reames, ng, tylka 2012 sol phys multi-spacecraft observation
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Reames, Ng, Tylka 2012 Sol Phys
Multi-spacecraft observation
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Reames, Ng, Tylka 2012 Sol Phys
Multi-spacecraft observation
![Page 3: Reames, Ng, Tylka 2012 Sol Phys Multi-spacecraft observation](https://reader033.vdocuments.net/reader033/viewer/2022061304/5513e2b355034679748b54f8/html5/thumbnails/3.jpg)
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.
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2011 Mar 21 Intensity time profiles at STEREO A 2011 Mar 21 Intensity time profiles at STEREO A Ng et al. 2012 In prep.Rouillard et al. 2012 May, ApJ
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CME ObservationCME Observation
Rouillard et al. 2012 May, ApJ
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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
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L1 and STEREO A pre-shock proton energy spectrumL1 and STEREO A pre-shock proton energy spectrum
Ng et al. 2012 In prep.Rouillard et al. 2012 May, ApJ
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Model SEP release time profiles at shock Model SEP release time profiles at shock