Image Assessment San Diego, November 2005

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Image Assessment San Diego, November 005 Pawel A. Penczek The University of Texas Houston Medical School Department of Biochemistry and Molecular Biology 6431 Fannin, MSB6.18, Houston, TX 77030, USA phone: (713) 500-5416 fax: (713) 500-065 Pawel.A.Penczek@uth.tmc.edu

Correlation coefficient definition and properties (Pearson s r) rxy = ( x x )( y y ) σ xσ y σ = (x x x 1 rxy = N σ x xy m m x σ xσ y x = mx = ) N x N mx xy x y = σ xσ y = x x y -1 rxy 1

Correlation coefficient in image assessment 1 rxy = N xy m m x y σ xσ y y x

Correlation coefficient in image assessment 1 rxy = N xy m m x y σ xσ y y r=0.99 x

Correlation coefficient in image assessment 1 rxy = N xy m m x y σ xσ y y r=-0.99 x

Correlation coefficient in image assessment 1 rxy = N xy m m x y σ xσ y y r=0.11 x

Correlation coefficient in image assessment r - proportion of the variance accounted for by the linear model r 1.00 r perfect linear relation 1.00 0.71 0.50 0.50 0.5 0.33 0.10 0.00 no linear relation 0.00-1.0 inverted contrast 1.00

Correlation coefficient statistical significance r is calculated from a sample of n pairs of numbers Fisher (191): 1 1+ r 1 1+ ρ 1 z = log N ζ = log, n 3 1 r 1 ρ Type I error: error rejection of the null hypothesis when is true. The risk of Type I error is α, the significance level. H0 : r = 0. Example: I calculated r = 0.15 with n = 00. I can reject the null hypothesis on a 5% (0.14) significance level, but not on a 1% (0.18) significance level. I can expect (tolerate) to be wrong 5 out of 100 times.

Correlation coefficient confidence interval r z= is calculated from a sample of n pairs of numbers 1 1+ r 1 1+ ρ ρ 1 log N ζ = log +, n 3 1 r 1 ρ n Confidence intervals of z at 100(1-α)% are z + qα r 1 n 3 for α = 0.05, qα = 1.96, so the confidence limits are z + 1.96 n 3 Confidence intervals of r : transform back using e z 1 r = z e +1

Correlation coefficient confidence interval r is calculated from a sample of n pairs of numbers If ρ=0, r has approximately normal distribution 1 N 0, n Confidence limits : + qα 1 n r

Correlation coefficient confidence interval z + qα (1) 68% of observations fall within σ of µ. () 95% of observations fall within σ of µ. (3) 99.7% of observations fall within 3 σ of µ. 1 n 3 Physicists standard deviation σ Statisticians significance level α 1.04 30% 1.96 5% 3.00.6% 3.09 % 3.9 1% 5.00 0.00006%

Signal-to-Noise Ratio (SNR) SNR = Power of signal Power of noise = Variance of signal Variance of noise means of signal and noise are both zero

Correlation coefficient relation to Signal-to-Noise Ratio in the image r xk = S k + N k N k, M k N ( 0, σ ), rxy N k, Nl xy = ( x ) ( y ) rxy 1 S k S + σ k = 1 k l xk = Sk + M k = 0, N k, M l = 0, S k S k σ S k σ N k, Sl = 0, +1 = SNR SNR + 1 k = 0,

Correlation coefficient relation to Signal-to-Noise Ratio in the image r SNR ρ= SNR + 1 ρ SNR = 1 ρ

Correlation coefficient properties Correlation coefficient is a measure of linear relationship between two variables The values of the correlation coefficient are between -1 and 1 Correlation coefficient is invariant with respect to linear transformations of the data The value of the squared correlation coefficient corresponds to the proportion of the variance accounted for by the linear model For ρ=0, the distribution of the correlation coefficient is approximately normal with σ=1/sqr(n) Using Fisher s transformation it is possible to calculate confidence intervals for any r Using correlation coefficient it is possible to calculate SNR in images

Fourier Shell Correlation WHAT DOES IT HAVE TO DO WITH RESOLUTION?!?

