Title: Plasmasheet Response to Multiple Substorm Activations
1Plasmasheet 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.
2What?
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
3Where?
2
IT-1
IT-2
Neutral Sheet
Interball Tail probe IT-1
Fig. 4
The IMAGE network of magnetic recordings.
4SCW parameters
Pi2/Pi1B onsets
- no electrojet currents,
- magnetic signatures gt DP1 current system
- determination of SCW position, parameters, etc.
5Interball 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
6ELECTRON 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)
7B-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
8By spikes (IT-1)
2048 UT
2052 UT
9Electron energy spectra (IT-1)
10Injection at Magion-4 (IT-2)
T1
T4
T2
- T1 202242 UT
- T2 204830 UT
- T4 205100 UT
11Timing 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.
12Summary 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
13Summary 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