PDS_VERSION_ID                  = PDS3
LABEL_REVISION_NOTE             = "Figure Captions for Published Paper.
                                   John Haberman, 2006-03-14"

DATA_SET_ID                     = "HP-SSA-GCMS-3-FCO/DESCENT-V1.0" 
 REFERENCE_KEY_ID               = "NIEMANNETAL2005"
RECORD_TYPE                     = UNDEFINED
PRODUCT_ID                      = "FIGURE_2"
PRODUCT_CREATION_TIME           = 2006-03-14T12:15:00
^PNG_DOCUMENT                   = "FIGURE_2.PNG"

OBJECT                          = PNG_DOCUMENT
 DOCUMENT_NAME                  = "FIGURE_2"
 DOCUMENT_TOPIC_TYPE            = "SCIENCE REPORT"  
 INTERCHANGE_FORMAT             = BINARY
 PUBLICATION_DATE               = 2006-03-14                                  
 DOCUMENT_FORMAT                = "PNG"             
 DESCRIPTION                    = "
Figure 2 : The mole fraction of methane to nitrogen in the Titan
atmosphere is plotted versus altitude.  The CH4 mole fraction is 
1.41 x 10^-2 in the stratosphere. It begins increasing below 
32 km. At about 8 km, it reached a plateau of about 4.9 x 10^-2.
The inset shows an increase of methane at 16 m/z, when compared 
to nitrogen (in this case 14N^+ ) at m/z = 14, near 16 km. This 
is probably due to condensates evaporating in the inlet system 
of the mass spectrometer as the Huygens probe passed through 
the methane haze.
"
END_OBJECT                      = PNG_DOCUMENT

END