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Mnemonic:

UVS_JUP_AP_AIRGLOW_STARE

Name:

UVS Jupiter AP Airglow Stare

Description:

Monitoring auroral and airglow emissions in stare mode using the Airglow Port (AP). Slit held along Jupiter' s North/South and on the central meridian, while Jupiter rotates below S/C creating a map. Histogram mode.

Payload:

UVS

Pointing

Pointing Type:

nadir

Target:

PTRSnippet file:

Advanced

Scheduling Rules:

- Specific cadence for a given period during the tour, to be constrained by 1 Gbit/week data downlink. - Observations including when distance to Jupiter R>20 Rj - To assess temporal evolution requires repetitive observations, including over short periods to look for changes over short periods

any rule that is used to schedule the observation: repetition rules, continuous (plasma instruments), one-off, every orbit, every day, etc

Avoidance Rules:

N/A

conditions that make the observation not possible (e.g. thruster firing)

Comments:

Support Plot 1:

Support Plot 2:

Support Plot 3:

Commanding

ITLSnippet file:

Power profiles

	Event	Time	Mode	User Defined Power (Watts)	Comment
Start 00:00:00 SCIENCE 8.17 [Watt]	Start	00:00:00	SCIENCE	-

Data profiles

	Event	Time	Mode	User Defined Data Rate (bit/s)	Comment
Start 00:00:00 User Defined 2250.0 [bit/s]	Start	00:00:00	User Defined	2250.0	Updated from PJ12.
Start 00:00:00 User Defined 22630.0 [bit/s]	Start	00:00:00	User Defined	22630.0	Added from 002 in PJ12

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