Date post: | 14-Dec-2015 |
Category: |
Documents |
Upload: | kerry-gallagher |
View: | 216 times |
Download: | 0 times |
Heat Flux(W·m-2 = J·s-1·m-2)
• Qs – radiation from the sun
• Qb – back radiation from Earth
• Qe – evaporative heat loss or gain
• Qh – sensible heat loss or gain
• Qv – advective heat loss or gain
Qt = Qs – Qb – Qe – Qh – Qv
James Prescott Joule, FRS
Radiation Paths
reflected
refractedabsorbedscattered
transmitted
V1
V2
Index of Refraction (η2/η1) = V1/V2
ηwater-air = 1.333 (at 20°C)
irradiance
Willebrord Snell
Solar Spectrum
d
e
hvdM
kT
hv
o
1
2)(
0
5
2
Max Planck
Stefan-Boltzmann Law
CSUN: What is the solar constant?
SUNSUNEarth
SUNSUN C
r
rT
2
24
4
4
where
If TSUN = 5775K, CSUN = ?
Distributed solar irradiance at top of atmosphere (MJ/m2/day)
Solar irradiance
The solar constant isn’t constant!
SOHO
UV images of 11 year solar cycle
Note the sunspots
Distribution of Water and Land
Solar Heating
Inflow = Outflow CSUN(1-A)πr2 = 4πr2σT4
If A=0.3 and CSUN=1367 W·m-2, what is T=?
Earth’s mean temperature balance requires an extra term
414 EARTHSUN
GHE TAC
Q
QGHE: What is the greenhouse effect?
TEarth: What is Earth’s temperature?
A: Is Earth’s albedo fixed?
How would Earth’s temperature change if the albedo changed from 30% to 29%?
4%)30(30.01
4 AEARTHSUN
GHE TC
Q
4%)29(29.01
4 AEARTHSUN
GHE TC
Q minus
)(30.029.04
4%)29(
4%)30( AEARTHAEARTH
SUN TTC
If TEARTH(A=30%) = 288K, TEARTH(A=29%) = ?
Relative Humidity (RH) and Saturation Vapor Pressure (es)
Example: RH = ?Tair = 30°; Tdew point = 10°es = 39 mb; eair = 12 mb
Evaporation from the Sea Surface
Qe = ρwaterE·LEvaporation (E) is in meters per second, and
latent heat of evaporation (L) is L= 2495 x 103 J·kg-1
Evaporation minus precipitation in millimeters per day
Seasonal Thermoclineand Mixed-Layer Depth
Earth Remote Sensing
Passive Microwave Remote Sensing
SSM/I – Special Sensor Microwave Imagermicrowave brightness temperatures at
19.35, 22.2, 37.0, and 85.5 GHz
Sea Ice Variability
Sea level from satellite altimetry
(active microwave sensing)
𝐷( 𝐽 ∙𝑘𝑔−1)≡∫𝛼 ∙𝑑𝑝
Infrared Satellite Imagery
Exitance vs. Wavelength
0
1
2
3
4
5
6
7
8
9
10
0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21
Wavelength (micrometers)
Lo
g E
xita
nce
Solar Irradiance at 1 AU
Earth Exitance at 288K
Infrared Image
Upper few millimeters of the sea surface
Sea Surface Temperature (SST)Skin Temperature and Bulk Temperature
OCN 5401
Questions?
Chapter 3