Rotational Raman scattering in the Earth's atmosphere ... - SRON

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68 Chapter 3 Figure 3.13: Same as Fig. 3.12 but for different atmospheric parameters. The calculations are performed for a solar and viewing geometry of ϑ 0 = 40 ◦ , ϑ v = 10 ◦ , ∆ϕ = 120 ◦ . (left panel) Dependence on ozone column C = 200–400 DU for an albedo of A = 0.1. (middle panel) Dependence on Lambertian ground albedo A = 0.0–1.0 for a vertically integrated ozone column of C = 300 DU. (right panel) Truncated atmosphere at a truncation height z trun =0–10 km for a Lambertian ground albedo = 0.8. The difference in b mean for the error scenarios e min and e max is less than 0.02 for I app1 , and less than 0.03 and 3.00 for I app2 and I app3 , respectively.
A vector radiative transfer model using the perturbation theory approach 69 Figure 3.14: Mean relative bias b mean as function of solar zenith angle ϑ 0 for simulated GOME measurements I pol and model simulations I app1 , I app2 , and I app3 in Eqs. (3.66), (3.67) and (3.68) at the center of the Ca II K and H Fraunhofer lines at 393.5 and 396.8 nm. The model atmosphere and the viewing geometry are the same as for the left panel of Fig. 3.12. The difference in b mean for the error scenarios e min and e max is less than 0.04 for I app1 , and less than 0.04 and 2.43 for I app2 and I app3 , respectively.
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VRIJE UNIVERSITEIT Rotational Raman
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Contents 1 Introduction 1 1.1 Obser
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1 Introduction 1.1 Observing skylig
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Introduction 3 Extracting the wealt
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Introduction 5 and Spurr, 1997, Vou
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Introduction 7 energy: E rot (v,J)
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Introduction 9 Figure 1.4: Probabil
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Introduction 11 scattered radiance
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Introduction 13 approximation in wh
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Introduction 15 scattering have bee
Page 23 and 24: 2 A doubling-adding method to inclu
Page 25 and 26: A doubling-adding method to include
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Page 46 and 47: 40 Chapter 3 nm with a spectral res
Page 48 and 49: 42 Chapter 3 contributions of lower
Page 50 and 51: 44 Chapter 3 if we use the effectiv
Page 52 and 53: 46 Chapter 3 This in turn results i
Page 54 and 55: 48 Chapter 3 This may be shown in a
Page 56 and 57: 50 Chapter 3 The forward and adjoin
Page 58 and 59: 52 Chapter 3 Here, ∆ = diag [1, 1
Page 60 and 61: 54 Chapter 3 Figure 3.3: Relative R
Page 62 and 63: 56 Chapter 3 biases the simulation
Page 64 and 65: 58 Chapter 3 3.4.2 Approximation me
Page 66 and 67: 60 Chapter 3 where I ram,app and I
Page 68 and 69: 62 Chapter 3 3.5 Simulation of pola
Page 70 and 71: 64 Chapter 3 Figure 3.10: Relative
Page 72 and 73: 66 Chapter 3 dependence on the vert
Page 76 and 77: 70 Chapter 3 3.6 Summary A vector r
Page 78 and 79: 72 Chapter 3 where λ is the wavele
Page 80 and 81: 74 Chapter 3 where S l is the expan
Page 82 and 83: 76 Chapter 3 3.C Appendix: Evaluati
Page 85 and 86: 4 Accurate modeling of spectral fin
Page 87 and 88: Accurate modeling of spectral fine-
Page 103 and 104: 5 Retrieval of cloud properties fro
Page 105 and 106: Retrieval of cloud properties from
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References Aben, I., F. Helderman,
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References 121 Ellery, A., D. Wynn-
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References 123 Lacis, A. A., J. Cho
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References 125 Schulz, F., K. Stamn
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Summary A spectrum of sunlight that
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Summary 129 Earth radiance spectrum
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Samenvatting Het door de aardatmosf
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Samenvatting 133 met een vector-mod
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