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Hi Rod, re: > Oh and one more thing..... > > I am still trying to figure out how to do this part: > > How do I find the reflection angle of visible and effective radius? I think you mean solar zenith angle. There is no routine in core McIDAS that outputs solar zenith angle for individual points or Lat,Lon boxes. There is, however, a routine in McIDAS XRD (X Research and development) that can output the solar zenith angle for individual points. The routine I am referring to is SATANGLES. Since the XRD portion of the Unidata McIDAS-X distribution is not built/installed by default, it is possible that you will have to build and install it yourself: <logged in as 'mcidas' on iset2> cd ~/mcidas2009/src make xrd make install.xrd Since XRD routines are not part of McIDAS core, their documentation can be "sketchy", and they will not be found in the McIDAS-X User's Guide. The only documentation for SATNAGLES is, therefore, through HELP: HELP SATANGLES The bad thing about SATANGLES is that it is usable for images that are currently loaded into a McIDAS session frames. One then has to move the mouse cursor over a point and then run SATANGLES to get information for the pixel selected. The other MAJOR limit to using SATANGLES is that it only works for select navigation types: HELP SATANGLES SATANGLES -- Lists satellite zenith, solar zenith, and relative angles at cursor location SATANGLES Remark: Works for GOES, GVAR and GMS Navigation This is a renamed copy of a McIDAS-XRD 2007 routine called ANGLES. Renaming was needed since there is a subroutine in the McIDAS distribution called angles.for. ---------- This means that it will work for your original images (e.g., images from the G13/IR27APR11 dataset), but not for remapped images (e.g., images created by IMGREMAP). re: > Is there a way they can be in a ASCII text file? SATANGLES does not have an option to write its output to ASCII text files, but information for individual pixels can be written to ASCII text files by specifying the DEV=T <fname> keyword sequence in SATANGLES invocations. Since the solar zenith angle should not change drastically over the area that you are interested in for a particular time, you may be able to do spot checks to see if the pixels can be kept pursuant to the guidelines you forwarded in a previous email: > On Wed, Oct 31, 2012 at 11:01 AM, Dan Lindsey <address@hidden> wrote: > Hi Nimrod, > > I calculate the solar zenith angle (it's a function of latitude, > longitude, date, and time), and only consider effective radius > retrievals valid when the solar zenith angle is less than 68 degrees > (90 degrees means the sun is on the horizon, and 0 degrees means > directly overhead). I don't know if MATLAB has a solar zenith angle > routine. > ... Cheers, Tom -- **************************************************************************** Unidata User Support UCAR Unidata Program (303) 497-8642 P.O. Box 3000 address@hidden Boulder, CO 80307 ---------------------------------------------------------------------------- Unidata HomePage http://www.unidata.ucar.edu **************************************************************************** Ticket Details =================== Ticket ID: RDQ-637778 Department: Support McIDAS Priority: Normal Status: Closed