MuSTAnG - Muon Spaceweather Telescope for Anisotropies

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Muon Spaceweather
Telescope for Anisotropies
Greifswald
- MuSTAnG -
Rainer Hippler
MuSTAnG
1
International Cooperation
With financial
support by ESA
Rainer Hippler
MuSTAnG
2
Co-Authors
A. Mengel, U Greifswald, Germany
F. Jansen, 1A Greifswald, Germany
G. Bartling, 1A Greifswald, Germany
W. Göhler, HTS Coswig, Germany
K. Munakata, Shinshu University, Japan
S. Yasue, Shinshu University, Japan
C. Kato, Shinshu University, Japan
M. Duldig, AAD Hobart, Australia
E. Flückiger, U Bern, Switzerland
G. Kolbe, AUS Stralsund, Germany
K. Kudela, IEP-SAS, Slovakia
Rainer Hippler
MuSTAnG
3
Greifswald
Home town of Caspar David Friedrich
Rainer Hippler
MuSTAnG
Marktplatz
4
Physics in Greifswald
2006
Rainer Hippler
MuSTAnG
5
Wendelstein-7-X Greifswald
Large Stellarator for
Fusion Research
Rainer Hippler
MuSTAnG
6
Spaceweather Storms
Coronal mass ejections
(CME) provide hazards to
the earth environment, in
particular to satellites,
and to power lines on
ground.
Reliable spaceweather
forecast required.
Rainer Hippler
MuSTAnG
7
Precursor Storm Signals
SSC (01:39UT 9/9 1992)
1
Nagoya V (60GV)
0
-1
(%)
Misato V (145GV)
-2
-3
Sakashita V (331GV)
-4
-5
248
250
252
254
256
day of year
Rainer Hippler
MuSTAnG
8
MuSTAnG




Muon Spaceweather Telescope for
Anisotropies at Greifswald
Multi-directional muon telescope for
spaceweather forecasting
Stage 1: 2 × 16 = 32 detectors of
0.25 m2 size each
Stage 2: Extensions to up to 2 × 36 =
72 detectors foreseen
Rainer Hippler
MuSTAnG
9
MuSTAnG: phase 1 (4m2)
Upper detector layer
Lead layer
Lower detector layer
Rainer Hippler
MuSTAnG
10
Viewing directions
upper layer
Viewing directions
are defined by
the passage of
a single muon
through one
upper and one
lower detector.
lower layer
Rainer Hippler
MuSTAnG
11
MuSTAnG: phase 1
Rainer Hippler
MuSTAnG
2
(4m )
12
Asymptotic viewing directions




Rainer Hippler
MuSTAnG
Location:
Greifswald
13 (of 49)
Viewing
directions:
V, N, E, S, W
Detector size:
0.25 m2
Rigidity spectrum:
50-150 GV
13
Detector element (4 × 0.25 = 1 m2)
Detector box:

4 scintillator plates each with

17 wavelength-shifting fibres connected to

P30A photomultiplier modules
Rainer Hippler
MuSTAnG
14
Scintillator/WLS fibre/PMT
Rainer Hippler
MuSTAnG
15
P30A module
Rainer Hippler
MuSTAnG
16
MuSTAnG
Detector boxes
Rainer Hippler
MuSTAnG
17
Scintillator
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MuSTAnG
18
Scintillator plates with wavelength-shifting fibres
Rainer Hippler
MuSTAnG
19
Detected muons (single)
Rainer Hippler
MuSTAnG
20
Detected muons (coincident)
1000
T: 3600 s
P: 25698
B:
182
Counts
800
600
S: (7.088±0.045)/s
0.63 %
400
200
0
0
1000
2000
3000
4000
Time (ns)
Upper detector-lower detector coincidences (0.0625 m2)
Rainer Hippler
MuSTAnG
21
Measured statistical accuracy


0°: 23000/h x 16 = 0.16 %
30°: 14000/h x 12 = 0.24 %
Rainer Hippler
MuSTAnG
22

Accuracy Requirement:
counts/hour/direction:
1% or better
Rainer Hippler
MuSTAnG
23
Integration of MuSTAnG into
existing muon telscope network
MuSTAnG will be part of an international
muon telescope network:
 Nagoya (Japan)
 Hobart (Australia)
 Sao Martinho (Brazil)
 Bartol (USA)
Rainer Hippler
MuSTAnG
24
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MuSTAnG
25
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MuSTAnG
26
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MuSTAnG
27
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MuSTAnG
28
University of Greifswald
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MuSTAnG
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MuSTAnG
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