2. The maximum wavelength of an ideal black body cavity radiation absorption is 6000 A. a....
Why is the radiation in a cavity as if it came from a "black body"?
8. Compute the ratio of the increase of intensity of black-body radiation at a wavelength of 641 nm for an increase of temperature from 1200 to 1500 K
At what temperature must a body be heated to generate black-body spectrum with a maximum wavelength of 160nm.
A star has the maximum emission at a wavelength lmax=300 nm. Calculate the surface temperature of the star, assuming that the star behaves like an ideal black body.
A black body has an effective surface temperature of 450°C. Determine: (a) The total radiation energy (W/m2) that can be emitted by the black body (b) Determine total radiation energy (W/m%) that can be emitted by the black body within the 5-50 um wavelength region (c) The spectral blackbody emissive power of the black body at a wavelength of 10 um. 12
8. A black body has an effective surface temperature of 450°C. Determine: (a) The total radiation energy (W/m²) that can be emitted by the black body (b) Determine total radiation energy (W/m²) that can be emitted by the black body within the 5-50 um wavelength region (c) The spectral blackbody emissive power of the black body at a wavelength of 10 um.
The thermal emission of the human body has maximum intensity at a wavelength of approximately 9.5um.Part A:What photon energy corresponds to this wavelength?E = _______
The Wien displacement law states that the wavelength maximum in micrometers for blackbody radiation is A T = 2.9 x 10 where Tis the temperature in kelvins. Calculate the wavelength maximum for a blackbody that has been heated to a 10000 K Wavelength = jum b. 6000 K Wavelength= um c. 2000 K Wavelength = um d. 1000 K Wavelength = um
A star can be approximated to a black body mostly constituted of gas with a surface temperature T. From the black body density of oscillators we can demonstrate that the power emitted in the forward direction by the star of surface area A per unit wavelength is: A exp( )-1 (Eg.1) Maximum emission Using Equation I , give an approximation of the power Permitted at short wavelengths (λ<<1). c.
7. What is the relation between temperature and intensity of black body radiation? 8. What is the relation between the temperature of a black body and the color of its radiation? 9. What is the closest thing to a black body in our everyday life? 10. What is the importance of Planck's radiation law for modern Physics?