TPF-I SWG Report - Exoplanet Exploration Program - NASA
TPF-I SWG Report - Exoplanet Exploration Program - NASA
TPF-I SWG Report - Exoplanet Exploration Program - NASA
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D ESIGN AND A R C H I T E C T U R E T RADE S TUDIES<br />
Design Teams. This process involved representatives from Ball Aerospace, Lockheed Martin and<br />
Northrop Grumman. Inputs were also solicited from the <strong>TPF</strong>-I Science Working Group. Participants were<br />
asked to weight the discriminators; an average of the responses was taken to determine the initial values,<br />
and the weights were normalized so that the sum of all weights equals 100. The weights represent the<br />
relative importance given to the discriminators and are separate from any consideration of the options.<br />
Wherever possible, a discriminator was quantified using one or more metrics. For example, for the<br />
discriminator “Control system complexity” the metric chosen was the number of control loops needed for<br />
the basic array operation. These metrics helped to inform the scoring process, although scoring is<br />
fundamentally subjective. The scoring of the discriminators for each option was conducted at a 2-day<br />
meeting held at JPL in December 2004, with approximately 20 participants from JPL and the contractors.<br />
For each discriminator the best option was scored a 10, and a simple voting system was used to establish<br />
the scores for the other options. Sometimes the scores bore a linear relationship to the metrics; sometimes<br />
explicitly not. If there was little difference between the options then the scores were close together; large<br />
differences were reflected in a low score for the worst option. The contribution to the final score is given<br />
by the product of the weight and the score, with the weight reflecting the importance of the discriminator<br />
and the score showing the size of the difference between the options. The weighted sum of the scores has<br />
a maximum possible value of 1000 points for each option.<br />
After the initial round of scoring there were multiple rounds of iteration in which both the weights and<br />
scores could be adjusted. This may sound like “gaming the system,” but the intent is not that we turn the<br />
crank on the process and blindly accept the outcome; rather it is that the final table should reflect the<br />
collective engineering judgment of the group. The process is inevitably subjective (particularly the<br />
assigning of weights), but is highly transparent. It structures the analysis, focuses discussion on the key<br />
areas, and invites criticism and comment.<br />
-18 m -9 m +9 m +18 m<br />
Config A 0 ±π/2<br />
π ±3π/2<br />
Nulling baselines:<br />
Imaging baselines:<br />
B null = 27 m<br />
B img = 15 m<br />
Config B 0 π ±π/2 ±3π/2<br />
Nulling baselines:<br />
Imaging baselines:<br />
B null = 9 m<br />
B img = 27 m<br />
Figure 4-24. Schematic showing collector spacing for the Structurally Connected Interferometer. There are two<br />
different ways to phase the interferometer. In Configuration A, the nulling baselines are interleaved. In<br />
Configuration B, the nulling baselines are adjacent.<br />
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