Optical resolution The resolution of a microscope objective is defined as the smallest distance between two points on a specimen that can still be distinguished as two separate entities. Resolution is a somewhat subjective concept. The theoretical limit of the resolution is set by the wavelength of the light source: R = const λ

Optical resolution Hypothetical Airy disk (a) consists of a diffraction pattern containing a central maximum (typically termed a zero th order maximum) surrounded by concentric 1st, nd, 3rd, etc., order maxima of sequentially decreasing brightness that make up the intensity distribution. If the separation between the two disks exceeds their radii (b), they are resolvable. The limit at which two Airy disks can be resolved into separate entities is often called the Rayleigh criterion. When the center-to-center distance between the zero th order maxima is less than the width of these maxima, the two disks are not individually resolvable by the Rayleigh criterion (c).

Resolution-limiting factors in electron microscopy The wavelength of the electrons (depends on the voltage: 100kV - 0.037 Å; 300kV 0.00Å) The quality of the electron optics (astigmatism, envelope functions) The underfocus setting. The resolution of the TEM is often defined as the first zero in the contrast transfer function (PCTF) at Scherzer (or optimum) defocus. Signal-to-Noise Ratio (SNR) level in the data Accuracy of the alignment

The concept of optical resolution is not applicable to electron microscopy and single particle reconstruction In single particle reconstruction, there is no external standard by which the resolution of the results could be evaluated. Resolution measures in EM have to estimate internal consistency of the results. Unless an external standard is provided, objective estimation of the resolution in EM is not possible.

FRC - Fourier Ring Correlation Saxton W.O. and W. Baumeister. The correlation averaging of a regularly arranged bacterial cell envelope protein. J. Microsc., 17, 17-138 (198). FSC Fourier Shell Correlation (3-D) DPR Differential Phase Residual Frank J., A. Verschoor, M. Boublik. Computer averaging of electron micrographs of 40S ribosomal subunits. Science, 14, 1353-1355 (1981). -D & 3-D SSNR Spectral Signal-to-Noise Ratio Unser M., L.B. Trus, A.C. Steven. A new resolution criterion based on spectral signal-to-noise ratios. Ultramicroscopy, 3, 39-5 (1987). Penczek, P. A. Three-dimensional Spectral Signal-to-Noise Ratio for a class of reconstruction algorithms. J. Struct. Biol., 138, 34-46 (00) Q-factor van Heel M. and J. Hollenberg. The stretching of distorted images of two-dimensional crystals. In: Proceedings in Life Science: Electron Microscopy at Molecular Dimensions (Ed.: W. Baumeister). Springer Verlag, Berlin (1980). only -D

Fourier Ring Correlation FSC ( R) = * F G n n n R Fn Gn n R n R 1 A. either: 1. Split (randomly) the data set of available images into halves;. Perform the alignment of each data set independently ; B. or: 1. Perform the alignment of the whole data set;. Split (randomly) the aligned data set into halves; 3. Calculate two averages (3-D reconstructions); 4. Compare the averages in Fourier space by calculating the FRC. WARNINGS - method B valid only if the noise component in the data is independent (not aligned) - the two sets in method A might not be as independent as one assumes.

Fourier Shell Correlation FSC Second set of images G First set of images F F G s R FSC FSC ( R) = FnGn 1.0 * n R Fn Gn n R n R 1 0.5 0.0 s resolution

Fourier Shell Correlation WHY DOES IT WORK? FSC provides a measure of the Spectral Signal-to-Noise Ratio in the reconstruction. FSC is directly related to alignment errors.

Impact of alignment errors on FRC curves σt=0. σt=0.4 σr=8 degrees σr=4 degrees σr=0 σt=0 Baldwin, P.R. and Penczek P.A.: Estimating alignment errors in sets of -D images. JSB 150 11, 005.

Spectral Signal-to-Noise Ratio (SSNR) in D A set of Fourier transforms of D images. R K elements in each Fourier pixel Calculate SSNR according to the equation: SSNR ( R ) = SSNR(R) Fn,k n R k K Fn,k F K 1 n R k 1 where F n = Fn,k K k 1 n 1.0 0 10 0 30 R

Relations between FSC and SSNR FSC SSNR = 1 FSC SSNR FSC = SSNR + 1 For large number of images Variance(SSNR) Variance(FSC) When FSC is calculated for a data set split into halves: FSC SSNR = 1 FSC FSC is a biased estimate of SSNR. For large number of images, the bias is negligible.

