IOC-MIPS_345a |
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10470C |
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Title: |
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Optimum Operating Temperature for the MIPS 24um Array |
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Objective: |
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Determine what temperature yields the best overall performance of the 24um array. |
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Description: |
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Dark current, responsivity, and latent image behavior need to be characterized as a function |
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including flow / state diagram |
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of detector operating temperature. |
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At each of five detector temperature settings (use same set as in thermal-vac): |
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Take 25 30-second exposures with the scan mirror in the dark position. |
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Using the 10 second exposures, measure a moderately bright star using a 4x4 dither pattern. |
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Move the scan mirror to place the 160um array into the dark. |
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Take 25 10-second exposures with the 160um array to check for scattered emission |
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from the 24um array. |
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Place in Schedule: |
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After aperture door is opened. |
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(relative to water shed events) |
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Required Conditions: |
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Basic MIPS operation must be confirmed including detector and electronics aliveness tests. |
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MIPS 24um aperture must have been located. |
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Background must be less than 2e-8 W/cm^2/sr |
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or T<6.5K |
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Resources: |
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duration (best estimate) |
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1.5 hr |
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real time downlink (Y / N) |
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no |
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special post event actions (Y / N) |
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no |
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Generates 330 DCEs. |
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Outcome: |
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description |
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Best temperature setting for the 24um array will be known. |
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can proceed in parallel with other activity |
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No, requires some dedicated pointing. |
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must outcome be confirmed before next event / test /activity |
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No |
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method of confirmation (sensor TLM, data analysis, etc.) |
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data analysis |
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estimate of data turn around if required for confirmation |
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N/A |
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Unique or included in planned AOT? |
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Will use dark current IER, photometry AOT |
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Contingency Plan: |
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"What if..." |
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IOC Critical |
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Y |
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References: |
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Template last updated: |
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7-Sep-99 |
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M. Rieke |
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