1. Reames, Ng, Tylka 2012 Sol Phys Multi-spacecraft observation

2. Reames, Ng, Tylka 2012 Sol Phys Multi-spacecraft observation

3. CME/SEP Connection Plasma flow in a CME controls where and when the field lines connect to the shock and hence the observed SEP intensity variation. Such multi-spacecraft observation will be made by Solar Probe Plus and Solar Orbiter near the Sun with far greater precision and with concurrent CME observation.

4. 2011 Mar 21 Intensity time profiles at STEREO A Ng et al. 2012 In prep.Rouillard et al. 2012 May, ApJ

5. CME Observation Rouillard et al. 2012 May, ApJ

6. The shock expansion accounts for the times of SEP injections and the injection delay between the field lines leading to L1 and STEREO A. Rouillard et al. 2012 May, ApJ

7. L1 and STEREO A pre-shock proton energy spectrum Ng et al. 2012 In prep.Rouillard et al. 2012 May, ApJ

8. Model SEP release time profiles at shock