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FMRI GLM Analysis 7/15/2014Tuesday Yingying Wang

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Presentation on theme: "FMRI GLM Analysis 7/15/2014Tuesday Yingying Wang"— Presentation transcript:

1 FMRI GLM Analysis 7/15/2014Tuesday Yingying Wang http://neurobrain.net/2014STBCH/index.html

2 Realignment Smoothing Normalization General linear model Statistical parametric map (SPM) Image time-series Parameter estimates Design matrix Template Kernel Random field theory p <0.05 Statisticalinference GLM 2

3 Parametric statistics one sample t-test two sample t-test paired t-test Anova AnCova correlation linear regression multiple regression F-tests etc… all cases of the General Linear Model 3

4 The General Linear Model (GLM) T-tests, correlations and Fourier analysis work for simple designs and were common in the early days of imaging. The General Linear Model (GLM) is now available in many software packages and tends to be the analysis of choice. Why is the GLM so great? the GLM is an overarching tool that can do anything that the simpler tests do you can examine any combination of contrasts (e.g., intact - scrambled, scrambled - baseline) with one GLM rather than multiple correlations the GLM allows much greater flexibility for combining data within subjects and between subjects 4

5 The General Linear Model (GLM) it also makes it much easier to counterbalance orders and discard bad sections of data the GLM allows you to model things that may account for variability in the data even though they aren’t interesting in and of themselves (e.g., head motion) as we will see later in the course, the GLM also allows you to use more complex designs (e.g., factorial designs) 5

6 A mass-univariate approach Time 6

7 7

8 General Linear Model Equation for single voxel j: y j = x j1  1 + … x jL  L +  j  j ~ N(0,  2 ) y j : data for scan, j = 1…J x jl : explanatory variables / covariates / regressors, l = 1…L  l : parameters / regression slopes / fixed effects  j : residual errors, independent & identically distributed (“iid”) (Gaussian, mean of zero and standard deviation of σ) Equivalent matrix form: y = X  +  X : “design matrix” / model 8

9 GLM 9

10 The Design Matrix 10

11 Estimation of the parameters i.i.d. assumptions: OLS estimates: 11

12 OLS (Ordinary Least Squares) This is a scalar and the transpose of a scalar is a scalar The goal is to minimize the quadratic error between data and model 12 You find the extremum (max or min) of a function by taking its derivative and setting it to zero

13 13

14 What are the problems? 1.BOLD responses have a delayed and dispersed form. 2.The BOLD signal includes substantial amounts of low- frequency noise. 3.The data are serially correlated (temporally auto correlated)  this violates the assumptions of the noise model in the GLM Design Error 14

15 The response of a linear time-invariant (LTI) system is the convolution of the input with the system's response to an impulse (delta function). Problem 1: Shape of BOLD response 15

16 Solution: Convolution model of the BOLD response expected BOLD response = input function  impulse response function (HRF)  HRF blue = data green = predicted response, taking convolved with HRF red = predicted response, NOT taking into account the HRF 16

17 Problem 2: Low frequency noise blue = data black = mean + low-frequency drift green = predicted response, taking into account low-frequency drift red = predicted response, NOT taking into account low-frequency drift Linear model 17

18 discrete cosine transform (DCT) set Solution 2: High pass filtering 18

19 Problem 3: Serial correlations non-identity non-independence t1 t2 t1 t2 i.i.d n: number of scans n n 19

20 Problem 3: Serial correlations n n auto covariance function with 1 st order autoregressive process: AR(1) n: number of scans 20

21 Solution 3: Pre-whitening 1. Use an enhanced noise model with multiple error covariance components, i.e. e ~ N(0,  2 V) instead of e ~ N(0,  2 I). 2. Use estimated serial correlation to specify filter matrix W for whitening the data. This is i.i.d 21

22 How do we define W ? Enhanced noise model Remember linear transform for Gaussians Choose W such that error covariance becomes spherical Conclusion: W is a simple function of V  so how do we estimate V ? 22

23 Linear Model effects estimate error estimate statistic  GLM includes all known experimental effects and confounds Convolution with a canonical HRF High-pass filtering to account for low-frequency drifts Estimation of multiple variance components (e.g. to account for serial correlations) 23

24 Contrasts in the GLM 24 We can examine whether a single predictor is significant (compared to the baseline) We can also examine whether a single predictor is significantly greater than another predictor

25 Implementation of GLM in SPM 25

26 Contrasts [1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0] [1 0 0 -1 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0] 26

