A synoptic view of solar transient evolution in the inner heliosphere using the Heliospheric Imagers on STEREO

Geophysical Research Letters

Volumn 36, Issue 2, 2009, Pages

  Davies, J A ^a   Harrison, R A ^a   Rouillard, A P ^a,b   Sheeley Jr , N R ^c   Perry, C H ^a   Bewsher, D ^a   Davis, C J ^a   Eyles, C J ^a,d   Crothers, S R ^a   Brown, D S ^e  

^a RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^b UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^c NAVAL RESEARCH LABORATORY   (United States)

^d UNIVERSITY OF VALENCIA   (Spain)

^e ABERYSTWYTH UNIVERSITY   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

ELECTRIC FIELD EFFECTS; IMAGE SENSORS;

CORONAL MASS EJECTIONS; HELIOSPHERE; IMAGERS; TRANSIENT EVOLUTIONS; WELL-ESTABLISHED TECHNIQUES;

SOLAR ENERGY;

CORONA; CORONAL MASS EJECTION; SOLAR ACTIVITY;

EID: 62749145030     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2008GL036182     Document Type: Article

References (14)

1. Brown, D. S., D. Bewsher, and C. J. Eyles (2009), Calibrating the pointing and optical parameters of the STEREO heliospheric imagers, Sol. Phys., 254, 185.
2. Brueckner, G. E., et al. (1995), The Large Angle Spectroscopic Coronagraph (LASCO), Sol. Phys., 162, 357.
3. Eyles, C. J., et al. (2003), The Solar Mass Ejection Imager (SMEI), Sol. Phys., 21, 19.
4. Eyles, C. J., et al. (2009), The heliospheric imagers on-board the STEREO mission, Sol. Phys., in press.
5. Howard, R. A., et al. (2008), Sun Earth Connection Coronal and Heliospheric Investigations (SECCHI), Space Sc. Rev., 136, 67.
6. Kahler, S. W., and D. F. Webb (2007), V arc interplanetary coronal mass ejections observed with the Solar Mass Ejection Imager, J. Geophys. Res., 112, A09103, doi:10.1029/2007JA012358.
7. Rouillard, A. P., et al. (2008), First imaging of corotating interaction regions using the STEREO spacecraft, Geophys. Res. Lett., 35, L10110, doi:10.1029/2008GL033767.
8. Simnett, G. M., et al. (1997), LASCO observations of disconnected magnetic structures out to and beyond 28 solar radii during coronal mass ejections, Sol. Phys., 175, 685.
9. Sheeley, N. R., et al. (1997), Measurements of flow speeds in the corona between 2 and 30 solar radii, Astrophys. J., 484, 472.
10. Sheeley, N. R., J. H. Walters, Y.-M. Wang, and R. A. Howard (1999), Continuous tracking of coronal outflows: Two kinds of coronal mass ejection, J. Geophys. Res., 104, 24, 739.
11. Sheeley, N. R., et al. (2008a), SECCHI observations of the Suns gardenhose density spiral, Astrophys. J., 674, 109.
12. Sheeley, N. R., et al. (2008b), Heliospheric images of the solar wind at Earth, Astrophys. J., 675, 853.
13. Vourlidas, A., and R. A. Howard (2006), The proper treatment of coronal mass ejection brightness: A new methodology and implications and observations, Astrophys. J., 642, 1216.
14. Wang, Y.-M., and N. R. Sheeley Jr. (2006), Observations of flux rope formation in the outer corona, Astrophys. J., 650, 1172.