Evidence map›Paper›PMID 41374574›Full record

ArticleSensors (Basel, Switzerland)2025

A Solar Array Temperature Multivariate Trend Forecasting Method Based on the CA-PatchTST Model.

Yunhai Wang, Xiaoran Shi, Zhenxi Zhang, Feng Zhou

Abstract read
In one paragraph

Article in Sensors (Basel, Switzerland), 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

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1 · What the graph read from it

What it found

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The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

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3 · Its place in the literature

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0 citing papers in PubMed.

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4 · The record

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5 · Who and what money

Authors and funding

4 authors.

Yunhai WangKey Laboratory of Electronic Information Countermeasure and Simulation Technology of Ministry of Education, Xidian University, Xi'an 710071, China.
Xiaoran ShiKey Laboratory of Electronic Information Countermeasure and Simulation Technology of Ministry of Education, Xidian University, Xi'an 710071, China.ORCID 0000-0003-4636-2966
Zhenxi ZhangKey Laboratory of Electronic Information Countermeasure and Simulation Technology of Ministry of Education, Xidian University, Xi'an 710071, China.ORCID 0009-0009-6297-623X
Feng ZhouSchool of Aerospace Science and Technology, Xidian University, Xi'an 710071, China.

Funding

China Postdoctoral Science Foundation 2024M761178 and 2025M771739Fundamental Research Funds for the Central Universities ZYTS25144National Natural Science Foundation of China 62401429, 62401445, and 62425113Postdoctoral Fellowship Program of CPSF GZC20241332, GZC20232048 and GZC20251207
6 · The paper itself

Abstract

System reliability, which is essential for the normal operation of satellites in orbit, is decisively governed by the performance of solar array, making accurate temperature forecasting of solar array imperative. Reliable solar array temperature forecasting is essential for predictive maintenance and autonomous power-system management. Forecasting relies on temperature telemetry data, which provide comprehensive thermal information. This task remains challenging due to the high-dimensional, long-horizon temperature sequences with inherent cross-variable coupling, whose dynamics exhibit nonlinear and non-stationary behaviors owing to orbital transitions and varying operational modes. In this context, multi-step forecasting is essential, as it better characterizes long-term dynamics of temperature and provides forward-looking trends that are beyond the capability of single-step forecasting. To tackle these issues, we propose a solar array temperature multivariate trend forecasting method based on Cross-Attention Patch Time Series Transformer (CA-PatchTST). Specifically, we decompose temperature variables into trend and residual components using a moving average filter to suppress noise and highlight the dominant component. In addition, the PatchTST model extracts local features and long-term dependencies of the trend and residual components separately through the patching encoders and channel-independent mechanisms. The cross-attention mechanism is designed to capture the correlation between temperature variables of different devices in solar array. Extensive experiments on the real solar array temperature dataset demonstrate that the CA-PatchTST surpasses mainstream baselines in root mean square error (RMSE), mean absolute error (MAE), and mean absolute percentage error (MAPE), with ablation studies further confirming the complementary roles of sequence decomposition and cross-attention.

Indexed as

cross-attention mechanismPatchTSTsatellite telemetry datasolar arraytemperature multivariate trend forecasting

Identifiers

PMID41374574
PMCPMC12694205

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.