UVS_001_AP_SAA - View Observation Card: UVS Operations

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Constants

Definition Type	Mode Type	Time Sampling (sec)	Total Integration Time (sec)	Pulse Height (bins)	Pulse Height (bits)	Count Rate	Background Rate	Well Depth (bits)	Framing Overhead Histogram	Altitude
Pixel List Histogram	AP HP

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This observation is for distant (>+/- 2 hours) SAA stares with high spectral resolution across the slit to look for al species, including the N2 LHB band emissions (125 – 220nm), N (124nm, 141 nm, 149 nm), Cl (lines between 118 – 140), Ca (188.3), Mg (182.8), CO (151 and 148 nm) and C (156 nm and 155 nm), and H2 and Werner bands (85 – 165 nm), Sulfur emissions.

Acquired in AP mode to collect as many photons as possible, especially with the very high spectral resolution.

This example created for when Clipper is ~100,000 km from Europa

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	Spectral Dimension		Spatial Dimension		mode Binning Resolution				(Mbits/sec)	(Mbits)	(Mbits)
#	Min Wavelength (nm)	Max Wavelength (nm)	Spatial Bin Bottom (°)	Spatial Bin Top (°)	Spectral Bins		Spatial Bins		Data Rate	Science Data Volume	Total Data Volume
1	pixel	pixel	pixel	pixel	resolution (nm)	# of X bins limit	resolution °	# of Y bins limit
2	pixel	pixel	pixel	pixel	resolution (nm)	# of X bins limit	resolution °	# of Y bins limit
3	pixel	pixel	pixel	pixel	resolution (nm)	# of X bins limit	resolution °	# of Y bins limit
4	pixel	pixel	pixel	pixel	resolution (nm)	# of X bins limit	resolution °	# of Y bins limit
5	pixel	pixel	pixel	pixel	resolution (nm)	# of X bins limit	resolution °	# of Y bins limit
6	pixel	pixel	pixel	pixel	resolution (nm)	# of X bins limit	resolution °	# of Y bins limit
7	pixel	pixel	pixel	pixel	resolution (nm)	# of X bins limit	resolution °	# of Y bins limit
8	pixel	pixel	pixel	pixel	resolution (nm)	# of X bins limit	resolution °	# of Y bins limit
					Totals
					Total Bits

WD
SIH
TOI
Spec
Spat
PHB
LUT
Masks
FO
Science DV
Total DV

SC
BC
HP
IT
Spec
Spat
PH
LUT
Masks
FO
Science DV
Total DV