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        <Text>&lt;p&gt;The Les Houches school of physics has always  played a pioneering role in the development of  French and European science since its birth.  In our field, it can be noted the sessions  held in 1974 and 1983 (physics and chemistry  of the interstellar medium) to prepare the  community to IRAM, in 1991 and 1998 for ISO,  in 1990 for the teledetection and space use of  heterodyne techniques (Odin, SMOS and MIRO on  Rosetta) and in 2007 for the Herschel  venture.&lt;/p&gt; &lt;p&gt; For the first time, three complementary  techniques will be used on the same spacecraft  to observe the Far Infrared domain that cannot  be observed from the ground due to atmospheric  opacity: coherent detection techniques,  spectrophotometry and imaging at Terahertz  frequencies.  Most of the laboratories working  in these technologically difficult areas  (experiments at 2 Kelvin are complicated  enough in the laboratory, but in space it is a  real challenge) have built these instruments  in worldwide consortia.&lt;/p&gt; &lt;p&gt;This session has been supported by CNRS, INSU,  CEA, CNES, ESA, MESR, Observatoire de Paris,  Observatoire de Marseille-Provence and  Université Joseph Fourier.  P.J. Encrenaz, Herschel Mission Scientist.&lt;/p&gt;</Text>
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        <Text>&lt;p&gt;The Les Houches school of physics has always  played a pioneering role in the development of  French and European science since its birth.  In our field, it can be noted the sessions  held in 1974 and 1983 (physics and chemistry  of the interstellar medium) to prepare the  community to IRAM, in 1991 and 1998 for ISO,  in 1990 for the teledetection and space use of  heterodyne techniques (Odin, SMOS and MIRO on  Rosetta) and in 2007 for the Herschel  venture.&lt;/p&gt; &lt;p&gt; For the first time, three complementary  techniques will be used on the same spacecraft  to observe the Far Infrared domain that cannot  be observed from the ground due to atmospheric  opacity: coherent detection techniques,  spectrophotometry and imaging at Terahertz  frequencies.  Most of the laboratories working  in these technologically difficult areas  (experiments at 2 Kelvin are complicated  enough in the laboratory, but in space it is a  real challenge) have built these instruments  in worldwide consortia.&lt;/p&gt; &lt;p&gt;This session has been supported by CNRS, INSU,  CEA, CNES, ESA, MESR, Observatoire de Paris,  Observatoire de Marseille-Provence and  Université Joseph Fourier.  P.J. Encrenaz, Herschel Mission Scientist.&lt;/p&gt;</Text>
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