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• W2020724416 startingPage "L39" @default.
• W2020724416 abstract "Using Wind 3 s plasma and magnetic field data, we have identified nine reconnection exhausts within a solar wind disturbance on 1998 October 18–20 driven by a moderately fast interplanetary coronal mass ejection (ICME). Three of the exhausts within the ICME were associated with current sheets having local field shear angles, θ, ranging from 4° to 9°, the smallest reported values of θ yet associated with reconnection exhausts in a space plasma. They were observed in plasma characterized by extremely low (0.02–0.04) plasma β, and very high (281–383 km s−1) Alfvén speed, VA. Low β allows reconnection to occur at small θ and high VA leads to exhaust jets that are fast enough relative to the surrounding solar wind to be readily identified. Very small-θ current sheets are common in the solar wind at 1 AU, but typically are not associated with particularly low plasma β or high VA. On the other hand, small-θ current sheets should be common in the lower solar corona, a plasma regime of extremely low β and extremely high VA. Our observations lend credence to models that predict that reconnection at small-θ current sheets is primarily responsible for coronal heating." @default.
• W2020724416 created "2016-06-24" @default.
• W2020724416 creator A5066058076 @default.
• W2020724416 creator A5073617450 @default.
• W2020724416 date "2013-01-16" @default.
• W2020724416 modified "2023-09-26" @default.
• W2020724416 title "MAGNETIC RECONNECTION IN THE SOLAR WIND AT CURRENT SHEETS ASSOCIATED WITH EXTREMELY SMALL FIELD SHEAR ANGLES" @default.
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• W2020724416 doi "https://doi.org/10.1088/2041-8205/763/2/l39" @default.
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