Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
user_area:carbon_monitoring_satellite_carbonsat [2013/10/19 12:17]
arve [Results]
user_area:carbon_monitoring_satellite_carbonsat [2013/10/19 12:22]
arve
Line 20: Line 20:
 is also shown how aerosols, surface albedo and rotational Raman is also shown how aerosols, surface albedo and rotational Raman
 scattering may be included in the simulation. scattering may be included in the simulation.
 +
 ====== Spectral resolution ====== ====== Spectral resolution ======
 The requirement for the spectral resolution in the O<​sub>​2</​sub>​-A 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 resolution((Fontenla,​ J., White, O. R., Fox, P. A., Avrett, E. H., and
 Kurucz, R. L.: Calculation of solar irradiances. I. Synthesis of the 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 We use units of photons/​nm/​s/​m<​sup>​2</​sup>​ in order to be
 able to include rotational Raman scattering. The following uvspec able to include rotational Raman scattering. The following uvspec
Line 39: Line 40:
  
   wavelength 756 776   wavelength 756 776
-  ​+
 ====== O2-A band absorption ====== ====== O2-A band absorption ======
 High resolution absorption cross sections of the appropriate gases are High resolution absorption cross sections of the appropriate gases are
Line 152: Line 153:
 Rotational Raman scattering may be included by adding the following Rotational Raman scattering may be included by adding the following
 line. Note that this will increase the computing time by about a 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 ====== ====== Miscellanoues ======
Line 184: Line 185:
  
 We then modify some of the default values as follows: ​ We then modify some of the default values as follows: ​
-        ​+
   aerosol_vulcan 1          # Aerosol type above 2km   aerosol_vulcan 1          # Aerosol type above 2km
   aerosol_haze 6            # Aerosol type below 2km   aerosol_haze 6            # Aerosol type below 2km
Line 249: Line 250:
  
   conv UVSPEC_CARBONSAT_NC_noraman_aero.OUT slit_function_0.03_0.001 ​ > UVSPEC_CARBONSAT_NC_noraman_aero.OUTc_0.3   conv UVSPEC_CARBONSAT_NC_noraman_aero.OUT slit_function_0.03_0.001 ​ > UVSPEC_CARBONSAT_NC_noraman_aero.OUTc_0.3
- 
  
 The TOA radiance for the full wavelength region covered by the The TOA radiance for the full wavelength region covered by the
Line 278: Line 278:
 gzipped tar ball gzipped tar ball
 {{:​user_area:​carbon_monitoring_satellite_carbonsat:​carbonsat_example.tgz|}}. {{:​user_area:​carbon_monitoring_satellite_carbonsat:​carbonsat_example.tgz|}}.
- 
- 
- 
  
 
 
user_area/carbon_monitoring_satellite_carbonsat.txt ยท Last modified: 2013/10/19 12:22 by arve
Recent changes RSS feed Creative Commons License Valid XHTML 1.0 Valid CSS Driven by DokuWiki
Drupal Garland Theme for Dokuwiki