European Space Agency
Mars Express: PFS
The Martian atmosphere consists mainly of carbon
dioxide and nitrogen with a very small proportion of
water vapour and ozone. The PFS (Planetary Fourier
Spectrometer) will measure the global atmospheric
distribution of water vapour and other minor
constituents with greater accuracy than previous
missions. The PFS Principal Investigator is
Dr. Davide Grassi,
Istituto di Fisica dello Spazio Interplanetario, Rome,
The primary source for PFS data is the
ESA Planetary Science Archive.
Through a cooperative agreement between ESA and NASA,
the PDS Geosciences Node is hosting a copy of the PFS
Copy of PFS Data at the PDS Geosciences Node
September 27, 2011. PFS Extended Mission 3
data through 31 Dec 2010 is now online.
April 7, 2011. This site now has
PFS data acquired between 23 June 2003 and 30 June 2010.
More information about PFS is on the
ESA web site.