The Effective Radiative Forcing (ERF) for the greenhouse gases (GHG) from 1750 to 2018 is fairly well known. (Assume all ERFs are exact for this problem) GHGS CO2 CH4 N20 03 halocarbons LAMBDA range Equilibrium AT range ERF 1750-2018 AT 2.15 0.54 0.19 IQ3. Calculate the LAMBDA parameter relating equilibrium temperature change AT to ERF 0.35 0.40 1.30 units W/m2 W/m2 W/m2 W/m2 W/m2 The observed 1750-2018 global mean surface temperature change AT is C C per W/m2 C
The Effective Radiative Forcing (ERF) for the greenhouse gases (GHG) from 1750 to 2018 is fairly well known. (Assume all ERFs are exact for this problem) GHGS CO2 CH4 N20 03 halocarbons LAMBDA range Equilibrium AT range ERF 1750-2018 AT 2.15 0.54 0.19 IQ3. Calculate the LAMBDA parameter relating equilibrium temperature change AT to ERF 0.35 0.40 1.30 units W/m2 W/m2 W/m2 W/m2 W/m2 The observed 1750-2018 global mean surface temperature change AT is C C per W/m2 C
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
Problem 1LR
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Transcribed Image Text:The Effective Radiative Forcing (ERF) for the greenhouse gases (GHG) from 1750 to 2018 is fairly well
known. (Assume all ERFS are exact for this problem)
ERF
GHGS
1750-2018
units
CO2
2.15
W/m2
CH4
0.54
W/m2
N20
0.19
W/m2
03
0.35
W/m2
halocarbons
0.40
W/m2
IQ3. Calculate the LAMBDA parameter relating equilibrium temperature change AT to ERF
LAMBDA
C per W/m2
range
Equilibrium AT
range
The observed 1750-2018 global mean surface temperature change AT is
ΔΤ
1.30
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