====== Telecon 20171205 ====== Attending: Kris, Tom, Roger, Qi, Karl, Shaul, Brian Notes by : Karl \\ === Agenda=== * New sun shields, new alpha/beta? (JPL, UMN) * {{::extension_shields.pdf|Last Week's Presentation}} * {{::171130_pico_iso-front.jpg?25|New approach}} * Focal plane V3.0 (Karl) * {{::sensitivity_updates_20171205.pdf|V3.0 status}} * Update from JPL === Notes:=== New sun shields, new alpha/beta? (JPL, UMN) * high angle tulip shields. * primary protected. * possible adjustments to alpha 30 or 35 Focal plane V3.0 (Karl) * 40K primary and 0.07% emissivity. * a 10% margin is included in these numbers given to the science team, just so they see less fluctuations. * Shaul: option to increase FP size and number bolos by 2x. Keep this in mind. * Limits currently are data rate, see main imager wiki: posting/datavolume * 15k bolos give 3 Tb/day but DSN for 4 hours is 2 Tb/day * Kris: this is a stiff constraint for 10 yrs in future. Planck saw same type of limits evaporate during their planning. Update from JPL * Roger: Wiring and thermal load w/ Chris Paine. TDM and FDM. * FDM, has few wires to mK. More complicated warm readout. (Shaul: more power, yes. not necessarily more complicated. ) * Power usage 15k bolos -- 375 W for FDM * TDM, fewer wires. simpler warm readout * calculating heat load on mK from heat conduction and detector dissipation. * dissipation < 1 uW. not a problem. * wire count * x64 -- 1850 wires (TDM), with 350 mK buffer stage, few - 50 uW load on mK. * x128 -- 1140 wires, 3-30 uW load. * Next step, starting on FDM. * Peter Day is detector Team X partner. Typically supportive of aggressive stance. * Brian: Joelle's model given to thermal analyst * from him: * Just satellite drifting passively: space craft 260 K, primary 31 K. * Adding heat sources, coolers, etc. to refine numbers. * Shaul: need inputs to Goddard for ADR design. Timeline? * Tom: need this by end of this week. Team X is December 19.