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Walen and Slow-mode Shock Analyses Applied to High-Speed Flows of the Near-Earth Magnetotail

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Title: Walen and Slow-mode Shock Analyses Applied to High-Speed Flows of the Near-Earth Magnetotail


1
Walen and Slow-mode Shock Analyses Applied to
High-Speed Flows of the Near-Earth Magnetotail
  • S. Eriksson1, C. Mouikis2, M. W. Dunlop3, M.
    Oieroset4,
  • D. N. Baker1, C. Cully1, H. Reme5, and A. Balogh6
  • 1 Laboratory for Atmospheric and Space Physics,
    University of Colorado, Boulder, USA
  • 2 Space Science Center, University of New
    Hampshire, Durham, USA
  • 3 Rutherford Appleton Laboratory, Chilton, UK
  • 4 Space Sciences Laboratory, University of
    California, Berkeley, USA
  • 5 Centre dEtude Spatiale des Rayonnements,
    Toulouse, France
  • 6 Imperial College, London, UK

Contact information eriksson_at_lasp.colorado.edu
2
Outline
  • Introduction
  • Tail reconnection and slow-mode shocks
  • deHoffmann-Teller and Walen analyses
  • Slow-mode shock criteria
  • Cluster observations
  • 2001-08-27 from 0350 UT to 0435 UT
  • 2001-09-15 from 0355 UT to 0520 UT
  • 2002-08-21 from 0750 UT to 0840 UT
  • Summary

3
Tail Reconnection and Slow-mode Shocks
Hill, T.W., JGR, 80, 4689, 1975
Feldman et al., JGR, 92, 83, 1987
  • Acceleration in tail reconnection is assumed to
    take place across a slow-mode shock (SS)
    connected to the diffusion region.
  • SS generated due to near-symmetric conditions
    (comparable plasma density and magnetic field
    strength) on either side of the current layer.
  • Configuration essentially that of Petschek
    1964 (above right).

4
Tail Reconnection and Slow-mode Shocks
Hill, T.W., JGR, 80, 4689, 1975
Feldman et al., JGR, 92, 83, 1987
  • Slow-mode shocks were first observed in the
    tail by e.g. Feldman et al. 1984, 1987 using
    the Rankine-Hugoniot (RH) jump conditions on ISEE
    2 data.
  • Later confirmed by Geotail RH observations
    e.g. Saito et al., 1995 Seon et al., 1996 and
    by Wind data Oieroset et al., 2000 using the
    shear-stress balance test on Wind data 60 Re
    downtail.

5
deHoffmann-Teller Analysis
Khrabrov and Sonnerup, ISSI Sci.rep., 1998
  • The existence of an HT frame indicates the
    presence of a quasi-stationary coherent pattern
    of magnetic field and plasma velocity.

6
Shear-Stress Balance (Walen) Test
  • Disturbance generated by reconnection propagates
    away from the diffusion region at a field-aligned
    phase speed in the HT shock frame determined by
    the type and strength of the shock.

7
Shear-Stress Balance (Walen) Test
  • The sign of the Walen slope depends on whether
    the B-field is parallel or antiparallel to the
    flow direction.

8
Walen Analysis in the Magnetotail
Walen slope
Oieroset et al., JGR, 105, 25,247, 2000.
9
Walen Analyses at Wind (x -60 Re)
Oieroset et al., JGR, 105, 25,247, 2000.
  • Earthward jet
  • Negative Bx
  • Walen slope
  • should be positive

(Note that there is no ion composition in the
Wind data set and that these slopes were derived
assuming 100 H.)
10
Slow-mode Shock Criteria
11
Cluster Observations on 2001-08-27
A
B
C
12
Walen Analyses 2001-08-27
A Tailward flows in Northern Hemisphere
13
Walen Analyses 2001-08-27
B Earthward flows in Northern Hemisphere
14
Walen Analyses 2001-08-27
C Earthward flows in Northern Hemisphere
15
Shock Analysis on 2001-08-27
A
B
C
A
C
16
Shock Normal Optimization 2001-08-27
17
Cluster Observations on 2001-09-15
A
B
C
18
Walen Analyses 2001-09-15
A Tailward flows in Northern Hemisphere
19
Walen Analyses 2001-09-15
B Tailward flows in Northern Hemisphere
20
Walen Analyses 2001-09-15
C Tailward flows in Southern Hemisphere
21
Shock Analysis on 2001-09-15
B
A
C
A
B
22
Cluster Observations on 2002-08-21
A
B
C
23
Walen Analyses 2002-08-21
A Tailward flows in Northern Hemisphere
24
Walen Analyses 2002-08-21
B Tailward flows in Northern Hemisphere
25
Walen Analyses 2002-08-21
C Tailward flows in Southern Hemisphere
26
Shock Analysis on 2002-08-21
B
A
C
B
27
Summary
  • The Walen test together with the location of
    Cluster suggest the presence of slow-mode shocks
    on the tailward sides of near-Earth X-lines
    (Xgt-19 Re) for three events 2001-08-27,
    2001-09-15, 2002-08-21.
  • Earthward jets seemingly fail the Walen test more
    readily than tailward jets.
  • Joint Walen and RH analyses generally confirm the
    presence of slow-mode shocks during accelerated
    tailward flows. Based on three events and several
    jets.
  • Shock-normal analyses suggest that magnetic
    coplanarity theorem results in a normal near the
    optimized (minimum RH deviations) direction.
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