- Page 1: User’s GuideVLIDORTVersion 2.6Rob
- Page 6 and 7: 52H4. The68H5. References__________
- Page 8 and 9: 1.1.2. Development of Linearized Ve
- Page 10 and 11: and a complete differentiation of t
- Page 12 and 13: 8. (Version 2.6). The BRDF suppleme
- Page 15 and 16: 2. Description of the VLIDORT model
- Page 17 and 18: The six sets of “Greek constants
- Page 19 and 20: 2.1.4. Jacobian definitionsAtmosphe
- Page 21 and 22: Here, E is the 4 x 4 identity matri
- Page 23 and 24: This procedure was not used in the
- Page 25 and 26: ~L ( Ap~L ( Cp~(2)n(2)n) = −δL)
- Page 27 and 28: In Eq. (2.78), p = n + 1. For surfa
- Page 29 and 30: HH−+nα−−nα( x,μ)=( x,μ)=e
- Page 31 and 32: 1In the plane-parallel case, we hav
- Page 33 and 34: In section 2.4.1, scattering was as
- Page 35 and 36: oader layers at high SZA. Further,
- Page 37 and 38: transmitted direct-beam reflectance
- Page 39 and 40: 3. The numerical VLIDORT model3.1.
- Page 41 and 42: more algebra (chain rule differenti
- Page 43 and 44: 2000]; this can be used outside the
- Page 45 and 46: Verification of each stage of the l
- Page 47 and 48: 3.3.4. Solution savingIn DISORT and
- Page 49 and 50: This is a 2N system for the desired
- Page 51: time)*100%. Tests were made for sev
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unning the installation tests. Both
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the use of a toggle (OMEGA_SMALLNUM
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detail in section 4.3.2 below. Wher
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Finally, in vlidort_aux, there are
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and carried on with this default. I
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FORTRAN 90/95 compiler (courtesy V.
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# Main scalar testsSOURCES_SOLAR =
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4.3.4. Installation and testingTo i
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Table 4.5. Files for VLIDORT Scalar
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(3) Return the reply to the entry "
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There are two types of exception ha
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IN NO EVENT SHALL RT SOLUTIONS BE L
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Frankenberg, C., C. O'Dell, L. Guan
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Siewert, C.E., A concise and accura
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6. Appendices6.1 TablesThis section
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Table A4: Type Structure VLIDORT_Fi
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atmosphere with one cloud layer.DO_
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component S, incident solar angle s
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LAYER_VARY_NUMBER (n) Integer (I) N
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Table G3-1: Type structure VLIDORT_
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Table H4: Type Structure VLIDORT_Li
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DO_BVP_TELESCOPING Logical Do bound
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We now turn to more specific inform
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geometries and all 5 output levels.
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1. Ross-thin kernel - kernel factor
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In order to develop solutions in te
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given incident and reflected angles
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these are the BRDF parameters. E.g.
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6.3.3.2 BRDF configuration file cha
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22 1 ⎡ α ⎤P ( α,σ ) = exp⎢
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the models. Surface reflectance Jac
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We will also consider the simpler s
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environment will then call the subr
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Table B2: Type Structure VSLEAVE_In