Earth is tilted (oblique) on its Axis!

Similar documents
Seasonal & Diurnal Temp Variations. Earth-Sun Distance. Eccentricity 2/2/2010. ATS351 Lecture 3

HEATING THE ATMOSPHERE

L.O: THE ANGLE OF INSOLATION ANGLE INSOLATION: THE ANGLE SUNLIGHT HITS THE EARTH

Meteorology Pretest on Chapter 2

Lecture 3: Global Energy Cycle

Page 1. Name:

ATMOSPHERIC ENERGY and GLOBAL TEMPERATURES. Physical Geography (Geog. 300) Prof. Hugh Howard American River College

Chapter 2 Solar and Infrared Radiation

Lecture #03. January 20, 2010, Wednesday

Why the Earth has seasons. Why the Earth has seasons 1/20/11

Fluid Circulation Review. Vocabulary. - Dark colored surfaces absorb more energy.

SEASONAL AND DAILY TEMPERATURES

1 What Is Climate? TAKE A LOOK 2. Explain Why do areas near the equator tend to have high temperatures?

Energy: Warming the earth and Atmosphere. air temperature. Overview of the Earth s Atmosphere 9/10/2012. Composition. Chapter 3.

Lecture 2: Global Energy Cycle

Topic 6: Insolation and the Seasons

NATS 101 Section 13: Lecture 7. The Seasons

Topic # 11 HOW CLIMATE WORKS continued (Part II) pp in Class Notes

5) The amount of heat needed to raise the temperature of 1 gram of a substance by 1 C is called: Page Ref: 69

Insolation and Temperature variation. The Sun & Insolation. The Sun (cont.) The Sun

(1) Over the course of a day, the sun angle at any particular place varies. Why?

Warming Earth and its Atmosphere The Diurnal and Seasonal Cycles

1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely

Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate

Seasons, Global Wind and Climate Study Guide

Seasonal & Daily Temperatures

Energy and Seasons A B1. 9. Which graph best represents the general relationship between latitude and average surface temperature?

Practice Questions: Seasons #1

Chapter 2. Heating Earth's Surface & Atmosphere

(1) How does the annual average sun angle at solar noon (that is, the sun angle at noon averaged over a full year) depend on latitude?

1 What Is Climate? TAKE A LOOK 2. Explain Why do areas near the equator tend to have high temperatures?

Numerical Example An air parcel with mass of 1 kg rises adiabatically from sea level to an altitude of 3 km. What is its temperature change?

November 20, NOTES ES Rotation, Rev, Tilt.notebook. vertically. night. night. counterclockwise. counterclockwise. East. Foucault.

Topic # 12 How Climate Works

9/1/14. Chapter 2: Heating Earth s Surface and Atmosphere. The Atmosphere: An Introduction to Meteorology, 12 th. Lutgens Tarbuck

- global radiative energy balance

The Earth is a Rotating Sphere

Lecture 2: Global Energy Cycle

Solar Flux and Flux Density. Lecture 2: Global Energy Cycle. Solar Energy Incident On the Earth. Solar Flux Density Reaching Earth

Prentice Hall EARTH SCIENCE

Earth s Heat Budget. What causes the seasons? Seasons

Observation: predictable patterns of ecosystem distribution across Earth. Observation: predictable patterns of ecosystem distribution across Earth 1.

C) wavelength C) eastern horizon B) the angle of insolation is high B) increases, only D) thermosphere D) receive low-angle insolation

The inputs and outputs of energy within the earth-atmosphere system that determines the net energy available for surface processes is the Energy

Lecture 4 Air Temperature. Measuring Temperature. Measuring Temperature. Surface & Air Temperature. Environmental Contrasts 3/27/2012

The following terms are some of the vocabulary that students should be familiar with in order to fully master this lesson.

Chapter 4: Weather & Climate. (Pg )

3. Which color of the visible light has the shortest wavelength? A) violet B) green C) yellow D) red

In the News: &id= &m=

SUBJECT : GEOGRAPHY ROTATION AND REVOLUTION This paper consists of 5 printed pages.

