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 Rainer Hippler 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 Rainer Hippler MuSTAnG 25 Rainer Hippler MuSTAnG 26 Rainer Hippler MuSTAnG 27 Rainer Hippler MuSTAnG 28 University of Greifswald Rainer Hippler MuSTAnG 29 Rainer Hippler MuSTAnG 30