CRISM
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- FRT00013BEB_07_IF124S_TRR3
About CRISM
CRISM is a visible-infrared imaging spectrometer with a scanable field of view. CRISM can cover wavelengths from 0.362 to 3.92 microns (362 to 3920 nanometers) at 6.55 nanometers/channel, enabling the CRISM team to identify a broad range of minerals on the Martian surface.
CRISM is flying on the Mars Reconnaissance Orbiter, or MRO, launched in August 2005 from Cape Canaveral Air Force Station, Florida.
The Johns Hopkins University Applied Physics Laboratory managed CRISM's development.
CRISM is flying on the Mars Reconnaissance Orbiter, or MRO, launched in August 2005 from Cape Canaveral Air Force Station, Florida.
The Johns Hopkins University Applied Physics Laboratory managed CRISM's development.
CRISM: FRT00013BEB_07_IF124S_TRR3
Image Data
Click on the field name to see the glossary definition for that field.
Name | Value | Type | Idx |
---|---|---|---|
Image ID | FRT00013BEB_07_IF124S_TRR3 | Basic | 10 |
Bands | 107 | Basic | 11 |
Center Lat | -99.999° | Basic | 12 |
Center Lon | -999.999° | Basic | 13 |
Max Emission Angle | 37.538555° | Basic | 14 |
Min Emission Angle | 7.6170406° | Basic | 15 |
Max Incidence Angle | 36.605984° | Basic | 16 |
Min Incidence Angle | 35.950134° | Basic | 17 |
Lines | 420 | Basic | 18 |
Mars Year | 29 | Advanced | 19 |
MRO Activity Id | IF124 | Basic | 20 |
Instrument Pointing mode | DYNAMIC POINTING | Basic | 21 |
Wavelength | S | Basic | 22 |
Wavelength Filter | 0 | Basic | 23 |
Observation Id | 16#00013BEB# | Basic | 24 |
Observation Type | FRT | Basic | 25 |
Orbit | 0 | Basic | 26 |
Derived Data Record | http://pds-geosciences.wustl.edu/mro/mro-m-crism-6-ddr-v1/mrocr_1002/ddr/2009/2009_197/frt00013beb/frt00013beb_07_de124s_ddr1.img | Basic | 27 |
Derived Data Record Label | http://pds-geosciences.wustl.edu/mro/mro-m-crism-6-ddr-v1/mrocr_1002/ddr/2009/2009_197/frt00013beb/frt00013beb_07_de124s_ddr1.lbl | Basic | 28 |
Targeted Reduced Data Record | http://pds-geosciences.wustl.edu/mro/mro-m-crism-3-rdr-targeted-v1/mrocr_2103/trdr/2009/2009_197/frt00013beb/frt00013beb_07_if124s_trr3.img | Basic | 29 |
Targeted Reduced Data Record Label | http://pds-geosciences.wustl.edu/mro/mro-m-crism-3-rdr-targeted-v1/mrocr_2103/trdr/2009/2009_197/frt00013beb/frt00013beb_07_if124s_trr3.lbl | Basic | 30 |
Max Phase Angle | 62.796616° | Basic | 31 |
Min Phase Angle | 42.081318° | Basic | 32 |
Product Creation Time | 2010-11-25T19:03:49 | Advanced | 33 |
Image ID(s) | FRT00013BEB_07_DE124S_DDR1 | Basic | 34 |
Product Version | 3 | Basic | 35 |
Scan Mode | SHORT | Basic | 36 |
Solar Distance | 213962624 | Basic | 37 |
Solar Longitude | 304.16827 | Advanced | 38 |
Start Time (UTC) | 2009-07-16T03:47:50.452 | Basic | 39 |
Stop Time (UTC) | 2009-07-16T03:49:42.193 | Basic | 40 |
Volume ID | MROCR_2103 | Basic | 41 |
About CRISM
CRISM is a visible-infrared imaging spectrometer with a scanable field of view. CRISM can cover wavelengths from 0.362 to 3.92 microns (362 to 3920 nanometers) at 6.55 nanometers/channel, enabling the CRISM team to identify a broad range of minerals on the Martian surface.
CRISM is flying on the Mars Reconnaissance Orbiter, or MRO, launched in August 2005 from Cape Canaveral Air Force Station, Florida.
The Johns Hopkins University Applied Physics Laboratory managed CRISM's development.
CRISM is flying on the Mars Reconnaissance Orbiter, or MRO, launched in August 2005 from Cape Canaveral Air Force Station, Florida.
The Johns Hopkins University Applied Physics Laboratory managed CRISM's development.