Source-linked AI summary

A method for multimodal analysis of TAIGA experiment data using essential features

Alexander Kryukov, Julia Dubenskaya, Elena Fedotova, Elizaveta Gres, Stanislav Polyakov, Eugene Postnikov, Alexander Razumov, Pavel Volchugov, Dmitry Zhurov

arXiv:2610.08985v1astro-ph.IMastro-ph.HEcs.LG

TL;DR

TAIGA's IACT and HiSCORE data come from different types of installations, and the paper addresses their joint multimodal analysis. It combines extracted features in a multitask network and reports higher EAS-parameter accuracy than traditional analysis on simulated Monte Carlo data.

  • Problem

    The paper targets joint multimodal analysis of data from different types of experimental facilities, including IACT and HiSCORE.

    Source: §2 · p. 3, CONCLUSIONS · p. 5
  • Method

    The method combines IACT autoencoder hidden-space data and HiSCORE geometric features in a fully connected multitask network for EAS parameter extraction.

    Source: §2 · p. 3
  • Results

    Monte Carlo experiments showed EAS parameter accuracy two to three times higher than with traditional analysis.

    Source: CONCLUSIONS · p. 5
  • Takeaways & Limitations

    Autoencoder feature extraction supports joint analysis of data from multiple facilities of different types at the essential-feature level.

    Source: CONCLUSIONS · p. 5

Abstract

from arXiv · show

The aim of processing and analyzing experimental data from physical experiments is to obtain physically significant information about the phenomenon under study. This goal is achieved by multi-stage processing of experimental data, during which noise associated with measurements is suppressed and the dimensionality of the input data is reduced. In this paper, we propose a new method based on the use of neural networks such as autoencoders to extract essential features. The special value of the proposed approach lies in the possibility of its application to the analysis of multimodal data received simultaneously from several installations. We will apply this approach to a multimodal data (MMD) of the experiment TAIGA. Currently, the analysis of the MMD is carried out independently for each installation separately. Therefore, the development of methods for the joint analysis of MMD from TAIGA-type installations is an urgent task in cosmic ray physics and gamma-ray astronomy. Based on Monte Carlo simulation, it is shown that the proposed method allows for effective MMD analysis. It can also be used for MMD analysis at other experimental complexes.

1. Unique experimental complex TAIGA

TAIGA combines imaging atmospheric Cherenkov telescopes with wide-angle HiSCORE stations, but traditional reconstruction processes the two data sources in separate stages.

1. Unique experimental complex TAIGA

  • IACT cameras contain about 600 PMTs assembled in a hexagonal grid, with each PMT recording input-signal amplitude.Source: §1 · p. 2
  • HiSCORE comprises more than 120 stations covering 1 km², spaced about 150 m apart, and recording signal amplitude, duration, and arrival time.Source: §1 · p. 2
  • IACTs record Cherenkov-light distributions from EAS, while HiSCORE records their spatiotemporal distributions at ground level.Source: §1 · p. 2
  • Traditional processing first uses HiSCORE to estimate the EAS arrival point and axis direction, then converts IACT images to Hillas parameters for estimating energy and particle type.Source: §1 · p. 3
  • This two-stage method does not jointly combine data from both experimental sets.Source: §1 · p. 3

2. Multimodal data analysis of TAIGA facilities

The proposed analysis compresses and fuses IACT and HiSCORE information as essential features before predicting EAS physical parameters.

2. Multimodal data analysis of TAIGA facilities

  • The optimal autoencoder hidden-space dimension was determined to be 12 for compressing input data while retaining acceptable reconstruction accuracy.Source: §2 · p. 3
  • IACT hidden-space data and HiSCORE geometric parameters extracted with 1D convolution networks are used as essential features.Source: §2 · p. 3
  • The features are concatenated into one vector and passed to a fully connected multitask network to extract EAS physical parameters.Source: §2 · p. 3

3. Discussion and results

On simulated Monte Carlo data, the proposed method outperformed traditional analysis on EAS parameter reconstruction. The discussion connects this result to feature extraction and joint analysis across different facilities.

3. Discussion and results

  • 0.3 at 40 TeV and 0.1 at 400 TeV were the machine-learning relative energy reconstruction errors, versus 0.8 and 0.3 for the traditional method.The traditional method underestimated EAS energy, producing a systematic error of 56 TeV.Source: Figure 3 · p. 4, §3 · p. 4
  • The comparison used a test set of about 2,000 events, generated from 40 to 400 TeV and excluded from training and validation.Training used about 30,000 joint IACT1 and HiSCORE Monte Carlo events, with about 10,000 additional joint events for validation.Source: §3 · pp. 3–4
  • The machine-learning method's EAS core-position error was about 6 m, more than two times less than the traditional method's; Figure 4 shows the comparison.Source: §3 · pp. 4–5, Figure 4 · p. 5
  • Autoencoder-type feature extraction allows data from different facilities to be combined at the essential-feature level for joint multimodal analysis.Source: CONCLUSIONS · p. 5
  • The approach treats the autoencoder latent space as an abstract input representation, avoiding the need to interpret its parameters in physically motivated terms.Source: CONCLUSIONS · p. 5
  • A fully connected multitask network can use specialized heads adapted to the characteristics of the EAS physical parameters being reconstructed.Source: CONCLUSIONS · p. 5
  • EAS parameter accuracy was two to three times higher with the proposed method than with traditional analysis in Monte Carlo experiments.Source: CONCLUSIONS · p. 5
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