27 Hypothesis Testing - Introduction Is the mean of a measurement different from zero? Mean of several measurements Many experiments Ratio of effect vs. noise  t-statistic Null Distribution of T Null distribution What distribution of T would we get for  = 0? 0     Exp A     Exp B 27

28 Hypothesis Testing  Null Hypothesis H 0 Typically what we want to disprove (no effect).  The Alternative Hypothesis H A expresses outcome of interest. To test an hypothesis, we construct “test statistics”.  Test Statistic T The test statistic summarises evidence about H 0. Typically, test statistic is small in magnitude when the hypothesis H 0 is true and large when false.  We need to know the distribution of T under the null hypothesis. Null Distribution of T 28

29 Hypothesis Testing  p-value: A p-value summarises evidence against H 0. This is the chance of observing a value more extreme than t under the null hypothesis. Null Distribution of T  Significance level α : Acceptable false positive rate α.  threshold u α Threshold u α controls the false positive rate t p-value Null Distribution of T  uu  Conclusion about the hypothesis: We reject the null hypothesis in favour of the alternative hypothesis if t > u α t 29

30 c T = 1 0 0 0 0 0 0 0 T = contrast of estimated parameters variance estimate effect of interest > 0 ? = amplitude > 0 ? =  1 = c T  > 0 ?  1  2  3  4  5... T-test - one dimensional contrasts – SPM{t} Question: Null hypothesis: H 0 : c T  =0 Test statistic: 30

31 T-contrast in SPM con_???? image ResMS image spmT_???? image SPM{t}  For a given contrast c: beta_???? images 31

32 T-test: a simple example Q: activation during listening ? Null hypothesis:  1 = 0  Passive word listening versus rest SPMresults: Threshold T = 3.2057 {p<0.001} voxel-level p uncorrected T ( Z  ) Mm mm mm 13.94 Inf0.000-63 -27 15 12.04 Inf0.000-48 -33 12 11.82 Inf0.000-66 -21 6 13.72 Inf0.000 57 -21 12 12.29 Inf0.000 63 -12 -3 9.89 7.830.000 57 -39 6 7.39 6.360.000 36 -30 -15 6.84 5.990.000 51 0 48 6.36 5.650.000-63 -54 -3 32

33 T-test: summary T-test is a signal-to-noise measure (ratio of estimate to standard deviation of estimate).  T-contrasts are simple combinations of the betas; the T- statistic does not depend on the scaling of the regressors or the scaling of the contrast. H0:H0:vs H A :  Alternative hypothesis: 33

34 Scaling issue The T-statistic does not depend on the scaling of the regressors. [1 1 1 1 ]  Be careful of the interpretation of the contrasts themselves (eg, for a second level analysis): sum ≠ average  The T-statistic does not depend on the scaling of the contrast. / 4 Subject 1 [1 1 1 ] Subject 5  Contrast depends on scaling. / 3 34

35 F-test - the extra-sum-of-squares principle Model comparison: Full model ? X1X1 X0X0 or Reduced model? X0X0 Test statistic: ratio of explained variability and unexplained variability (error) 1 = rank(X) – rank(X 0 ) 2 = N – rank(X) RSS RSS 0 Null Hypothesis H0: True model is X0 (reduced model) 35

36 F-test - multidimensional contrasts – SPM{F} Test multiple linear hypotheses: Full model ? Null Hypothesis H0:  3 =  4 =  5 =  6 =  7 =  8 = 0 X 1 (  3-8 ) X0X0 0 0 1 0 0 0 0 0 0 0 0 1 0 0 0 0 0 0 0 0 1 0 0 0 0 0 0 0 0 1 0 0 0 0 0 0 0 0 1 0 0 0 0 0 0 0 0 1 c T = c T  = 0 Is any of  3-8 not equal 0? 36

37 F-contrast in SPM ResMS image spmF_???? images SPM{F} ess_???? images ( RSS 0 - RSS ) beta_???? images 37

38 F-test example: movement related effects Design matrix 2468 10 20 30 40 50 60 70 80 contrast(s) Design matrix 2468 10 20 30 40 50 60 70 80 contrast(s) 38

39 F-test: summary. F-tests can be viewed as testing for the additional variance explained by a larger model wrt a simpler (nested) model  model comparison.  In testing uni-dimensional contrast with an F-test, for example  1 –  2, the result will be the same as testing  2 –  1. It will be exactly the square of the t-test, testing for both positive and negative effects.  F tests a weighted sum of squares of one or several combinations of the regression coefficients .  In practice, we don’t have to explicitly separate X into [X 1 X 2 ] thanks to multidimensional contrasts.  Hypotheses: 39