Data and formulas at the end. Exam would be Weds. May 8, 2008

Chapter 3. Multiple Choice Questions

The Earth-Moon-Sun System

ATMOSPHERE PACKET CHAPTER 22 PAGES Section 1 page 546

Aim: What causes Seasons?

4-1 The Role of Climate

Temperature Variation on Earth. Goal: Explain our atmosphere s interaction with the Sun s radiation

4-1 The Role of Climate

Prentice Hall EARTH SCIENCE. Tarbuck Lutgens

What is Climate? Understanding and predicting climatic changes are the basic goals of climatology.

Lecture Outlines PowerPoint. Chapter 16 Earth Science 11e Tarbuck/Lutgens

Topic # 12 Natural Climate Processes

Which graph best shows the relationship between intensity of insolation and position on the Earth's surface? A) B) C) D)

Directed Reading. Section: Solar Energy and the Atmosphere RADIATION. identical point on the next wave. waves

Laboratory Exercise #7 - Introduction to Atmospheric Science: The Seasons and Daily Weather

A Living Planet. The Earth Inside and Out

Next quiz: this Friday, questions. Plus more on Wednesday.

Lecture 11: Meridonal structure of the atmosphere

The Atmosphere. Importance of our. 4 Layers of the Atmosphere. Introduction to atmosphere, weather, and climate. What makes up the atmosphere?

Climate System. Sophie Zechmeister-Boltenstern

2/22/ Atmospheric Characteristics

C) the seasonal changes in constellations viewed in the night sky D) The duration of insolation will increase and the temperature will increase.

ARCH 1250 APPLIED ENVIRONMENTAL STUDIES. CLASS TWO - CLIMATE Macroclimate and Microclimate

Topic # 12 HOW CLIMATE WORKS

CHAPTER 6 Air-Sea Interaction Pearson Education, Inc.

Which Earth latitude receives the greatest intensity of insolation when Earth is at the position shown in the diagram? A) 0 B) 23 N C) 55 N D) 90 N

Chapter 3: Temperature

1 A 3 C 2 B 4 D. 5. During which month does the minimum duration of insolation occur in New York State? 1 February 3 September 2 July 4 December

Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun

Chapter 11 Lecture Outline. Heating the Atmosphere

4-1 The Role of Climate. Copyright Pearson Prentice Hall

Chapter Introduction. Earth. Change. Chapter Wrap-Up

5. In which diagram is the observer experiencing the greatest intensity of insolation? A) B)

Exploring more with seasons Name: Block

Planet Earth. Part 2

Earth s Heat Budget. What causes the seasons? Seasons

CHAPTER 3. The sun and the seasons. Locating the position of the sun

Exercise 6. Solar Panel Orientation EXERCISE OBJECTIVE DISCUSSION OUTLINE. Introduction to the importance of solar panel orientation DISCUSSION

Lesson Overview. Climate. Lesson Overview. 4.1 Climate

AT350 EXAM #1 September 23, 2003

Reasons for the seasons - Rebecca Kaplan

Natural Causes of Climate. 3B Day 2

Laboratory Exercise #7 - Introduction to Atmospheric Science: The Seasons

Sunlight and its Properties Part I. EE 446/646 Y. Baghzouz

Meteorology Practice Test

LAB: What Events Mark the Beginning of Each Season?

GEOGRAPHY EYA NOTES. Weather. atmosphere. Weather and climate

S CIENCE O VERVIEW. 59 Lesson Plan. Standards Benchmarks. Science Overview. Lesson Overview. Answer Key. Resources. My Angle on Cooling ME S S EN G ER

Daily Motions. Daily Motions. Solar and Sidereal Days. Annual Motions of the Sun. Coordinate system on Earth. Annual Motion of the Stars.

