RMPh 2014, Теория — Задача 2. Theoretical Problem no. 2 (10 points) — Terrestrial climate modeling

Romanian Master of Physics 2014 · 10 т.

Условие

Climate change and global warming, the life of humans in new climatic conditions becomes topics of public interest in recent decades.

On a cosmic scale, the only phenomena occurring in Earth's energy balance are absorption and emission of radiation. One can say that the earth's climate condition depends on delicate balance between the energy that our planet receives for the formidable energy source that is the sun and the energy that Earth radiates into space. Consider that solar constant for the radiation coming from the Sun towards the Earth is wS=1370 W⋅m−2w_S = 1370\ \mathrm{W}\cdot\mathrm{m}^{-2}.

A body that absorbs electromagnetic radiation reaching the surface, regardless of the wavelength of the radiation and emits electromagnetic radiation according to the temperature of its surface is called a blackbody. A black body emits energy with a specific spectral distribution, depending on its own temperature. Solid smooth lines, in the graph in Figure 1 show the spectral distribution of the emission energy of the Sun, equivalent to a black body.

Spectral irradiance of sunlight (W/m²/nm, 0 to 2.5) against wavelength (250 to 2500 nm), with Romanian labels: UV, Vizibil and Infraroşu bands; the yellow area is sunlight at the top of the atmosphere (Lumina Soarelui la limita de sus a atmosferei), the red area sunlight at sea level (Lumina Soarelui la nivelul mării), the grey curve the black-body spectrum at 5250 °C (Spectrul Corpului negru la 5250°C); absorption bands (benzi de absorbţie) are marked O3, O2, H2O and CO2.
Figure 1 (not for calculations purposes)

If ε(T)\varepsilon(T) represents the total energy (in the whole spectrum) emitted by unit area of a black body in unit time, and TT is the absolute temperature of the black body, then the Stefan - Boltzmann states that ε(T)=σ⋅T4\varepsilon(T) = \sigma\cdot T^4. In the expression σ=5,67⋅10−8 W⋅m−2⋅K−4\sigma = 5{,}67\cdot 10^{-8}\ \mathrm{W}\cdot\mathrm{m}^{-2}\cdot\mathrm{K}^{-4} is Stefan – Boltzmann constant.

Problem proposes you to use different modeling in different workloads and to determine the average temperature the Earth would have at the surface for each of the models used. Express the answers as function of symbols of quantities or numerical values marked in blue color in the problem statement. Express obtained numerical results in the form of integers.

Task no. 1 (1 т.)

In the task no. 1 uses simple modeling. Suppose that the energy is taken from the Sun and that the Earth loses energy as a black body.

1.a. Determine the expression of average temperature TPT_P that the Earth's surface should have , in accordance with simple modeling used. (0,70p) [0,7 т.]

1.b. Calculate the numerical value TPT_P of the average temperature that the Earth's surface should have, according to this model. (0,30p) [0,3 т.]

Task no. 2 (1 т.)

Simple modeling of the task no. 1 one assumes that the Earth is a black body. Assumption is unrealistic, because all images taken from space show the Earth as a luminous body.

Earth's atmosphere (especially clouds) reflects approximately 24% of the energy coming from the Sun and the Earth's surface (especially ice areas) still reflects 6% of the incident energy. Feature called albedo measures the ratio of reflected radiant flux and incident radiant flux. Considers that terrestrial albedo is A=30%A = 30\%.

2.a. Determine the expression of average temperature TP′T_P' that the Earth's surface should have, in accordance with simple modeling used in these workload. (0,70p) [0,7 т.]

2.b. Calculate the numerical value TP′T_P' of the average temperature that the Earth's surface should have, according to the model in workload 2a. (0,30p) [0,3 т.]

Task no. 3 (4 т.)

While the Sun emits energy mostly in the visible, relatively low temperature of the Earth's land surface causes its emission to be localized in the infrared spectrum. A careful modeling of climate takes account of the atmosphere. The atmospheric gas is a mixture having specific absorbent properties. The Spectrum illustrated in Figure 1 shows that the different atmospheric gases absorb radiation in different spectral domains. Characterization of the spectral absorption can be achieved by introduction of transmission coefficients in the visible αvis\alpha_{vis} and infrared αir\alpha_{ir}, respectively, representing the ratio of the energy passing through the air (in the visible or infrared), and the energy that enters the atmosphere. If radiation in a specified spectral range is completely absorbed, then the corresponding transmission coefficient is zero, and if radiation is not absorbed at all, then the transmission coefficient is one.

Task no. 3 proposes to determine the Earth's temperature TP′′T_P'' using a modeling that takes into account the partial reflection of light coming from the sun (albedo AA) and absorptive properties of the atmosphere (transmission coefficients αvis\alpha_{vis} and αir\alpha_{ir}).

3.a. Determine the expression of average temperature TP′′T_P'' that the Earth's surface should have, in accordance with modeling used in these workload. (2,50p) [2,5 т.]

3.b. Calculate the numerical value TP′′T_P'' of the average temperature that the Earth's surface should have when A=0,3A = 0{,}3, αvis=0,8\alpha_{vis} = 0{,}8 and αir=0,1\alpha_{ir} = 0{,}1. (0,30p) [0,3 т.]

3.c. Using modeling proposed in this workload, calculate the average temperature on the Earth surface, where albedo and transmission coefficients have the values given in Table 1 (1,20p)

Table 1

CaseIIIIIIIV
αvis\alpha_{vis}1111
αir\alpha_{ir}1100
AA0,30,00,00,3
TP′′ (K)T''_P\,(K)
tP′′ (∘C)t''_P\,(^{\circ}C)

[1,2 т.]

Task no. 4 (1 т.)

Use modeling proposed in the task no. 3 and assume that the distance between Earth and the Sun would rise by f=1%f = 1\%.

4.a. Determine the expression of average temperature TP′′′T_P''' that the Earth's surface should have, if A=0,3A = 0{,}3, αir=0,3\alpha_{ir} = 0{,}3 and αvis=0,6\alpha_{vis} = 0{,}6. (1,00p) [1 т.]

Task no. 5 (3 т.)

Assume that some of the sand found in the Sahara desert would be "transformed" into a "mirror glass".

5.a. Using the modeling proposed in task no. 3 estimates the surface that "mirror glass" should have so that the average temperature at the Earth's surface to fall 1∘C1^{\circ}C against the value determined in the task 3.b. Consider that the radius of the Earth is RP=6400 kmR_P = 6400\ \mathrm{km}. (3,00p) [3 т.]

© Topic proposed by:

Prof. Dr. Delia DAVIDESCU

Conf. Univ. Dr. Adrian DAFINEI

Отговори

Решение


Оригинал в Архива: th_problems.pdf · официални решения: th_solutions.pdf