The Solar Mass Ejection Imager (Smei)

By C. Eyles, G. Simnett, M. Cooke, B. Jackson, A. Buffington, P. Hick, N. Waltham, J. King, P. Anderson, P. E. Holladay. 2003

182 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/49e8a3118fcf8afdc8a3d6bb3ae82198eb1e6082

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In Aerospace Engineering

1. M. Temmer

In Astronomy and Astrophysics

1. M. Temmer
2. Nat Gopalswamy
3. B. Vršnak
4. N. Lugaz
5. T. Howard
6. Yuming Wang
7. C. Farrugia
8. R. Howard

Citations in the corpus

• Up to 1‐hour forecasting of radiation hazards from solar energetic ion events with relativistic electrons (2007, methodology): “Similarly, observations of comet tails with the Solar Mass Ejection Imager (SMEI) [Keil et al., 1996] have shown deflections of the same order of magnitude [Kuchar et al.”
• Kinematics of coronal mass ejections between 2 and 30 solar radii. What can be learned about forces governing the eruption (2004, methodology): “In such cases, the Thompson scattering measurements by the Solar Mass Ejection Imager (SMEI) combined with IPS observations (Jackson et al. 2003; Eyles et al. 2003) could be essential for the understanding of the IP propagation of CMEs and a successful prediction of 1 au transit time.”
• The Interaction of Successive Coronal Mass Ejections: A Review (2016, methodology): “The development of heliospheric imaging with the Solar Mass Ejection Imager (SMEI: Eyles et al., 2003, Jackson et al., 2004) and the HIs onboard STEREO have led to a large increase in the number of published cases of CMECME interaction being remotely observed.”
• The Heliospheric Imagers Onboard the STEREO Mission (2009, methodology): “The heritage for the HI instrument comes from the SMEI instrument (Eyles et al., 2003; Jackson et al., 2004), operating aboard the Coriolis spacecraft, launched in 2003.”
• Interplanetary Coronal Mass Ejections Observed in the Heliosphere: 1. Review of Theory (2009, background): “The Solar Mass Ejection Imager (SMEI, Eyles et al. 2003; Jackson et al. 2004) has been observing since February 2003, has identified and tracked over 300 ICMEs during its 6 year lifetime (e.g., Tappin et al. 2004; Howard et al. 2006; Webb et al. 2006) and continues to do so at the time of writing.”