40 Orthogonal regressors Variability in Y 40

41 Correlated regressors Shared variance Variability in Y 41

42 Correlated regressors Variability in Y 42

43 Correlated regressors Variability in Y 43

44 Correlated regressors Variability in Y 44

45 Correlated regressors Variability in Y 45

46 Correlated regressors Variability in Y 46

47 Correlated regressors Variability in Y 47

48 Design orthogonality For each pair of columns of the design matrix, the orthogonality matrix depicts the magnitude of the cosine of the angle between them, with the range 0 to 1 mapped from white to black.  If both vectors have zero mean then the cosine of the angle between the vectors is the same as the correlation between the two variates. 48

49 Correlated regressors: summary We implicitly test for an additional effect only. When testing for the first regressor, we are effectively removing the part of the signal that can be accounted for by the second regressor:  implicit orthogonalisation. Orthogonalisation = decorrelation. Parameters and test on the non modified regressor change. Rarely solves the problem as it requires assumptions about which regressor to uniquely attribute the common variance.  change regressors (i.e. design) instead, e.g. factorial designs.  use F-tests to assess overall significance. Original regressors may not matter: it’s the contrast you are testing which should be as decorrelated as possible from the rest of the design matrix x1x1 x2x2 x1x1 x2x2 x1x1 x2x2 xx xx 2 1 2 x  = x 2 – x 1.x 2 x 1 49

50 Design efficiency  The aim is to minimize the standard error of a t-contrast (i.e. the denominator of a t-statistic).  This is equivalent to maximizing the efficiency e: Noise variance Design variance  If we assume that the noise variance is independent of the specific design:  This is a relative measure: all we can really say is that one design is more efficient than another (for a given contrast). 50

51 Design efficiency AB A+B A-B  High correlation between regressors leads to low sensitivity to each regressor alone.  We can still estimate efficiently the difference between them. 51

52 Types of error Reality H1H1 H0H0 H0H0 H1H1 True negative (TN) True positive (TP) False positive (FP)  False negative (FN) specificity: 1- = TN / (TN + FP) = proportion of actual negatives which are correctly identified sensitivity (power): 1- = TP / (TP + FN) = proportion of actual positives which are correctly identified Decision 52

53 Correction for Multiple Comparisons With conventional probability levels (e.g., p <.05) and a huge number of comparisons (e.g., 64 x 64 x 12 = 49,152), a lot of voxels will be significant purely by chance e.g.,.05 * 49,152 = 2458 voxels significant due to chance How can we avoid this?  need to do correction for multiple comparisons 53

54 (1) Bonferroni correction Divide desired p value by number of comparisons Example: desired p value: p <.05 number of voxels: 50,000 required p value: p <.05 / 50,000  p <.000001 quite conservative can use less stringent values e.g., Brain Voyager can use the number of voxels in the cortical surface the luxury of a localizer task is that it allows you to correct for only those voxels you are interested in (i.e., the voxels that fall within your ROI) 54 Source: Jody Culham’s web slidesweb slides

55 (2) Cluster correction falsely activated voxels should be randomly dispersed set minimum cluster size to be large enough to make it unlikely that a cluster of that size would occur by chance assumes that data from adjacent voxels are uncorrelated (not true) 55

56 (3) Test-retest reliability Perform statistical tests on each half of the data The probability of a given voxel appearing in both purely by chance is the square of the p value used in each half e.g.,.001 x.001 =.000001 Alternatively, use the first half to select an ROI and evaluate your hypothesis in the second half. 56

57 (4) Consistency between subjects Though seldom discussed, consistency between subjects provides further encouragement that activation is not spurious. Present group and individual data. 57 (5) Screen saver scan You can test how many voxels really do light up when really nothing is happening.

58 ROI VoxelField FWE FDR * voxels/volume Height Extent ROI VoxelField Height Extent There is a multiple testing problem (‘voxel’ or ‘blob’ perspective). More corrections needed as.. Detect an effect of unknown extent & location 58

59 Book – must read 59 Statistical Parametric Mapping: The Analysis of Functional Brain Images. Elsevier, 2007.

60 Home Work http://www.fil.ion.ucl.ac.uk/spm/data/auditory/ http://www.fil.ion.ucl.ac.uk/spm/doc/spm8_man ual.pdf#Chap:data:auditoryhttp://www.fil.ion.ucl.ac.uk/spm/doc/spm8_man ual.pdf#Chap:data:auditory Walk through SPM manual chapter 28 Sample data can be found in the general folder If you have any question, ask me or Danielle. Bonus for those who finish the homework by next training session. 60


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