From 602e3f541733ff7797e0fddff0e8edd8c09e011a Mon Sep 17 00:00:00 2001 From: Manuel Grizonnet <manuel.grizonnet@orfeo-toolbox.org> Date: Tue, 26 Aug 2014 16:21:08 +0200 Subject: [PATCH] BUG: rendering of app long description is wrong in the cookbook(pdf) --- Applications/Radiometry/otbOpticalCalibration.cxx | 8 ++++---- 1 file changed, 4 insertions(+), 4 deletions(-) diff --git a/Applications/Radiometry/otbOpticalCalibration.cxx b/Applications/Radiometry/otbOpticalCalibration.cxx index 4ecc65abab..5f84494049 100644 --- a/Applications/Radiometry/otbOpticalCalibration.cxx +++ b/Applications/Radiometry/otbOpticalCalibration.cxx @@ -141,7 +141,7 @@ private: "- solar illuminations, one value for each band (passed by a file).\n\n" "For the conversion from DN (for Digital Numbers) to spectral radiance (or 'TOA radiance') L, the following formula is used :\n\n" -"(1)\tL(b) = DN(b)/gain(b)+bias(b)\t(in W/m²/steradians/micrometers)\twith b being a band ID.\n\n" +"(1)\tL(b) = DN(b)/gain(b)+bias(b)\t(in W/m2/steradians/micrometers)\twith b being a band ID.\n\n" "These values are provided by the user thanks to a simple txt file with two lines, one for the gains and one for the biases.\n" "Each value must be separated with colons (:), with eventual spaces. Blank lines are not allowed. If a line begins with the '#' symbol, then it is considered as comments.\n" @@ -150,7 +150,7 @@ private: "In order to convert TOA radiance to TOA reflectance, the following formula is used :\n\n" -"(2)\tR(b) = (pi*L(b)*d²) / (ESUN(b)*cos(θ))\t(no dimension)\twhere : \n\n" +"(2)\tR(b) = (pi*L(b)*d*d) / (ESUN(b)*cos(θ))\t(no dimension)\twhere : \n\n" "- L(b) is the spectral radiance for band b \n" "- pi is the famous mathematical constant (3.14159...) \n" @@ -163,9 +163,9 @@ private: "These values are provided by the user thanks to a txt file following the same convention as before.\n" "Instead of providing the date of acquisition, the user can also provide a flux normalization coefficient 'fn'. " "The formula used instead will be the following : \n\n" -"(3) \tR(b) = (pi*L(b)) / (ESUN(b)*fn²*cos(θ)) \n\n" +"(3) \tR(b) = (pi*L(b)) / (ESUN(b)*fn*fn*cos(θ)) \n\n" "Whatever the formula used (2 or 3), the user should pay attention to the interpretation of the parameters he will provide to the application, " -"by taking into account the original formula that the metadata files assum.\n\n" +"by taking into account the original formula that the metadata files assumes.\n\n" "Below, we give two examples of txt files containing information about gains/biases and solar illuminations :\n\n" "- gainbias.txt :\n" -- GitLab