Open AccessKinematic properties of solar coronal mass ejections: Correction for projection effects in spacecraft coronagraph measurements
Author(s) -
Howard T. A.,
Nandy D.,
Koepke A. C.
Publication year - 2008
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2007ja012500
Subject(s) - coronagraph , coronal mass ejection , physics , spacecraft , sky , kinematics , acceleration , astrophysics , solar prominence , projection (relational algebra) , magnitude (astronomy) , astronomy , solar wind , planet , plasma , computer science , classical mechanics , exoplanet , quantum mechanics , algorithm , magnetic field
One of the main sources of uncertainty in quantifying the kinematic properties of coronal mass ejections (CMEs) using coronagraphs is the fact that coronagraph images are projected into the sky plane, resulting in measurements which can differ significantly from their actual values. By identifying solar surface source regions of CMEs using X‐ray and H α flare and disappearing filament data, and through considerations of CME trajectories in three‐dimensional (3‐D) geometry, we have devised a methodology to correct for the projection effect. We outline this method here. The methodology was automated and applied to over 10,000 CMEs in the Coordinated Data Analysis Workshop (CDAW) (SOHO Large Angle Spectroscopic Coronagraph) catalog spanning 1996–2005, in which we could associate 1961 CMEs with an appropriate surface event. In the latter subset, deprojected speeds, accelerations, and launch angles were determined to study CME kinematics. Our analysis of this subset of events reconfirms some important trends, notably that previously uncovered solar cycle variation of CME properties are preserved, CMEs with greater width have higher speeds, and slower CMEs tend to accelerate while faster CMEs tend to decelerate. This points out that statistical trends in CME properties, recovered from plane‐of‐sky measurements, may be preserved even in the face of more sophisticated 3‐D measurements from spacecrafts such as STEREO, if CME trajectories are predominantly radial. However, our results also show that the magnitude of corrected measurements can differ significantly from the projected plane‐of‐sky measurements on a case‐by‐case basis and that acceleration is more sensitive to the deprojection process than speed. Average corrected speed and acceleration tend to be a factor of 1.7 and 4.4 higher than their projected values, with mean corrected speed and acceleration magnitudes being on the order of 1000 km/s and 50 m/s 2 , respectively. We conclude that while using the plane‐of‐sky measurements may be suitable for studies of general trends in a large sample of events, correcting for projection effects is mandatory for those investigations which rely on a numerically precise determination of the properties of individual CMEs.