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Lab 3: Earth Sun-Geometry

Lab 3: Earth Sun-Geometry

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Lab 3: Earth Sun-Geometry. Earth-Sun Geometry. Earth’s axis is tilted 23½ ° (from the perpendicular to the plane of the ecliptic) Primary cause for Earth’s seasons! Tilt is oriented in the same direction all year: North Pole points towards Polaris. Earth-Sun Geometry. Solstices : - PowerPoint PPT Presentation

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Page 1: Lab 3: Earth Sun-Geometry

Lab 3:Earth Sun-Geometry

Page 2: Lab 3: Earth Sun-Geometry

Earth-Sun Geometry

• Earth’s axis is tilted 23½° (from the perpendicular to the plane of the ecliptic)

• Primary cause for Earth’s seasons!• Tilt is oriented in the same direction all year:

• North Pole points towards Polaris

Page 3: Lab 3: Earth Sun-Geometry
Page 4: Lab 3: Earth Sun-Geometry

Earth-Sun Geometry

• Solstices:– Summer (June 21 or 22) • Northern Hemisphere is tilted 23½° toward the sun

– Sun’s rays are directly over head at 23½° N (Tropic of Cancer)

– Winter (December 21 or 22)• Northern Hemisphere is tilted 23½° away from the sun

– Sun’s rays are directly over head at 23½° S (Tropic of Capricorn)

Solar Noon = Sun at highest point in the sky

Page 5: Lab 3: Earth Sun-Geometry

Earth-Sun Geometry

http://www.geography.hunter.cuny.edu/~tbw/wc.notes/2.heating.earth.surface/01_EarthSun.html

Page 6: Lab 3: Earth Sun-Geometry

Equinoxes:– Midway between solstices

• Autumnal equinox – September 22 or 23• Vernal equinox – March 21 or 22

Page 7: Lab 3: Earth Sun-Geometry
Page 8: Lab 3: Earth Sun-Geometry

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Page 9: Lab 3: Earth Sun-Geometry
Page 10: Lab 3: Earth Sun-Geometry
Page 11: Lab 3: Earth Sun-Geometry

Sun angles vary with latitude:– High sun angles in the tropics– Medium sun angles at mid-latitude– Low sun angles in the arctic

Page 12: Lab 3: Earth Sun-Geometry

Sun Angle by Season

Page 13: Lab 3: Earth Sun-Geometry

• Solar declination: latitude at which the sun is directly above at solar noon (only between 23 ½ N-S)

• Zenith angle (ZA): the angle between a point directly overhead & the sun at solar noon

• Solar elevation angle (SA): the angle of the sun above the horizon at solar noon

Page 14: Lab 3: Earth Sun-Geometry

Finding Zenith - The 3 D’s

1. Date2. (where the sun is) Directly Overhead =3. Declination

Find the difference between the location and the declination

HINTS:•Locations in same hemisphere = SUBTRACT!•Locations in different hemispheres = ADD!• Solar Declination is 0° = SUBTRACT!

Page 15: Lab 3: Earth Sun-Geometry

Steps to Find Zenith Angle and Sun Angle

1. Find location2. Find solar declination based on date (where the sun is

directly overhead3. Find Zenith (difference between location and solar

declination)4. Find Sun Angle = 90 – Zenith

SUN ANGLE + ZENITH WILL ALWAYS = 90HINTS:

•Locations in same hemisphere = SUBTRACT!•Locations in different hemispheres = ADD!• Solar Declination is 0° = SUBTRACT!

Page 16: Lab 3: Earth Sun-Geometry

Calculating Solar Declination

• Use formula: 23.5 * sine (n)OR

• Use an Analemma!http://www.analemma.com/Pages/framesPage.html

Page 17: Lab 3: Earth Sun-Geometry
Page 18: Lab 3: Earth Sun-Geometry

Daylight Hours

• Length of daylight (in addition to solar intensity) is another principal factor that determines solar radiation receipt on earth.

• Circle of illumination – any given time half of the earth is illuminated by the sun.

• Daylight length changes daily throughout the year for every location not on the equator

• So, solar radiation exposure time, like solar intensity, is not distributed uniformly on earth. Except on the equinoxes (everywhere receives 12 hrs of days and 12 hrs of night).

Page 19: Lab 3: Earth Sun-Geometry

Yearly daylight hrs – equator; 30oN; 60oN

Page 20: Lab 3: Earth Sun-Geometry

Solar angle; azimuth; daylight hours

Page 21: Lab 3: Earth Sun-Geometry

Earth – Sun Geometry at 40oN: Solstices

•Sun has it’s longest arc…• Rises North of East• Sets North of West

Page 22: Lab 3: Earth Sun-Geometry

Earth – Sun Geometry at 40oN: Solstices

•Sun has it’s shortest arc…• Rises South of East• Sets South of West

Page 23: Lab 3: Earth Sun-Geometry

Earth – Sun Geometry at 40oN: Equinoxes

• Equinoxes:– Midway between solstices

• Autumnal equinox – September 22 or 23• Vernal equinox – March 21 or 22

•Sun arc is “normal”…• Rises in the East• Sets in the West

Page 24: Lab 3: Earth Sun-Geometry

1. 66.5 – 23.5°(SD) = 43°(ZA)

2. 90° – 43°(ZA) = 47°(SA)

SD = 23½°N

47°

1. June 21: summer solstice (23½ °N)

2. NH tilted towards the sun

Page 25: Lab 3: Earth Sun-Geometry

1. Note your latitude!2. Determine –

a. Sun at 90° b. ZA (difference between your locations)c. SA (90° – ZA)

a. Sun at 90°: 23½° Sb. ZA: 23½° + 60° = 83½°c. SA: 90° – 83½° = 6½°

**units determined by 1/sin(SA)

83½° ZA

8.834 units

The larger the unit, the cooler the temperature.WHY?

Page 26: Lab 3: Earth Sun-Geometry

0 1 2 3 4 5 6 7 8 9

0 0.00 1.75 3.49 5.23 6.98 8.72 10.45 12.19 13.92 15.64

10 17.36 19.08 20.79 22.50 24.19 25.88 27.56 29.24 30.90 32.56

20 34.20 35.84 37.46 39.07 40.67 42.26 43.84 45.40 46.95 48.48

30 50.00 51.5 52.99 54.46 55.92 57.36 58.78 60.18 61.57 62.93

40 64.28 65.61 66.91 68.20 69.47 70.71 71.93 73.14 74.31 75.47

50 76.60 77.71 78.80 79.86 80.90 81.92 82.90 83.87 84.80 85.72

60 86.60 87.46 88.29 89.10 89.88 90.63 91.36 92.05 92.72 93.36

70 93.97 94.55 95.11 95.63 96.13 96.59 97.03 97.44 97.81 98.16

80 98.48 98.77 99.03 99.25 99.45 99.62 99.76 99.86 99.94 99.98

SUN ANGLE: 36½°

Radiation Intensity