Abstract
On May 10, 2002 the CLUSTER spacecraft (SC) encountered a ∼450 km (five magnetosheath thermal proton gyro-radii) wide high-latitude magnetopause (MP). Magnetic field observations indicate the crossing of a ∼130 km thick MP current sheet (CS) located inside a magnetic hole. Proton flux measurements diagnose a dense boundary layer (BL) directly attached to the MP and an additional rare BL located earthwards from the MP. Enhanced magnetic fluctuations are found near the local proton-cyclotron frequency Ωcp (0.4-2 Hz). Applying the phase-differencing technique we obtained a wavelength of 150-250 km and the propagating direction earthward perpendicular to the MP. Inside the MP the pitch-angle proton distribution demonstrates the presence of a transverse population. The formation of the two BLs can be understood by enhanced collisionless diffusion of magnetosheath protons due to wave-particle interaction, while higher-energy protons (W p > 300 eV) penetrate into the BLs also via finite gyro-radius effect. Copyright 2006 by the American Geophysical Union.
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CITATION STYLE
Panov, E. V., Büchner, J., Fränz, M., Korth, A., Savin, S. P., Fomaçon, K. H., … Rème, H. (2006). CLUSTER observation of collisionless transport at the magnetopause. Geophysical Research Letters, 33(15). https://doi.org/10.1029/2006GL026556
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