By Peter V. Hobbs
This moment variation of An advent to Atmospheric Radiation has been commonly revised to deal with the elemental learn and quantitative size of the interactions of sunlight and terrestrial radiation with molecules, aerosols, and cloud debris in planetary atmospheres. It comprises 70% new fabric, a lot of it stemming from the research of the atmospheric greenhouse results of exterior radiative perturbations in weather platforms, and the advance of methodologies for inferring atmospheric and floor parameters via distant sensing. Liou's complete remedy of the basics of atmospheric radiation used to be constructed for college kids, lecturers, and researchers in atmospheric sciences, distant sensing, and weather modeling.Features*Balanced remedy of basics and applications*Includes over a hundred and seventy illustrations to enrich the concise description of every subject*Numerous examples and hands-on routines on the finish of every chapterAbout the AuthorDr. ok. N. Liou is Professor of Atmospheric Sciences on the collage of California, la. he's a member of the nationwide Academy of Engineering and Fellow of AAAS, AGU, AMS, and the Optical Society of the USA. Professor Liou got the Jule G. Charney Award from AMS in 1998 "for his pioneering paintings within the thought and alertness of radiative move and its interplay with clouds."
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Extra resources for Aerosol–Cloud–Climate Interactions
Atmospheric Radiation. Theoretical Basis, 2nd ed. Oxford University Press, New York. Chapter 3 presents an authoritative and advanced discussion of the vibration–rotation spectra of molecules. , and Thompson, M. H. (1984). Astronomy: Fundamentals and Frontiers, 2nd ed. Wiley, New York. Chapter 4 contains an excellent description in lay terms of absorption line formation. McCartney, E. J. (1983). Absorption and Emission by Atmospheric Gases. Wiley, New York. Chapters 4 and 5 provide enlightened discussions of the fundamentals of rotational, vibrational, and electronic transitions.
This leads to τ∗ I (τ ; μ, φ) = I (τ∗ ; μ, φ)e−(τ∗ −τ )/μ + τ J (τ ; μ, φ)e−(τ −τ )/μ dτ (1 ≥ μ > 0). 23) To derive the downward intensity (μ < 0) at level τ , a factor eτ/μ is used and μ is replaced by −μ. After carrying out integration from τ = 0 to τ , we obtain τ I (τ ; −μ, φ) = I (0; −μ, φ)e−τ/μ + J (τ ; −μ, φ)e−(τ −τ )/μ 0 dτ (1 ≥ μ > 0). 24) In Eqs. 24), I (τ∗ ; μ, φ) and I (0; −μ, φ) represent the inward source intensities at the bottom and top surfaces, respectively, as shown in Fig. 16.
1984). Astronomy: Fundamentals and Frontiers, 2nd ed. Wiley, New York. Chapter 4 contains an excellent description in lay terms of absorption line formation. McCartney, E. J. (1983). Absorption and Emission by Atmospheric Gases. Wiley, New York. Chapters 4 and 5 provide enlightened discussions of the fundamentals of rotational, vibrational, and electronic transitions. Penner, S. S. (1950). Quantitative Molecular Spectroscopy and Gas Emissivities. Addison-Wesley, Reading, MA. Chapters 1–3 provide helpful explanations of blackbody radiation and absorption line proﬁles.