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Plasmasheet Response to Multiple Substorm Activations

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Title: Plasmasheet Response to Multiple Substorm Activations


1
Plasmasheet Response to Multiple Substorm
Activations
The Interball-ground experimentators
T. Bösinger, V. A. Segeev, A. G. Yahnin, L.
Vagina, K. Kudela, J.-A. Sauvaud, D. Milling,
N. L. Borodkova, V. N. Lutsenko, A. Skalsky, et
al.
2
What?
1
A series of substorms, substorm intensifications
and activations north of Scandinavia on 9
December 1995 and Interball Tail Probe (IT1) and
its Companion (IT2)
Substorm I
Substorm II
Substorm III
Table 1 Time line, observation platforms, main
events
SCW Substorm Current wedge uFAC upward
directed Field Aligned Current AEJw westward
Auroral ElectroJet PS Plasma Sheet
3
Where?
2
IT-1
IT-2
Neutral Sheet
Interball Tail probe IT-1
Fig. 4
The IMAGE network of magnetic recordings.
4
SCW parameters
Pi2/Pi1B onsets
  • no electrojet currents,
  • magnetic signatures gt DP1 current system
  • determination of SCW position, parameters, etc.

5
Interball tail-probe (IT-1) - ground temporal
correlation
Pi2/Pi1B onsets
  • close temporal relationship between magnetic
  • signatures at IT-1 and auroral stations (e.g.
    KEVO)
  • from 20 to 22 UT
  • 4 substorms, the first three conjugate to
    Scandinavia

6
ELECTRON data from Interball tail-probe (IT-1)
  • disappearance of PS electrons (exit to the lobe)
    gradually
  • starting at 1930 and in between 2043 and
    2052 UT.
  • similar to above but with higher time resolution
  • (2020 to 2100 UT) and PA close to
    field-aligned
  • note behaviour of S/C potential (low energy
    electrons)

7
B-field (gsm) at IT-1
20 nT
Bz
By
Bx
lobe
SCW
-40 nT
2015 UT
2045 UT
20 nT
Bz
By
SCW
Bx
lobe
-40 nT
2030 UT
2100 UT
  • large changes in Bx, small changes in By and Bz
  • intrusion of IT-1 into PS gt PS expansion
  • intrusion of IT-1 into PS in agreement with
    ELECTRON data
  • IT-1 not far from the PS-boundary
  • no or only small signatures of dipolarization
  • spiky By bursts, By-shear gt FAC
  • at PS-boundary FACs ?
  • SCW gt large scale, large time constant current
    system
  • FACs at PS-boundary gt current filaments
  • current filements in B-turbulent region

8
By spikes (IT-1)
2048 UT
2052 UT
9
Electron energy spectra (IT-1)
10
Injection at Magion-4 (IT-2)
T1
T4
T2
  • T1 202242 UT
  • T2 204830 UT
  • T4 205100 UT

11
Timing PS-expansion (IT-1) versus Injection
(IT-2)
The high temporal resolution of PRAM, ELECTRON
(IT-1) and DOK-S (IT-2) data made it possible to
do some relative timing analysis
  • throughout the timing analysis we distinguished
    between onset
  • and peak values, wherever possible.
  • during substorm I, the appearance of
    PS-electrons at IT-1
  • occurred within 3 s at the same time,
    independent of energy
  • and pitch-angle.
  • the same holds for substorm II within 6 s,
    beside that PS
  • electrons appeared in 3 subsequent jumps. Each
    was dealt
  • separately.
  • during substorm II, the onsets of sudden Bx
    deflection and
  • PS-electrons appearance (IT-1) were delayed by
    10 to 20 s with
  • respect to electron injection onset (IT-2). The
    peak values in the
  • 3 data sets were, however, reached
    simultaneously.
  • during substorm I, the onsets of Bx deflection,
    and appearance
  • of PS-electrons (IT-1), and electron injection
    signatures (IT-2)
  • were probably also delayed (data gap).
  • Pi2/PiB onsets as determined on the ground were
    within 1 min
  • simultaneous with IT-1/IT-2 signatures.
  • the By spike associated appearance of PS
    electrons was lead by
  • field-aligned electrons.

12
Summary and Conclusions
general aspects
  • substorms during low magnetic activity
  • substorms of small intensity (lt 100 nT)
  • practically no PEJ currents
  • magnetic signatures only of DP-1 type
  • active region north of Scandinavia
  • contracted auroral oval
  • no injection signatures at geostationary orbit
  • IT-1 and IT-2 conjugate to active region at x
    -10-12 Re
  • IT-1 and IT-2 either inside PS, close to NS, at
    PS boundary
  • or exiting into the lobe
  • PS expansion simultaneous with onsets of
    substorms,
  • no or small dipolarization signatures
  • appearance of PS electrons at IT-1 simultaneous
    within
  • 3 s regardless of energy and pitch angle
  • injection signatures (gt 23 keV) at IT-2 (-10.6
    Re) 10-20 s
  • earlier than PS expansion at IT-1 (-11.6 Re)
  • IT-1 and IT-2 close but tailward of reconnection
    region
  • tiny, small substorms exhibit the same
    signatures as big
  • ones

13
Summary and Conclusions
specific aspects
  • field-aligned current filements (By spikes) at
    PS boundary
  • during PS expansion
  • appearance of By spike associated PS electrons
    led by
  • field-aligned electrons
  • deeper in the PS, electrons PA distribution
    isotropic
  • deeper in the PS, B-field turbulent
  • B-field turbulence as long as SCW development
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