MET 61 1 MET 61 Introduction to Meteorology MET 61 Introduction to Meteorology - Lecture 9 “Radiative Transfer” Dr. Eugene Cordero Stull: Chapter 2 Class.

Slides:



Advertisements
Similar presentations
Earth-Sun Relationships
Advertisements

Seasons.
Chapter 2 Where We’re Headed: Solar Energy, Seasons and the Atmosphere
Insolation.
Earth’s Motions, Solar Radiation, and the Seasons
Sun Angles  Impact the amount of Insolation  Daylight Hours Seasonal Seasonal October – March October – March Low – SunLow – Sun April – September April.
Chapter 2 Solar Energy to Earth and the Seasons Robert W. Christopherson Charlie Thomsen.
SEASONS AND THE SUN PATH
SOLAR ENERGY ► Solar energy is transmitted to earth in the form of short and long wave (SW and LW) radiation, since the sun is very hot. SW is light (visible.
Review Question In your own words, define Geography. BAD Answer: The science that studies the relationships between natural and cultural systems and the.
Solar Radiation Solar Spectrum most the energy received from the sun is electromagnetic radiation in the form of waves. Electromagnetic Spectrum is.
MET Lecture 3 Radiation Continued Dr. Craig Clements San Jose State University.
Earth Systems Science Chapter 3 I. Global Energy Balance and the Greenhouse Effect: The Physics of the Radiation Balance of the Earth 1.Electromagnetic.
MET 10 - Lecture 3 Radiation Continued Dr. Craig Clements San Jose State University.
MET 61 1 MET 61 Introduction to Meteorology MET 61 Introduction to Meteorology - Lecture 7 “Warming the Earth and Atmosphere” Dr. Eugene Cordero San Jose.
MET 61 1 MET 61 Introduction to Meteorology MET 61 Introduction to Meteorology - Lecture 8 “Radiative Transfer” Dr. Eugene Cordero San Jose State University.
PEC Solar Energy Technology (MEC-2) UET-Taxila Basics of Solar Energy Prof. Dr. A. R. El-Ghalban Department of Mechanical Engineering Prepared by University.
Outline Further Reading: Chapter 04 of the text book - global radiative energy balance - insolation and climatic regimes - composition of the atmosphere.
The Sun, Seasons and Weather
Solar Energy Part 1: Resource San Jose State University FX Rongère January 2009.
South North East West Sunrise Sunset Azimuth Angle (From South) Altitude altitude angle horizontal surface perpendicular to surface zenith angle Sun Figure.
Chapter 2 Solar Energy to Earth and the Seasons
Earth Science Golodolinski/Black 2009
Coordinate Systems.
1 MET 112 Global Climate Change MET 112 Global Climate Change - Lecture 3 Clouds and global climate Dr. Eugene Cordero San Jose State University Outline.
Announcements Clear sky patrol has not yet started We will start using PRS units this week, make sure that you have one.
Lecture 3 read Hartmann Ch.2 and A&K Ch.2 Brief review of blackbody radiation Earth’s energy balance TOA: top-of-atmosphere –Total flux in (solar or SW)=
1 MET 12 Global Climate Change - Lecture 4 Clouds and global climate Shaun Tanner San Jose State University  By the end of this chapter you should: Understand.
Earth’s Energy Balance
DAILY INSOLATION OVER THE YEAR AT VARIOUS LATITUDES (NORTH HEMISPHERE)
1 Why do we have seasons? Jeff Gawrych Met
Earth-Sun Relationships The Reasons for the Seasons.
Astronomy The Path of the Sun.
Climates, Seasons, & Days
Science 3360 Lecture 5: The Climate System
1 Lecture 29 Measuring Time on Earth Ozgur Unal. 2  What time is it in your hometown at the moment?  What time is it in NYC?
Malaria Season beginning end.
Planetary Energy Budget Current News and Weather Electromagnetic Spectrum Insolation (Short-Wave Energy) Terrestrial Radiation (Long-Wave Energy) Greenhouse.
1 MET 112 Global Climate Change MET 112 Global Climate Change - Lecture 3 The Earth’s Energy Balance Dr. Eugene Cordero San Jose State University Outline.
Earth-Sun Relationships The Reasons for the Seasons.
The earths energy balance MR ASKEW. The unequal heating of the atmosphere  Short wave radiation heats the earths surface.  The heated earth radiates.
Earth in Space EARTH, THE SUN, AND THE SEASONS. Earth, the Sun, and the Seasons  Why is Earth colder in winter than in the summer?  Not because Earth.
Earth-Sun Relationships p.p. 481 – 482 & Nearly all energy that drives our weather and climate on Earth comes from the Sun Earth only absorbs.
AstroLab-2 Locating Stars in the Sky Merav Opher-Fall 2004.
Earth-Sun Relationships The Reasons for the Seasons.
The Sun’s Path. Summer Solstice (approximately June 20-21) North Pole: The North Pole (90 degrees north latitude) receives 24 hours of daylight, as it.
Lab 3: Earth Sun-Geometry
Chapter 2 Solar Energy, Seasons and the Atmosphere
Natural Environments: The Atmosphere
The Earth as a Rotating Planet
Solar Energy to Earth and the Seasons
The electromagnetic spectrum
Planetary Energy Budget
Lesson 3: Seasons on earth notes
Objectives 2f and 4c 2f = 3/3 = 100% 4c = 11/11 = 100%
DO NOW Turn in Review #13. Pick up notes and Review #14.
LINES OF LATITUDE AND LONGITUDE
Climates, Seasons, & Days
Climates, Seasons, & Days
Chapter 4A: SOLAR RADIATION- GEOMETRY
World Geography Climates
L.O: SWBAT explain why the angle of insolation (angle of sunlight) gives Earth its climates and seasons.
AOSC Lesson 4.
APPARENT PATH OF THE SUN
Seasons.
Solar Energy to Earth and Seasons
Thermodynamics Atmosphere
Chapter 4A: SOLAR RADIATION- GEOMETRY
Presentation transcript:

