Commit 386a1661 authored by Tyler Wilson's avatar Tyler Wilson
Browse files

PROG: Removed all references to special multi-byte characters in the XML file... 

PROG:  Removed all references to special multi-byte characters in the XML file because they were causing problems on progs 10,12 and 6.  References #3880.

git-svn-id: http://subversion.wr.usgs.gov/repos/prog/isis3/trunk@6897 41f8697f-d340-4b68-9986-7bafba869bb8
parent 912fa215

isis/src/hayabusa/apps/amicacal/amicacal.xml

+11 −11
Original line number Diff line number Diff line
@@ -239,7 +239,7 @@ xsi:noNamespaceSchemaLocation="http://isis.astrogeology.usgs.gov/Schemas/Applica 
    This converts the raw DN values to I/F (radiance) units.  The formula is:

    <br/><br/>

     <div style="font-size:90%; font-family:monospace; margin:5px; margin-left:30px;">

      <center><strong>IoF = Raw*[&#960;*(R<sub>s</sub>)<sup>2</sup>]/F</strong></center>

      <center><strong>IoF = Raw*[pi*(R<sub>s</sub>)<sup>2</sup>]/F</strong></center>

      <br/><br/>

      <center><table border="1" cellpadding="5">

      <tr>
@@ -272,17 +272,17 @@ xsi:noNamespaceSchemaLocation="http://isis.astrogeology.usgs.gov/Schemas/Applica 
    form:

    <br/><br/>

     <div style="font-size:90%; font-family:monospace; margin:5px; margin-left:30px;">

                          <center> <strong>F<sub>foc</sub>(r) = exp(-&#945;*r) </strong></center>

                          <center> <strong>F<sub>foc</sub>(r) = exp(-alpha*r) </strong></center>

     </div>

     <br/><br/>

     The variable <strong>r</strong> is the distance in pixels from the optical center of the point

     source.  The values of <strong>&#945;</strong> for the different filters are listed below:

     source.  The values of <strong>alpha</strong> for the different filters are listed below:

     <br/><br/>

     <div style="font-size:90%; font-family:monospace; margin:5px; margin-left:30px;">



      <center><table border = "1" cellpadding="5">

      <tr>

          <td> Filter</td><td> &#945;</td>

          <td> Filter</td><td> alpha</td>

      </tr>

      <tr>

          <td> ul </td><td> 1.26 </td>
@@ -314,13 +314,13 @@ xsi:noNamespaceSchemaLocation="http://isis.astrogeology.usgs.gov/Schemas/Applica 


     <div style="font-size:90%; font-family:monospace; margin:5px; margin-left:30px;">

     <center> <strong>F<sub>ufoc</sub>(r) =  SUM(i=1...N){ [A<sub>i</sub>/

     (&#963;<sub>i</sub>*SQRT(2*&#960;))]

     * exp(-r<sup>2</sup>/2*(&#963;<sub>i</sub>)<sup>2</sup>}

     (sigma<sub>i</sub>*SQRT(2*pi))]

     * exp(-r<sup>2</sup>/2*(sigma<sub>i</sub>)<sup>2</sup>}

     </strong></center>

     </div>

     Both the focused and the unfocused components are calculated for each pixel in the image, and

     subtracted out of the final calibrated image.

     <strong>A<sub>i</sub></strong> and <strong>&#963;<sub>i</sub></strong> are constants

     <strong>A<sub>i</sub></strong> and <strong>sigma<sub>i</sub></strong> are constants

     derived empircally from images of Itokawa and the Moon and enumerated below:

     <br/><br/>
@@ -373,9 +373,9 @@ xsi:noNamespaceSchemaLocation="http://isis.astrogeology.usgs.gov/Schemas/Applica 
    <center><table border="1" cellpadding="5">



    <tr>

        <td></td><td>&#963;<sub>1</sub></td><td>&#963;<sub>2</sub></td><td>&#963;<sub>3</sub></td>

        <td>&#963;<sub>4</sub></td><td>&#963;<sub>5</sub></td>

        <td>&#963;<sub>6</sub></td>

        <td></td><td>sigma<sub>1</sub></td><td>sigma<sub>2</sub></td><td>sigma<sub>3</sub></td>

        <td>sigma<sub>4</sub></td><td>sigma<sub>5</sub></td>

        <td>sigma<sub>6</sub></td>

    </tr>

    <tr>

        <td>All bands</td><td>8</td><td>16</td><td>32</td><td>64</td><td>110</td>
@@ -402,7 +402,7 @@ xsi:noNamespaceSchemaLocation="http://isis.astrogeology.usgs.gov/Schemas/Applica 
    The output units of the DNs will depend on which calibration flags are turned on.

    <ul>

      <li>If IOF=TRUE, output units are measured in I/F</li>

      <li>Otherwise output units are measured in W/(m**2 micrometer sr)</li>

      <li>Otherwise output units are measured in W/(m<sup>2</sup> micrometer sr)</li>

    </ul>

  </p>