Difference between revisions of "UCSD-2019: Technical Working Group: SATs"

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== Charge ==
 
== Charge ==
  
 +
Generic L2 Parallel charge:
  
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* Identify key decisions that must be made (and justified) prior to CD-1
 +
* Make progress on (or actually make) those decisions,
 +
* Lay out a timeline and process for making each decision, consistent with the post-decision work and internal reviews that will be needed to complete preparations for CD-1,
 +
*  Ensure that those timelines and processes are understood and supported by the collaboration, and that we (together) believe we can follow them.
 +
 +
Attempt at S4 SAT-specific “Goal” statement:
 +
 +
“In order to meet CD-1 and 3a goals by Spring 2021, the SAT group is organizing inputs for a key decision followed by review in early 2020.  We anticipate this will entail a downselect between single-tube and three tube SAT cryostat options, including a definition of the interface between cryocoolers and telescope mounts, mount geometry, and configuration.  Our goal for this October session is to identify the inputs we need to make a good decision in early 2020, confirm the path to getting those and the earliest possible timeline.”
  
 
== Agenda ==
 
== Agenda ==

Revision as of 09:20, 17 October 2019

Link back to agenda

Charge

Generic L2 Parallel charge:

  • Identify key decisions that must be made (and justified) prior to CD-1
  • Make progress on (or actually make) those decisions,
  • Lay out a timeline and process for making each decision, consistent with the post-decision work and internal reviews that will be needed to complete preparations for CD-1,
  • Ensure that those timelines and processes are understood and supported by the collaboration, and that we (together) believe we can follow them.

Attempt at S4 SAT-specific “Goal” statement:

“In order to meet CD-1 and 3a goals by Spring 2021, the SAT group is organizing inputs for a key decision followed by review in early 2020. We anticipate this will entail a downselect between single-tube and three tube SAT cryostat options, including a definition of the interface between cryocoolers and telescope mounts, mount geometry, and configuration. Our goal for this October session is to identify the inputs we need to make a good decision in early 2020, confirm the path to getting those and the earliest possible timeline.”

Agenda

Remote attendance

Zoom link


Notes