Reconstruction of two-dimensional magnetopause structures from Cluster observations: verification of method
Authors:
- Annales GeophysicaeAGAnnales Geophysicae
- H HasegawaHHH Hasegawa
- I DandourasIDI Dandouras
Open Access
- 2 April 2004
- journal article
- Published by Copernicus GmbH in Annales Geophysicae
- Vol. 22 (4) , 1251-1266
Abstract
A recently developed technique for reconstructing approximately two-dimensional (∂/∂z≈0), time-stationary magnetic field structures in space is applied to two magnetopause traversals on the dawnside flank by the four Cluster spacecraft, when the spacecraft separation was about 2000km. The method consists of solving the Grad-Shafranov equation for magnetohydrostatic structures, using plasma and magnetic field data measured along a single spacecraft trajectory as spatial initial values. We assess the usefulness of this single-spacecraft-based technique by comparing the magnetic field maps produced from one spacecraft with the field vectors that other spacecraft actually observed. For an optimally selected invariant (z)-axis, the correlation between the field components predicted from the reconstructed map and the corresponding measured components reaches more than 0.97. This result indicates that the reconstruction technique predicts conditions at the other spacecraft locations quite well. The optimal invariant axis is relatively close to the intermediate variance direction, computed from minimum variance analysis of the measured magnetic field, and is generally well determined with respect to rotations about the maximum variance direction but less well with respect to rotations about the minimum variance direction. In one of the events, field maps recovered individually for two of the spacecraft, which crossed the magnetopause with an interval of a few tens of seconds, show substantial differences in configuration. By comparing these field maps, time evolution of the magnetopause structures, such as the formation of magnetic islands, motion of the structures, and thickening of the magnetopause current layer, is discussed. Key words. Magnetospheric physics (Magnetopause, cusp, and boundary layers) – Space plasma physics (Experimental and mathematical techniques, Magnetic reconnection)Keywords
This publication has 14 references indexed in Scilit:
- Relationship between field-aligned electron fluxes and field line topology at the tail lobe magnetopause: Geotail observationsAdvances In Space Research, 2005
- Double flux‐rope magnetic cloud in the solar wind at 1 AUGeophysical Research Letters, 2003
- Reconstruction of two‐dimensional structures in the magnetopause: Method improvementsJournal of Geophysical Research, 2003
- Reconstruction of magnetic clouds in the solar wind: Orientations and configurationsJournal of Geophysical Research, 2002
- Fluid and kinetics signatures of reconnection at the dawn tail magnetopause: Wind observationsJournal of Geophysical Research, 2001
- Reconstruction of magnetic flux ropes in the solar windGeophysical Research Letters, 2001
- Magnetopause transects from two spacecraft: A comparisonGeophysical Research Letters, 2000
- Two‐dimensional coherent structures in the magnetopause: Recovery of static equilibria from single‐spacecraft dataJournal of Geophysical Research, 1999
- Cold ion streams consisting of double proton populations and singly charged oxygen observed at the distant magnetopause by Geotail: A case studyJournal of Geophysical Research, 1997
- Magnetopause transectsGeophysical Research Letters, 1996