1 INTRODUCTION  
2 INTRINSIC ALIGNMENT MODELING  
2.1 IA Amplitude  
2.2 IA Density Power Spectra Models  
3 MODELING WEAK LENSING OBSERVABLES AND COVARIANCES  
4 SURVEY PARAMETERS  
4.1 Source Galaxy Distribution  
5 RESULTS  
5.1 Simulated Likelihood Analyses  
5.2 LSST Baseline Models  
5.3 Comparison of LSST, DES, Euclid, WFIRST  
5.4 Alternative IA Mitigation Strategies  
6 DISCUSSION AND CONCLUSIONS