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T1  - Coronal Magnetic Structure of Earthbound CMEs and In Situ Comparison 
SN  -  /  
UR  - http://hdl.handle.net/10138/298269 
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A1  - Palmerio, E.; Kilpua, E. K. J.; Möstl, C.; Bothmer, V.; James, A. W.; Green, L. M.; Isavnin, A.; Davies, J. A.; Harrison, R. A. 
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PB  -  
Y1  - 2018 
LA  - eng 
AB  - Predicting the magnetic field within an Earth-directed coronal mass ejection (CME) well before its arrival at Earth is one of the most important issues in space weather research. In this article, we compare the intrinsic flux rope type, that is, the CME orientation and handedness during eruption, with the in situ flux rope type for 20 CME events that have been uniquely linked from Sun to Earth through heliospheric imaging. Our study shows that the intrinsic flux rope type can be estimated for CM... 
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KW  - coronal mass ejections; corona; solar wind; magnetic field; flux ropes; INTERPLANETARY FLUX ROPES; DYNAMICS-OBSERVATORY SDO; MASS EJECTIONS; SOLAR-WIND; ACTIVE-REGION; MAGNETOSPHERIC STORMS; FIELD CONFIGURATIONS; GEOMAGNETIC STORM; STEREO MISSION; CLOUDS; 115 Astronomy, Space science 
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