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DTSTART:20160313T030000
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DTSTART:20161106T010000
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DTSTAMP:20161025T211237Z
UID:40AF6B43-9AF6-11E6-A7C6-0050568D7F66
DTSTART;TZID=America/New_York:20161031T150000
DTEND;TZID=America/New_York:20161031T160000
DESCRIPTION:With the advent of advanced instrumentation\, imaging spectrosc
 opy has been established as an irreplaceable technique for remotely sensin
 g the surface properties of planetary bodies. Imaging spectrometers have r
 evealed the composition of the surface of Mars\, the Moon\, and of course 
 the Earth. The spatial scale can vary from kilometers to micrometers\, whi
 le the wavelength range of interest spans the ultraviolet to the thermal i
 nfrared. In this talk we will review the enabling technologies that permit
  imaging spectrometers to achieve the required level of performance as wel
 l as application areas ranging from mineralogy to plant health\, water qua
 lity\, and ocean biology. We will also discuss the latest trends in instru
 mentation\, including CubeSat and Landsat-swath capability.\n\nCo-sponsore
 d by: SPIE-OSA Student Chapter\n\nSpeaker(s): Pantazis Mouroulis\, \, Pant
 azis Mouroulis\, \n\nRoom: CAR-2155\, Bldg: Building 76\, CIS\, Center for
  Imaging Science at RIT\, 54 Lomb Memorial Drive\, Rochester\, New York\, 
 United States\, 14623
LOCATION:Room: CAR-2155\, Bldg: Building 76\, CIS\, Center for Imaging Scie
 nce at RIT\, 54 Lomb Memorial Drive\, Rochester\, New York\, United States
 \, 14623
ORGANIZER:emmett@ientilucci.com
SEQUENCE:2
SUMMARY:Imaging Spectroscopy Technologies and Applications
URL;VALUE=URI:https://events.vtools.ieee.org/m/41831
X-ALT-DESC:Description: &lt;br /&gt;&lt;p&gt;&lt;span style=&quot;font-size: 10pt\;&quot;&gt;With the a
 dvent of advanced instrumentation\, imaging spectroscopy has been establis
 hed as an irreplaceable technique for remotely&amp;nbsp\;sensing the surface p
 roperties of planetary bodies. Imaging spectrometers have revealed the com
 position of the surface of Mars\, the&amp;nbsp\;Moon\, and of course the Earth
 . The spatial scale can vary from kilometers to micrometers\, while the wa
 velength range of interest spans&amp;nbsp\;the ultraviolet to the thermal infr
 ared. In this talk we will review the enabling technologies that permit im
 aging spectrometers to&amp;nbsp\;achieve the required level of performance as 
 well as application areas ranging from mineralogy to plant health\, water 
 quality\, and&amp;nbsp\;ocean biology. We will also discuss the latest trends 
 in instrumentation\, including CubeSat and Landsat-swath capability.&amp;nbsp\
 ;&lt;/span&gt;&lt;/p&gt;
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