MET 61 1 MET 61 Introduction to Meteorology MET 61 Introduction to Meteorology - Lecture 9 “Radiative Transfer” Dr. Eugene Cordero Stull: Chapter 2 Class Outline: Solar elevation and azimuth Surface radiation budget

MET 61 2 MET 61 Introduction to Meteorology Activity question Question 3: Calculate the radiative equilibrium temperature of the Earth’s surface and Earth’s atmosphere assuming that the earth’s atmosphere can be regarded as a thin layer with an absorptivity of 0.1 for solar radiation and 0.8 for terrestrial radiation. Assume the earth’s surface radiates as a blackbody at all wavelengths.

MET 61 3 MET 61 Introduction to Meteorology

MET 61 4 MET 61 Introduction to Meteorology

MET 61 5 MET 61 Introduction to Meteorology Nomenclature Earth’s tilt relative to orbital plane:  r =23.5° Solar declination angle (angle between ecliptic and equator):  s Julian day: d (day number ) Local elevation angle:  (sun angle relative to horizon) Solar zenith angle:  (sun angle relative to the vertical) Azimuth angle (sun angle relative to north)

MET 61 6 MET 61 Introduction to Meteorology Solar declination angle The solar declination angle is a function of the day of the year. C=2  (360°); d r =173 (summer solstice); d y =365 (or 366 if leap year)

MET 61 7 MET 61 Introduction to Meteorology Solar declination angle The solar declination angle is a function of the day of the year. C=2  (360°); d r =173 (summer solstice); d y =365 (or 366 if leap year)

MET 61 8 MET 61 Introduction to Meteorology Local Elevation Angle The local elevation angle is a function of the day the year and local time (ranges from 0-90°)  =latitude;  s =solar declination; C=2  (or 360); t d =length of day; t UTC =time of day in universal time; e =longitude (positive west of Greenwich meridian;

MET 61 9 MET 61 Introduction to Meteorology Local Elevation Angle The local elevation angle is a function of the day the year and local time (ranges from 0-90°)  =latitude;  s =solar declination; C=2  (or 360); t d =length of day; t UTC =time of day in universal time; e =longitude (positive west of Greenwich meridian;

MET MET 61 Introduction to Meteorology Local Azimuth Angle The local azimuth angle is a function of the day of the year and local time. (ranges from 0°-360 °)  =latitude;  s =solar declination;  =C/4-  (  =C-  if afternoon); C= 2  (or 360)

MET MET 61 Introduction to Meteorology Local Azimuth Angle The local azimuth angle is a function of the day of the year and local time. (ranges from 0°-360 °)  =latitude;  s =solar declination;  =C/4-  (  =C-  if afternoon); C= 2  (or 360)

MET MET 61 Introduction to Meteorology Surface Radiation Budget The net radiative flux perpendicular to the earth’s surface is

MET MET 61 Introduction to Meteorology Surface Radiation Budget The net radiative flux perpendicular to the earth’s surface is

MET MET 61 Introduction to Meteorology Surface Radiation Budget (II) The longwave IR is

MET MET 61 Introduction to Meteorology Surface Radiation Budget (II) The longwave IR is

MET MET 61 Introduction to Meteorology

Simplified radiative energy cascade for the Earth-atmosphere climate system Energy Input Energy Output E-A Climate System Extraterrestrial Short Wave Radiation Reflected Extraterrestrial Short Wave Radiation Terrestrial Long Wave Radiation Planetary Albedo Solar Temperature Planetary Temperature

MET MET 61 Introduction to Meteorology Activity 8 (Due April 4 th ) Question 1: Determine the local elevation and azimuth angle at SJSU for March 25 th, 2007 at noon local time. Verify this visually if possible! Question 2: Estimate the net radiation at the surface of SJSU (assume some albedo and justify) at the above time assuming two conditions: –A) Low clouds are present with a 50% coverage –B) No clouds are present. Question 3: Plot out the solar elevation angle versus the local time for Jan 20 th, March 20 th and June 20 th over San Jose. Explain your results. Question 4: Plot out the local elevation angle at SJSU at noon for an entire year. Explain your results.

MET MET 61 Introduction to Meteorology Quiz 1 Tuesday, Feb 24: ~ 30 minutes Part I: Multiple Choice/Short Answers –From Ahrens reading; general concepts –Closed book (notes) Part II: Problems –Like activities –Open book (notes)

MET MET 61 Introduction to Meteorology Review questions On June 21 st, at what latitude is the sun directly overhead at noon? On September 22 nd, at what latitude is the sun directly overhead at noon? How many hours of daylight are present at the South Pole on February 20 th ? Where would you expect to have longer days; 45 ° N on June 21 st or 50°S on Dec 21 st ?