Energy Balance and Temperature. Ch. 3: Energy Balance. Ch. 3: Temperature. Controls of Temperature

Transcription:

MONDAY AM Radiation, Atmospheric Greenhouse Effect Earth's orbit around the Sun is slightly elliptical (not circular) Seasons & Days Why do we have seasons? Why aren't seasonal temperatures highest at the summer solstice (June 21)? Why aren't daily temperatures highest at Noon? Earth is somewhat closer to Sun in January than in July... 1 Earth is tilted (oblique) on its Axis! June 21 23.5 Arctic Midnight Sun Is this why we have seasons? 2 Earth's orbitdistance aroundtothe Seasonally varying SunSun has only minor effect on seasonal temperatures; instead it is the tilt of earth's axis combined with earth's orbit around the sun that leads to seasons! 12 hours of daylight for everybody 23.5 Antarctic Polar Night 3 4

Sun's rays that strike a surface at an angle are less intense per unit area than those from directly above Seasons Seasons are regulated by the amount of solar energy received at Earth's surface The solar energy received at the top of the atmosphere depends on: angle at which sunlight locally strikes Earth's surface hours of daylight Seasons are NOT due to elliptical nature of earth's orbit around the sun! 5 Smaller angle of incoming solar radiation means the same amount of energy is spread over a larger area High Sun (summer) = more heating Low Sun (winter) = less heating 6 Midnight Sun NH summer June 21 Equinox March 20 Sep 22 NH winter Dec 21 7 The region north of the arctic circle experiences 24 hours of sunlight in summer (Earth's surface does not rotate out of solar exposure). 8

Sea-Level Temperatures Controls of Temperature January Tropics are warmer than polar regions, but land and water, ocean currents, and elevation create additional variations. Air temperature as you move around the globe varies regionally as a function of: Latitude Land and Water Distribution Ocean Currents (e.g. gulf stream) Elevation Mountain Ranges (e.g. Rockies) July 9 Southern hemisphere has fewer land masses and an ocean current that encircles the globe, creating more regular temperatures than in the northern hemisphere. Land versus Water / Ocean Land versus Water / Ocean: Seasonal Cycles Water has a very large heat capacity (4 times as large as land): to heat one kilogram of water by one degree Kelvin/Celcius an energy of 1000 calories is required (4186 Joules) Therefore, oceans (and large lakes) are able to store a large amount of heat, changing their temperature is much more difficult than land 10 Some heating of oceans goes into evaporation Water is a fluid, so heat in the oceans is mixed efficiently; Land primarily moves heat by conduction Large heat capacity of oceans make them much more resistant to changes in heat input than land Hence, annual temperature range is much smaller over oceans than land Sunlight can penetrate into the ocean 11 12

Regional Seasonal Cycles Daily (Diurnal) Temperature Variations Regional differences in the seasonal cycle of temperature are influenced by geography, such as latitude, altitude, and nearby water and ocean currents, as well as heat generated in urban areas San Francisco, CA is downwind of the Pacific Ocean Sun rays are most intense around noon As is the case with seasons, the maximum temperatures lag the peak incoming solar radiation Heat transfer mechanisms (heating & cooling) in the atmosphere are at the heart of understanding the diurnal cycle: Richmond, VA is downwind of North America! 13 Local Solar Changes Radiation Convection Conduction 14 Local Solar Changes by Latitude Northern hemisphere sunrises are in the southeast during winter, but in the northeast during summer Summer noon time sun is also higher above the horizon than the winter sun 15 Each day is like a mini seasonal cycle: 16

Temperature Lags Radiation The Earth's surface temperature is a balance between incoming solar radiation and outgoing terrestrial (longwave) radiation Peak temperature lags after peak insolation because surface continues to warm until infrared radiation exceeds What Controls Daily High Temperatures? Daily T max depends on: Radiation (e.g. Cloud Cover) Surface Type Absorption Characteristics (strong absorbers enhance instantaneous surface heating) Vegetation / Moisture (available energy partially used to evaporate water) Wind Strong wind generates mixing of heated air near the ground to higher altitudes insolation 17 18 Clouds reflect solar (shortwave) radiation but absorb and re-emit terrestrial (longwave/infrared) radiation 19