BAESI) Pressure San Jose State University, January 24, 2004
Winds
Winds.   at home  
More Climatic Interactions
EARTH SCIENCE Air Pressure and Wind.
General Atmospheric Circulation
UPPER-LEVEL WINDS Atmospheric pressure, temperature and winds at surface.
How are winds created Global wind changes Seasonal wind changes
Force Balance (Chap. 6) ATM100. Topics of the Day ◦ Review Test 1 ◦ Newton’s Laws of Motion ◦ Review of vectors and forces ◦ Forces that act to move the.
Unit 2: Surface Processes and the Hydrosphere Lesson 2: Wind and the Coriolis effect ( Heath Earth Science – Pg )
GEOG 1112: Weather and Climate
Physical Science Lecture 154 Instructor: John H. Hamilton.
Winds and Currents in the Oceans
Global and Local Winds.
THE 3 CELL MODEL.
Planetary Atmospheres, the Environment and Life (ExCos2Y) Topic 6: Wind Chris Parkes Rm 455 Kelvin Building.
Introduction #2 C Global Patterns. The first two slide shows in this introduction illustrated the importance of the sun’s solar energy and how it effects.
Atmospheric Forces Nick Bassill April 8 th Why Are Forces Important? When we speak of “forces,” we’re really describing why the air in the atmosphere.
Air Movement Chapter 4 – Section 3 Pages
A2 Module 4: Global Change
Ocean Currents Ocean Density. Energy in = energy out Half of solar radiation reaches Earth The atmosphere is transparent to shortwave but absorbs longwave.
Atmospheric Motion SOEE1400: Lecture 7. Plan of lecture 1.Forces on the air 2.Pressure gradient force 3.Coriolis force 4.Geostrophic wind 5.Effects of.
Place these answers onto your paper.
Southern Oscillation- Atmospheric component of ocean's El Niño. Oscillation in the distribution of high and low pressure systems across the equatorial.
Atmospheric circulation
THE THREE CELL MODEL;-FORMATION OF THE HADLEY CELL (1)
PLANETARY WIND SYSTEM.
The Atmosphere in Motion
THE 3 CELL MODEL.
Chapter 4 © Oxford University Press, All rights reserved. 1 CHAPTER 4 ATMOSPHERIC CIRCULATION.
1 0º Equator90º Pole LP HP  At the Equator the atmosphere is heated  Air becomes less dense and rises.  Rising air creates low pressure at the equator.
Understanding Wind. Review: What is air pressure? Air pressure: the force of the weight of air on a surface – exerted in all directions.
Global air circulation Mr Askew. Pressure gradient, Coriolis force and Geostrophic flow  Wind is produced by different air pressure between places. 
Insolation and Monsoonal Circulation GEOL 3100 Earth’s Climate and Environment: Past, Present, and Future.
Paper 1 Physical Core Atmosphere and Weather 1 GeographyCambridge AS level syllabus 9696.
Coriolis Effect: Deflection of moving objects/large masses due to the rotation of Earth on its axis (EX: currents & missiles) –Northern Hemisphere: RIGHT.
• At the poles (areas which receive less solar radiation), the air is cold and descends towards the equator through the lower layers of the atmosphere.
19.2 Pressure Centers and Winds
Global Circulation and Winds (Stewart Cap. 4)
Understanding Wind.
Global Average Barometric Pressure: January
19.1 Understanding Air Pressure & Wind
PLANETARY WIND SYSTEM.
Warm air rises and cold air sinks.
Warm air rises and cold air sinks.
Wind Notes 2012.
Fundamental Force Balances
Convection in the Atmosphere: Wind
Topic: Ocean Systems Essential Question: How does energy from the Sun drive wind and ocean currents?
Presentation transcript:

Why is the Winter Hemisphere Hadley Circulation stronger than the Summer Hemisphere Hadley Circulation? ATS 553

Based on: “Role of Continents in Driving the Hadley Cells”, by Kerry H. Cook, Journal of the Atmospheric Sciences, 1 April 2003, “Role of Continents in Driving the Hadley Cells”, by Kerry H. Cook, Journal of the Atmospheric Sciences, 1 April 2003,

In Intro, you learned…

Maybe you even learned… Northern Hemisphere Summer Northern Hemisphere Summer

Maybe you even learned… Southern Hemisphere Summer Southern Hemisphere Summer

However, Ramage shows… Northern Hemisphere Summer Northern Hemisphere Summer

However, Ramage shows… Southern Hemisphere Summer Southern Hemisphere Summer

So the question is… Why is the Hadley Circulation so strong in the WINTER Hemisphere? Why is the Hadley Circulation so strong in the WINTER Hemisphere?

But a better question is… Why is the Hadley Circulation so WEAK in the SUMMER Hemisphere? Why is the Hadley Circulation so WEAK in the SUMMER Hemisphere?

Strength of the Hadley Circ. Described by the low level meridional winds Described by the low level meridional winds

But first, let’s talk about trade winds.

Summer

Maintaining trade winds

What determines friction?

Summer hemisphere has weaker trade winds, so friction is less.

What determines friction? If friction is smaller, what happens to f times v?

What determines friction? Therefore, the v component has to be smaller!

What determines friction? Therefore, the Hadley Circulation has to be smaller in the Summer Hemisphere!

Temptation: To say that it must just be the opposite in the Winter Hemisphere: To say that it must just be the opposite in the Winter Hemisphere: “In the summer hemisphere, heat lows over continents result in a weak meridional pressure gradient force, weak trade winds, and a weak Hadley Circulation.” “In the summer hemisphere, heat lows over continents result in a weak meridional pressure gradient force, weak trade winds, and a weak Hadley Circulation.”

Temptation: To say that it must just be the opposite in the Winter Hemisphere: To say that it must just be the opposite in the Winter Hemisphere: “In the summer hemisphere, heat lows over continents result in a weak meridional pressure gradient force, weak trade winds, and a weak Hadley Circulation.” “In the summer hemisphere, heat lows over continents result in a weak meridional pressure gradient force, weak trade winds, and a weak Hadley Circulation.”

Temptation: To say that it must just be the opposite in the Winter Hemisphere: To say that it must just be the opposite in the Winter Hemisphere: “In the winter hemisphere, polar highs over continents result in a strong meridional pressure gradient force, strong trade winds, and a strong Hadley Circulation.” “In the winter hemisphere, polar highs over continents result in a strong meridional pressure gradient force, strong trade winds, and a strong Hadley Circulation.”

However… That’s not how it works in the Winter Hemisphere. That’s not how it works in the Winter Hemisphere. Polar highs are VERY VERY shallow features, with almost no impact on the meridional pressure gradient force. Polar highs are VERY VERY shallow features, with almost no impact on the meridional pressure gradient force.