Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

Give examples of radiative heat transfer processes dominated by surface- tosurface transfer and of processes for which the effects of absorption and emission in the space between surfaces (participating medium) are essential.

Short Answer

Expert verified
Question: Identify and describe examples of two types of radiative heat transfer processes: one dominated by surface-to-surface transfer and another where absorption and emission in the space between surfaces play a significant role. Answer: An example of surface-to-surface radiative heat transfer is heat transfer between two parallel plates with a vacuum between them, such as in a vacuum thermos. In this case, heat transfer is solely due to the exchange of radiation between the surfaces of the plates. On the other hand, an example where absorption and emission between surfaces play a crucial role is the Earth's atmosphere. Here, the participating medium consists of various gases, water vapor, and aerosols. The atmosphere absorbs and emits solar radiation and longwave radiation originating from the Earth's surface, which is essential in understanding the greenhouse effect.

Step by step solution

01

Example of Surface-to-Surface Transfer

An example of surface-to-surface radiative heat transfer would be heat transfer between two parallel plates with a vacuum between them. In this case, the particles in the vacuum do not participate in the heat transfer process, and the heat transfer is solely due to the exchange of radiation between the surfaces of the plates. This type of heat transfer is typically seen in a vacuum thermos, where the space between the double walls is evacuated to minimize heat transfer by conduction and convection. The shiny inner surfaces of the thermos also minimize the heat transfer by reflecting the radiations.
02

Example of Participating Medium Transfer

An example of radiative heat transfer where absorption and emission in the space between surfaces play a significant role is in the Earth's atmosphere. In this case, the participating medium consists of various gases, water vapor, and aerosols. The incoming solar radiation is partly absorbed and partly scattered by the atmosphere. The atmosphere also absorbs and emits longwave radiation that originates from the Earth's surface. This participating medium heat transfer is essential in understanding the greenhouse effect, where certain gases (like carbon dioxide and water vapor) absorb outgoing longwave radiation, causing the Earth's atmosphere to warm up.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Surface-to-Surface Transfer
Surface-to-Surface radiative heat transfer refers to the process where thermal energy is exchanged between two surfaces without any medium in between affecting the transfer. A perfect example of this is the heat transfer between two parallel plates in a vacuum. In a vacuum, there's neither air nor any particles to absorb, scatter, or emit the radiant energy. This lack of interaction means the heat is transferred directly between the surfaces via radiation.
This concept is commonly seen in items like vacuum thermoses. Here, the space between the walls of the thermos is evacuated, meaning there is no air that could mediate heat through conduction or convection. This ensures that heat transfer only takes place due to radiation. Additionally, the shiny surfaces inside the thermos help reflect thermal radiation, minimizing energy loss even further.
Understanding surface-to-surface transfer helps in designing systems where heat retention or isolation is crucial, such as in thermal insulators used in spacecraft.
Participating Medium
Participating medium describes a situation in radiative heat transfer where the medium between surfaces plays an active role, mainly through absorption, emission, and scattering of radiation. The Earth's atmosphere serves as a quintessential example. Here, gases, water vapor, and aerosols act as the participating medium.
When solar radiation enters the Earth's atmosphere, a portion is absorbed or scattered. Conversely, the Earth's surface emits longwave radiation, which again interacts with atmospheric components. This entire interaction affects how energy is distributed and is key to phenomena such as the greenhouse effect.
Key characteristics of a participating medium include:
  • Absorption: The medium absorbs radiant energy, gaining energy itself and altering the intensity of the radiation.
  • Emission: The medium can emit radiation, affecting energy transfer patterns.
  • Scattering: The redirection of radiation by particles in the medium.
Understanding these interactions is crucial for fields ranging from climate science to engineering applications, where predicting heat transfer is foundational.
Greenhouse Effect
The greenhouse effect is a natural process where certain gases in the Earth's atmosphere trap heat, leading to a warming effect. The process begins when solar radiation reaches the Earth. Some of this energy is absorbed by the Earth's surface, warming it, while the rest is reflected back towards space.
Earth's surface then emits heat in the form of longwave infrared radiation. Here is where the participating medium comes into play. Gases like carbon dioxide, methane, and water vapor absorb this outgoing radiation and re-emit it in all directions, including back towards the surface of the Earth. This trapped heat increases the Earth's temperature, creating the greenhouse effect.
This phenomenon is essential for maintaining the Earth's temperature conducive to life. However, human activities have increased concentrations of greenhouse gases, enhancing this effect and contributing to global warming. Key aspects include:
  • Natural vs. Enhanced: While the natural greenhouse effect is vital, the enhanced effect due to excess greenhouse gases is causing climate change.
  • Key Gases: Common greenhouse gases include CO2, CH4, and H2O.
Understanding the greenhouse effect is critical for addressing environmental challenges and developing sustainable solutions.

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Equation (4.8) is valid when the heat conductivity is independent on the direction. How would a generalization look like for the case of heat conductivity being different in the three coordinate directions? Which physical properties, e.g., of biomass material, could cause such difference?

What is the \(d^{2}\)-law for droplet evaporation? What are the assumptions that have to be satisfied for this law to be valid?

There is currently substantial interest in utilizing eukaryotic algae for the renewable production of several bioenergy carriers, including starches for alcohols, lipids for diesel fuel surrogates, and hydrogen for fuel cells. Algae can convert solar energy into fuels at high photosynthetic efficiencies and can thrive in saltwater systems. Part of an energy balance analysis of such a process is the computation of the penetration of the radiative heat flux in a pool of water. a. Considering the surface of the sun as a black surface at a temperature of 5777 \(\mathrm{K}\), determine the total (i.e., integrated over all wavelengths) solar heat flux incident on the top of the Earth's atmosphere. The radius of the sun is \(6.96 \times 10^{8} \mathrm{~m}\), and a representative value of the sun-to-Earth distance is \(1.496 \times 10^{11} \mathrm{~m}\). Compare your result to the generally accepted annual mean value of \(1366 \mathrm{~W} \cdot \mathrm{m}^{-2}\) and discuss possible reasons for difference. b. Assuming that at a certain location and time, when the sun is in the zenith, the total heat flux arriving on the Earth surface is \(1100 \mathrm{~W} \cdot \mathrm{m}^{-2}\), calculate the balance between incoming and outgoing radiative heat flux at the surface of a pond of stagnant water when the sun is at an angle of \(30^{\circ}\) from the zenith. The total hemispherical emissivity of water is known to vary from \(0.95\) to \(0.963\) in the temperature range from 273 to \(373 \mathrm{~K}\) (Kaviany, 2002 ). c. The absorption coefficient \(\mathbf{\kappa}_{\lambda}\) of clear water is known to depend on wavelength. In the visible range \((0.4-0.7 \mu \mathrm{m})\), it varies from \(0.02\) to \(0.6 \mathrm{~m}^{-1}\) (Modest 2003, p. 416 ). By solving the radiative transfer equation, determine the decrease of intensity of incoming sunlight in a water layer with a depth \(0.1 \mathrm{~m}\) for the case that the sun is at an angle of \(30^{\circ}\) from the zenith.

The radiative transfer equation Equation (4.12) contains terms representing the effects of scattering. For the simplest case of isotropic scattering, the scattering phase function is constant \(\Phi_{\lambda}\left(\mathbf{s}^{*}, \mathbf{s}\right) \equiv 1\). For this case, show, by integrating the RTE over all directions, that scattering does not influence the value of the total incident radiation \(\mathrm{G}\).

What is the form of the mass transfer equation for a steady nonreactive balance between advection and diffusion?

See all solutions

Recommended explanations on Environmental Science Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free