Deep learning based methods for gamma ray interaction location estimation in monolithic scintillation crystal detectors

2020 ◽  
Vol 65 (11) ◽  
pp. 115007
Author(s):  
Li Tao ◽  
Xin Li ◽  
Lars R Furenlid ◽  
Craig S Levin
2021 ◽  
Author(s):  
Jannes Münchmeyer ◽  
Dino Bindi ◽  
Ulf Leser ◽  
Frederik Tilmann

<p><span>The estimation of earthquake source parameters, in particular magnitude and location, in real time is one of the key tasks for earthquake early warning and rapid response. In recent years, several publications introduced deep learning approaches for these fast assessment tasks. Deep learning is well suited for these tasks, as it can work directly on waveforms and </span><span>can</span><span> learn features and their relation from data.</span></p><p><span>A drawback of deep learning models is their lack of interpretability, i.e., it is usually unknown what reasoning the network uses. Due to this issue, it is also hard to estimate how the model will handle new data whose properties differ in some aspects from the training set, for example earthquakes in previously seismically quite regions. The discussions of previous studies usually focused on the average performance of models and did not consider this point in any detail.</span></p><p><span>Here we analyze a deep learning model for real time magnitude and location estimation through targeted experiments and a qualitative error analysis. We conduct our analysis on three large scale regional data sets from regions with diverse seismotectonic settings and network properties: Italy and Japan with dense networks </span><span>(station spacing down to 10 km)</span><span> of strong motion sensors, and North Chile with a sparser network </span><span>(station spacing around 40 km) </span><span>of broadband stations. </span></p><p><span>We obtained several key insights. First, the deep learning model does not seem to follow the classical approaches for magnitude and location estimation. For magnitude, one would classically expect the model to estimate attenuation, but the network rather seems to focus its attention on the spectral composition of the waveforms. For location, one would expect a triangulation approach, but our experiments instead show indications of a fingerprinting approach. </span>Second, we can pinpoint the effect of training data size on model performance. For example, a four times larger training set reduces average errors for both magnitude and location prediction by more than half, and reduces the required time for real time assessment by a factor of four. <span>Third, the model fails for events with few similar training examples. For magnitude, this means that the largest event</span><span>s</span><span> are systematically underestimated. For location, events in regions with few events in the training set tend to get mislocated to regions with more training events. </span><span>These characteristics can have severe consequences in downstream tasks like early warning and need to be taken into account for future model development and evaluation.</span></p>


2017 ◽  
Vol 12 (02) ◽  
pp. C02034-C02034 ◽  
Author(s):  
C. Polito ◽  
R. Pani ◽  
C. Trigila ◽  
M.N. Cinti ◽  
A. Fabbri ◽  
...  

2005 ◽  
Vol 52 (5) ◽  
pp. 1439-1446 ◽  
Author(s):  
A.P. Dhanasopon ◽  
C.S. Levin ◽  
A.M.K. Foudray ◽  
P.D. Olcott ◽  
F. Habte

Universe ◽  
2021 ◽  
Vol 7 (11) ◽  
pp. 396
Author(s):  
Minbin Kim ◽  
Jakub Ripa ◽  
Il H. Park ◽  
Vitaly Bogomolov ◽  
Søren Brandt ◽  
...  

We developed an X-ray detector using 36 arrays, each consisting of a 64-pixellated yttrium oxyorthosilicate (YSO) scintillation crystal and a 64-channel multi-anode photomultiplier tube. The X-ray detector was designed to detect X-rays with energies lower than 10 keV, primarily with the aim of localizing gamma-ray bursts (GRBs). YSO crystals have no intrinsic background, which is advantageous for increasing low-energy sensitivity. The fabricated detector was integrated into UBAT, the payload of the Ultra-Fast Flash Observatory (UFFO)/Lomonosov for GRB observation. The UFFO was successfully operated in space in a low-Earth orbit. In this paper, we present the responses of the X-ray detector of the UBAT engineering model identical to the flight model, using 241Am and 55Fe radioactive sources and an Amptek X-ray tube. We found that the X-ray detector can measure energies lower than 5 keV. As such, we expect YSO crystals to be good candidates for the X-ray detector materials for future GRB missions.


2021 ◽  
Vol 907 (2) ◽  
pp. 121
Author(s):  
Li Tang ◽  
Xin Li ◽  
Hai-Nan Lin ◽  
Liang Liu

2021 ◽  
Author(s):  
C Christoph ◽  
G Birindelli ◽  
M Pizzichemi ◽  
M Kruithof-de Julio ◽  
E Auffray ◽  
...  

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