Stim Application: UVS Operations

Fake Card

fake card

Templates:

Dark Observation

Templates:

UVS_001_AP_SAA

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

Templates:

UVS_001_AP_SAA

[55 nm - 132.4 nm] = 0.6007751937984496 nm [132.4 nm - 210 nm] = 0.3007751937984496 nm [55 nm - 132.4 nm] = 0.6007751937984496 nm [34 nm - 132.4 nm] = 1.2299465240641712 nm

Templates:

sdjalkf

[55 nm - 132.4 nm] = 77.4 nm [132.4 nm - 210 nm] = 77.6 nm [55 nm - 132.4 nm] = 77.4 nm [132.4 nm - 210 nm] = 77.6 nm

Templates:

Umer

[55 nm - 126.3 nm] = 77.4 nm [126.3 nm - 210 nm] = 77.6 nm [55 nm - 126.3 nm] = 77.4 nm [126.3 nm - 210 nm] = 77.6 nm [55 nm - 126.3 nm] = 77.4 nm [126.3 nm - 210 nm] = 77.6 nm

Templates:

Observation Cards

Stim Templates

Fake Card

Dark Observation

UVS_001_AP_SAA

UVS_001_AP_SAA

sdjalkf

Umer

Dark Observation

UVS_001_AP_SAA

UVS_001_AP_SAA

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

Observation Cards

Stim Templates

Fake Card

Dark Observation

UVS_001_AP_SAA

UVS_001_AP_SAA

sdjalkf

Umer

Basic STIM 3 observations

Dark Observation

UVS_001_AP_SAA

UVS_001_AP_SAA