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Tracing Geomagnetic Conjugate Points by means of Extremely
Similar Interhemispheric Auroras
N. Sato (1), A. Kadokura (1), Y. Ebihara (1) ,H. Deguchi (1), and T. Saemundsson (2)
(1) National Institute of Polar Research, Tokyo, Japan ([email protected])
(2) Science Institute, University of Iceland, Iceland
National Institute of Polar Research (NIPR)
IAGA 2005
Auroral Conjugate Observation at Syowa and IcelandVisualization of the conjugate foot prints of the geomagnetic field lines
Conjugate point of Syowa Station (IGRF model)
Station
Glat (deg)
Glon (deg)
Inv.lat
(deg)
Mlon (deg
)
MLT (hr)
at 0.0 UT
L valu
e
D (deg)
I (deg)
B (nT)
Tjornes
66.20 -17.12 66.41 71.26 23.46 6.25 -16.21 76.57 52321
Syowa -69.00 39.58 66.27 71.75 23.49 6.17 -48.68 -63.61 43178
Comparison of geomagnetic parameters (Epoch: 23:20:00 UT, 26 Sep, 2003)
All-Sky Image and Geomagnetic mesh
at 120 km altitudeTJORNES SYOWA
at 23:23:00 UT on Sep. 26, 2003Magnetic zenith
Projection on Geomagnetic planeat 120 km altitude
TJORNES SYOWA
at 23:23:00 UT on Sep. 26, 2003 (elevation > 10 ゚ )
Abstract of the Syowa-Iceland Auroral Conjugate Observation, so far
• Starting from 1984 (20 years anniversary )• Executed every year in the equinox season,
mainly in September, for about two weeks• Simultaneous darkness for about 4 hours• Only 2~ 3 nights of simultaneous observation
in one season, mainly due to weather condition• Good conjugate event is rare
★September 26, 2003 event : The best conjugate event in the 20 year
history
SYOWA IcelandFluxgate magnetometer ○
Induction magnetometer ○
Riometer ○
VLF receiver ○
Imaging Riometer ○
All-sky TV camera ○ (only equinox)
All-sky monochromatic Imager ○ (from 2005)
Meridian Scanning Photometer
Fabry-Perot ImagerSuperDARN radar ○
MF-radar
Ionospheric vertical sounder
VHF Doppler radar
Instruments at conjugate stations
September 26, 2003 event
HAD
YOR
UPS
NUR
HAD
YOR
UPS
NUR
H D
SAMNET data Pi2 onset : 23:18 UTOnset occurred at westward of Iceland
meridian
TJR
TJR
TJR
SYW
SYW
SYW
MN
S
W E
N
MS
W E
September 26, 2003 event all-sky TV data (23:19:30 ~ 23:23:50 UT, 10 sec interval)
TJR
TJR
TJR
SYW
SYW
SYW
September 26, 2003 event all-sky TV data (23:24:00 ~ 23:28:20 UT, 10 sec interval)
TJR
TJR
TJR
SYW
SYW
SYW
September 26, 2003 event all-sky TV data (23:28:30 ~ 23:32:50 UT, 10 sec interval)
IMAGE/FUV WIC and POLAR VIS Earth Camera
Longitudinal displacement depending on the clock angle
Satellite Observation
Østgaard et al. (JGR, 2004)
-6
-4
-2
0
2
4 Sep.26, 2003
BxGSM(nT)
-4
-2
0
2
4
ByGSM(nT)
-4
-2
0
2
4BzGSM(nT)
0
90
180
270
360
21.0 21.5 22.0 22.5 23.0 23.5 24.0CLOCK ANGLE(deg)
TIME (UT)
(X, Y, Z)gsm = (29.0 ~ 28.6, 11.1 ~ 12.5, 2.4 ~ 1.9) ReACE Vsw ~ 500 km/s
IMF dataGeotail
Østgaard et al. (JGR, 2004)
T – 8.3 minfor X= -10
Re
Magnetic variation at Syowa and Tjornes
TJR
SYW
TJR
SYW
H(nT)
TJR
SYW
D(nT)
Z(nT)
26-27 September, 2003
Equivalent current & Ionospheric potential
H
D
Z
equivalent current
&ionospheric p
otentialB
+TJRSYW
TJR
SYW
j|| N
j|| S
If BN < BS then NP could be located eastward of SP
NP
SP
North-South asymmetry of magnetospheric configuration ?
dB
dB
BN
BS
Why BN < BS ?
IMF Bx effect ? (Bx < 0 in this case)
IMF Bx
SummarySummary The September 26, 2003 event is the best one in
the 20 year history of the Syowa-Iceland conjugate auroral observation.
Extremely similar auroral activities were observed for more than 1 hour.
During the observation, the conjugate point moved about 200 km in longitude and about 50 km in latitude.
This movement cannot be explained only by the By or clock angle effect of the IMF.
North-south asymmetry of magnetospheric configuration could be a cause of the movement.
Vsw(km/s)
B (nT)
By(nT)
Bz(nT)
ASY-D(nT)
ASY-H(nT)
SYM-H(nT)
ACE
Overview of the solar – geomagnetic condition
14-29 September, 2003