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Mnemonic:

UVS_JUP_SP_SOL_OCC

Name:

UVS Jupiter SP Solar Occultation

Description:

The large solar disc and the substantial distance from Jupiter mean that this will not provide the same vertical resolution as stellar occultations, but are useful for measurements of minor/trace constituents due to high S/N. This uses a fixed scan through the Solar Port (SP) at a selected RA and DEC, holding the pointing for an extended amount of time. Note: Here histograms, but pixellist mode possible.

Payload:

UVS

Pointing

Pointing Type:

inertial

Target:

Jupiter atmosphere

PTRSnippet file:

Advanced

Scheduling Rules:

- Event driven (both ingress and egress). - 3 or more events during the tour. Mix of low-latitude and mid-latitude events (so include one or more occultations during the high inclination phase) Synergistic observations with SWI. (no solar occult with MAJIS)..

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 73800.0 [bit/s]	Start	00:00:00	User Defined	73800.0

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