Go to the U of M home page
School of Physics & Astronomy
Probe Mission Study Wiki

User Tools


imagerteleconnotes20170807

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revisionPrevious revision
Next revision
Previous revision
imagerteleconnotes20170807 [2017/08/14 10:18] hananyimagerteleconnotes20170807 [2017/08/14 10:48] (current) hanany
Line 6: Line 6:
  
 __Action Items__ __Action Items__
 +  * UMN to develop focal plane loading model including load from mirror(s) and cold stop as a function of temperature
 +  * JPL to develop scaling of cooling cost depending on what mass we cool to which temperature
 +  * Need input on feasibility and cost model of deployable shields
 +  * Need input on cooling and trade-off with mass of stop and secondary mirror
 +  * Roger to work on ASIC solutions to TDM, FDM
 +    * discuss with Matt
 +    * do wiring load trade-off between the two options
    
 ====Telecon Notes==== ====Telecon Notes====
  
-Optics+__Optics__
   * UMN reviews tradeoff study between open and cross Dragon. For fixed aperture and f# Open Dragone has 3/4 the DLFOV of the crossed system. Largely agrees with the result from the comparison shown a week before when they had different f#.   * UMN reviews tradeoff study between open and cross Dragon. For fixed aperture and f# Open Dragone has 3/4 the DLFOV of the crossed system. Largely agrees with the result from the comparison shown a week before when they had different f#.
   * How large is the stop in the current Open Dragone design?   * How large is the stop in the current Open Dragone design?
Line 28: Line 35:
     * What are 'good' scan angles? Kris said with high confidence that he would give a report next week on scanning strategy.     * What are 'good' scan angles? Kris said with high confidence that he would give a report next week on scanning strategy.
  
 +__Focal Plane Technology__
 +
 +Roger and Jeff post their answers to the questions Shaul posed on last week on last week’s minutes page. 
 +
 +  * Q1: what is the plan for detector technology for the high frequency bands of the imager?
 +    * monochroic PSBs above 600 GHz because of Nb band gap. Not suitable for Nb-based antenna coupling. 
 +  * Q2: are the distribution of colors for pixels as described by the worksheet reasonable?
 +    * Yes. 2-3 colors per pixel is OK. Perhaps could fit more bands in lower frequency bands. 
 +  * Q3: are the bandwidths assumed reasonable?
 +    * Yes. Currently assuming 25% bandwidth
 +  * Q4: what should we assume about beam sizes as a function of frequency, specifically for the high frequency bands? Is it reasonable to assume single mode coupling all the way to the highest frequencies?
 +    * Yes. Single mode all the way to 900 GHz. “Technologies are there.”
 +
 +  * Roger points out that power consumption is poised to be an issue. He is looking to have a discussion with Matt. Charles (and Shaul) advocate assuming custom-made ASICs for which the power consumption could be significantly lower. How much lower? Need to check
 +  * Roger says that with current technologies he projects 400 and 1.1 kW for 10,000 detectors for the TDM, FDM, respectively. 
 +  * Jamie says that for EPIC-IM a JPL engineer found ways to reduce the power consumption of the TDM by a factor of 3(?) even without ASICs.
 + 
  
  
-Focal Plane Technology: 
  
-Roger and Jeff post their answers to the questions from last week on last week’s minutes page.  
-Below is a copy of the questions and some discussions people had today. 
  
-Q1: what is the plan for detector technology for the high frequency bands of the imager? 
-- > 600GHz for Galactic Science; conservative choice is SPT-type polarization-sensitive absorber 
-- Power consumption of read out is quite a large impactor considering the cost 
-- Different read out systems are discussed, e.g. TDM, FDM and ASICS 
-- 400 W or 1.1KW is probably too large 
-- ASICS has a factor of 10 cost saving in power 
  
-Q2: are the distribution of colors for pixels as described by the worksheet reasonable? 
-- 2-3 colors per pixel 
-- maybe fit more bands in lower frequency 
-- high frequency depends on f#, pixel size etc. 
  
-Q3: are the bandwidths assumed reasonable? 
-- 25% is reasonable 
  
-Q4: what should we assume about beam sizes as a function of frequency, specifically for the high frequency bands? Is it reasonable to assume single mode coupling all the way to the highest frequencies? 
-- “Technologies are there.” 
imagerteleconnotes20170807.1502723881.txt.gz · Last modified: 2017/08/14 10:18 by hanany