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• W2073412213 endingPage "L132" @default.
• W2073412213 startingPage "L127" @default.
• W2073412213 abstract "Coronal mass ejections (CMEs) are large-scale ejections of plasma and magnetic field from the solar corona, which propagate through interplanetary space at velocities of ∼100–2500 km s−1. Although plane-of-sky coronagraph measurements have provided some insight into their kinematics near the Sun (<32 R☉), it is still unclear what forces govern their evolution during both their early acceleration and later propagation. Here, we use the dual perspectives of the STEREO spacecraft to derive the three-dimensional kinematics of CMEs over a range of heliocentric distances (∼2–250 R☉). We find evidence for solar wind (SW) drag forces acting in interplanetary space, with a fast CME decelerated and a slow CME accelerated toward typical SW velocities. We also find that the fast CME showed linear (δ = 1) dependence on the velocity difference between the CME and the SW, while the slow CME showed a quadratic (δ = 2) dependence. The differing forms of drag for the two CMEs indicate the forces responsible for their acceleration may be different." @default.
• W2073412213 created "2016-06-24" @default.
• W2073412213 creator A5013085330 @default.
• W2073412213 creator A5027096810 @default.
• W2073412213 date "2010-11-08" @default.
• W2073412213 modified "2023-09-26" @default.
• W2073412213 title "SOLAR WIND DRAG AND THE KINEMATICS OF INTERPLANETARY CORONAL MASS EJECTIONS" @default.
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• W2073412213 doi "https://doi.org/10.1088/2041-8205/724/2/l127" @default.
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