Currently, sci.esa.int is under review and not being updated. For the latest information and news from ESA science missions and scientific results, please visit esa.int. For a comprehensive overview of ESA’s Science Programme and its missions, please refer to science.esa.int. For in-depth technical information aimed at ESA's scientific communities, you may also wish to consult cosmos.esa.int.

Asset Publisher

Back Cluster observation of collisionless transport at the magnetopause

Cluster observation of collisionless transport at the magnetopause

Publication date: 12 August 2006

Authors: Panov, E.V. et al.

Journal: Geophys. Res. Lett.
Volume: 33
Issue: 15
Page: L15109
Year: 2006

Copyright: American Geophysical Union

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 Omegacp (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 (Wp > 300 eV) penetrate into the BLs also via finite gyro-radius effect.

Link to publication
Last Update: Sep 1, 2019 9:18:16 AM
25-Jan-2026 05:38 UT

ShortUrl Portlet

Shortcut URL

https://sci.esa.int/s/WvP2ngA

Images And Videos

Related Publications

Related Links

See Also

Documentation