The Solar Mass-Ejection Imager (SMEI) Mission
By B. Jackson, A. Buffington, P. Hick, R. Altrock, S. Figueroa, P. E. Holladay, J. Johnston, S. Kahler, J. Mozer, S. Price and 14 more. 2003
168 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/aa2bbdbb6c93682fe0ff6ef6f48959cf8f668687
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In Astronomy and Astrophysics
Citations in the corpus
- Propagation of Interplanetary Coronal Mass Ejections: The Drag-Based Model (2013, background): “, 1995) onboard the Solar and Heliospheric Observatory (SoHO), the Solar Mass Ejection Imager (SMEI; Jackson et al., 2004), and espe-”
- STEREO IMPACT Investigation Goals, Measurements, and Data Products Overview (2008, unknown): “SMEI on Coriolis (Jackson et al. 2004) provides wide-field coronagraph images from an Earth-orbiting Air Force satellite platform, and is ideally suited for STEREO HI comparisons and in situ comparisons.”
- The Physical Processes of CME/ICME Evolution (2017, methodology): “…(e.g., Reiner et al. 2005b,a; Tappin 2006; Webb et al. 2006; Howard et al. 2013) onboard the Solar Mass Ejection Imager (SMEI) (Eyles et al. 2003; Jackson et al. 2004) and STEREO-HI (e.g., Liu et al. 2013, 2016), by tracking interplanetary radio type II bursts (e.g., Reiner et al. 2005a,b; Liu…”
- Massive pulsating stars observed by BRITE-Constellation - I. The triple system β Centauri (Agena) (2016, methodology): “Quite recently, photometry of β Cen was obtained by the SMEI experiment onboard the Coriolis satellite (Jackson et al. 2004) and analysed by Goss (2012).”
- 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.”
- 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.”