* ARTS-XML-DATA-2-1-37

	* planets/Jupiter/MPS/Jupiter.mean/Jupiter.mean.H2O_high.xml.gz,
	planets/aux/isotopologue_ratios/isotopratios.txt: Bug fixes.



git-svn-id: https://radiativetransfer.org/svn/rt/arts-xml-data/trunk@8057 aaf1aab0-4228-0410-ad68-8dceda47f409

ChangeLog

+2012-11-26 Jana Mendrok <jana.mendrok@ltu.se>
+
+	* ARTS-XML-DATA-2-1-37
+
+	* planets/Jupiter/MPS/Jupiter.mean/Jupiter.mean.H2O_high.xml.gz,
+	planets/aux/isotopologue_ratios/isotopratios.txt: Bug fixes.
+
 2012-11-24 Jana Mendrok <jana.mendrok@ltu.se>
 
 	* ARTS-XML-DATA-2-1-36

planets/aux/isotopologue_ratios/isotopratios.txt

@@ -78,7 +78,7 @@ STEP (1a)
 molecule-specific isotopic ratios can be derived from ratios of isotopologues
  that apart from the two isotopes we want to derive the ratio of are identical
  (but we need to be a bit careful with positional permutation factors and when
- more than one atom of the species i replaced at once, e.g. two D occuring in
+ more than one atom of the species is replaced at once, e.g. two D occuring in
  a molecule)
 
 examples:
@@ -89,7 +89,7 @@ examples:
 
  IR(D2O) / IR(H2O) = [ia(O) * [(D/H)/(1+D/H)]**2] /
                      [ia(O) * 1/(1+D/H)**2]
-                   = (D/H)*2
+                   = (D/H)**2
  => D/H = sqrt( IR(D2O) / IR(H2O) )
 
 simple when only one atom of the species of question occurs, e.g.,