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Table of contents
1. Introduction
1.1. Rosetta
1.2. Comet 67P/Churyumov-Gerasimenko
2. 3D reconstruction
2.1. MPCD technique
2.1.1. Input Model
2.1.2. Image Selection
2.1.3. Optimization
3. Boulder Characterization from optimized DTMs
3.1. Position Estimation
3.2. Dimension Estimation
3.3. Volume Estimation from DEM
4. Dynamic Models
4.1. Light received by local area
4.2. Surface Temperature
4.3. Water production rate
4.4. Non-gravitational acceleration
5. Results
5.1. Scenario 1 – Periodic Bursts
5.1.1. Movement of boulder
5.2. Scenario 2 – Single Outburst
5.2.1. Movement of boulder
5.3. Minimum surface fraction required
5.4. Summary
6. Conclusions
7. Bibliography
