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--- user_area:carbon_monitoring_satellite_carbonsat [2013/10/19 12:14]
arve [Results]
+++ user_area:carbon_monitoring_satellite_carbonsat [2013/10/19 12:22] (current)
arve
@@ Line 20: / Line 20: @@
 is also shown how aerosols, surface albedo and rotational Raman
 scattering may be included in the simulation.
 ====== Spectral resolution ======
 The requirement for the spectral resolution in the O<sub>2</sub>-A
@@ Line 29: / Line 30: @@
 resolution((Fontenla, J., White, O. R., Fox, P. A., Avrett, E. H., and
 Kurucz, R. L.: Calculation of solar irradiances. I. Synthesis of the
-solar spectrum, The Astrophysical Journal, 518, 480-499, 1999.))
+solar spectrum, The Astrophysical Journal, 518, 480-499, 1999.)).
 We use units of photons/nm/s/m<sup>2</sup> in order to be
 able to include rotational Raman scattering. The following uvspec
@@ Line 39: / Line 40: @@
   wavelength 756 776
 ====== O2-A band absorption ======
 High resolution absorption cross sections of the appropriate gases are
@@ Line 152: / Line 153: @@
 Rotational Raman scattering may be included by adding the following
 line. Note that this will increase the computing time by about a
-factor of 480.
+factor of 640.
-  #raman # Uncomment to include rotational Raman scattering.
+  raman
 ====== Miscellanoues ======
@@ Line 184: / Line 185: @@
 We then modify some of the default values as follows:
   aerosol_vulcan 1          # Aerosol type above 2km
   aerosol_haze 6            # Aerosol type below 2km
@@ Line 268: / Line 269: @@
 {{:user_area:carbon_monitoring_satellite_carbonsat:toa_spectra_aero.png?800|}}
+Rotational Raman scattering was included in the spectra above. The
+filling-in for no aerosols and with aerosols are shown below.
+{{:user_area:carbon_monitoring_satellite_carbonsat:toa_fi_aero.png?800|}}
+====== Input files ======
+The various input and output files discussed above are available as a
+gzipped tar ball
+{{:user_area:carbon_monitoring_satellite_carbonsat:carbonsat_example.tgz|}}.