Resolution criteria should be based on the SNR considerations FSC SSNR = 1 FSC Reasonable criterion: include only Fourier information that is above the noise level, i.e., SSNR>1. SSNR=1 => FSC=1/3=0.333 Another criterion: (3σ) include Fourier information that is significantly higher than zero, i.e., SSNR>0. SSNR=0 => FSC=0 FSC 3D SNR

FSC can be used to cross-validate EM results EM structure (crossresolution) X-ray crystallographic structure FSC electron density map, the voxel values are proportional to the Coulomb potentials of atoms

Cross-resolution relation between FRC and SSNR EM map G (corrupted by noise and other errors) X-ray map F (noise-free) F G s FSC ( R ) = FnGn R * n R F G n n n R n R 1 Cross-resolution 1.0 0.71 FSC SSNR = 1 FSC SSNR = 1 FSC = 0.0 s 1 = 0.71

0.33 Resolution versus cross-resolution 0.71

FSC z ( FSC ) + 0+ 3 n 3 3 n Radius = 100 voxels normalized spatial frequency

0+ FSC 3 n z ( FSC ) + 0.14 0.16 0.3 0.5 3 n 3 normalized spatial frequency

Resolution curve and optimum filtration FSC SSNR = 1 FSC FSC 3D SNR Wiener filter: SSNR G= F SSNR + 1 FSC G= F FSC + 1 The FSC curve should be used for optimum filtration. Thus, the resolution is given by the overall shape of the FSC, not by a single number.

FSC known problems 1. Number of independent voxels in Fourier space n Interpolation, scanning (image processing) Masking in real space (=convolution in F.space) Dependence on the box size Reduction of n due to symmetry (not included in the code) a. Oversample (pixel size 0.35 of that corresponding to expected resolution) b. Do not mask (particularly complicated shapes) c. Adjust box size d. Use higher cut-off (0.5). Overabundand projections or gaps in angular coverage Elon g at i on FSC curve impressive, but the structure visibly distorted (elongation, streaks) Use 3D SSNR to check the anisortopy of resolution 3. Alignment of noise a. Split dataset into halves and align independently b. Use matched filters 4. Not applicable when the number of projections is small (tomography!) dire c tion

Examples of resolution curves FSC 1.0 Healthy: 0.5 0.0 resolution f In low frequencies remains one, followed by a semigaussian fall-off, drops to zero at around /3 of maximum frequency, in high frequencies oscillates around zero.

Examples of resolution curves FSC 1.0 Unhealthy: 0.5 0.0 resolution f Rectangular : in low frequencies remains one, followed by a sharp drop, in high frequencies oscillates around zero. A combination of alignment of the noise and a sharp filtration during the alignment procedure. The result is fake.

Examples of resolution curves FSC 1.0 Unhealthy: 0.5 0.0 Resolution? f FSC never drops to zero in the whole frequency range. The noise component in the data was aligned. Non-linear operations applied (masking, thresholding). The result is fake. In rare cases it could mean that the data was severely undersampled (very large pixel size).

Examples of resolution curves FSC 1.0 Unhealthy: 0.5 0.0 resolution f After it drops to zero, increases in high frequencies oscillation. Data was low-passed filtered; errors in image processing code, mainly in interpolation; all images were rotated by the same angle.

Examples of resolution curves FSC 1.0 Unhealthy: 0.5 0.0 Resolution? f FSC oscillates around 0.5. The data is dominated by one subset with the same defocus value or there is only one defocus group. It is not incorrect per se, but unclear what is the resolution. Also, will result in artifacts.

Summary The concept of optical resolution is not applicable to electron microscopy and single particle reconstruction. Resolution measures in EM estimate the internal consistency of the results. The outcome is prone to errors. The existing resolution measures cannot distinguish between true signal and the aligned (correlated) noise component in the data. FSC and SSNR are mathematically largely equivalent, although the SSNR-based estimate of the spectral signal to noise ratio has lower statistical uncertainty than the FSC-based estimate. A reasonable resolution criterion should be based on the SSNR in the data and set such that the Fourier coefficients that are dominate by noise are excluded from the final analysis. For example, SSNR=1 => FSC=0.333. Confidence interval for FSC curves can be given if he number of independent voxels in the reconstruction could be known. The shape of the FSC curve defines an optimum filter for the average/reconstruction.