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. Author manuscript; available in PMC: 2010 Mar 17.
Published in final edited form as: J Opt Soc Am A Opt Image Sci Vis. 2008 Aug;25(8):1866–1874. doi: 10.1364/josaa.25.001866

Table 1. Results of Determining Size of Spheroidal Scatterers by Fitting Scattering Distribution to Mie Theorya.

Equator Polar Both Accuracy
Configuration TE, S11 23 35 13 71
TM, S11 46 17 18 79
TM, S22 12 42 19 74
TE, S22 67 1.0 23 91
random, S11 37 22 18 77
randomS22 52 13 24 89

Summary statistics Cell 41 18 18 76
Phantom 39 25 20 84
S11 36 24 14 75
S22 44 19 21 83
TE 18 39 16 72
Random 45 18 21 83
TM 57 9.0 19 85
a

Data are in percent. The average number of fits to each manifold was assessed for each configuration or summary statistic, where each manifold has a width of 2λ/nS. The final column is a measure of success for the hypothesis; namely, that the size determination is within one wavelength of one of the dimensions of the spheroidal scatterer. Data in boldface correspond to configurations or summary statistics with a normalized root mean square error (NRMSE) less than 0.1; data in lightface correspond to an NRMSE between 0.1 and 0.13. The average null NRMSE is 0.40 and always greater than 0.38. For all configurations and summary statistics, the difference between the NRMSE and the null NRMSE is statistically significant (p<10−3).