Demonstration venue · read-only. Every page can be browsed; the buttons that would change it are switched off. Create an account to run TaxoReview on your own data. A simulation from public publication records: the people listed were not invited and did not agree to review.
? Tutorial for this page

Shunya Nagashima

dblp:360/6422 · DBLP profile ↗
← Back
1ranked-venue papers
1as first author
1since 2021 · last 2025
—ORCID · unresolved

Domains — the database's venue-derived domains; a paper can count in several

Artificial intelligence and machine learning · 1 · 1 first-author · 1 since 2021Graphics, computer vision, multimedia, augmented reality and games · 1 · 1 first-author · 1 since 2021

Expertise — from the expertise taxonomy: the topics of the expert's papers under the CCF categories. A weight counts papers with recency: 1 for a paper about the topic, 0.3 when the topic is its context, halved every five years.

Artificial intelligence
1 paper
Deep learning architectures and training · 50% Representation and self-supervised learning · 50%
Interdisciplinary, comprehensive, and emerging computing
1 paper
Computational science and engineering · 100%

Topics — the 3 heaviest of 4, each with the papers that count most for it

TopicWeightPapersLastEvidence papers
Machine learning › Representation and self-supervised learning › representation learning › unsupervised representation learning › self-supervised representation learning
masked autoencoder
0.912025
Deep Space Weather Model: Long-Range Solar Flare Prediction from Multi-Wavelength Images · ICCV 2025
Machine learning › Deep learning architectures and training
state space model
0.912025
Deep Space Weather Model: Long-Range Solar Flare Prediction from Multi-Wavelength Images · ICCV 2025
Computational science and engineering › astronomy
solar flare prediction
0.912025
Deep Space Weather Model: Long-Range Solar Flare Prediction from Multi-Wavelength Images · ICCV 2025

Methods — techniques the papers use, named apart from their topics

sparse masked autoencoder · 1.7multi-wavelength image analysis · 1.7deep state space model · 1.7
YearPublicationVenuePosition
2025 Deep Space Weather Model: Long-Range Solar Flare Prediction from Multi-Wavelength Images
abstract
Accurate, reliable solar flare prediction is crucial for mitigating potential disruptions to critical infrastructure, while predicting solar flares remains a significant challenge. Existing methods based on heuristic physical features often lack representation learning from solar images. On the other hand, end-to-end learning approaches struggle to model long-range temporal dependencies in solar images. In this study, we propose Deep Space Weather Model (Deep SWM), which is based on multiple deep state space models for handling both ten-channel solar images and long-range spatio-temporal dependencies. Deep SWM also features a sparse masked autoencoder, a novel pretraining strategy that employs a two-phase masking approach to preserve crucial regions such as sunspots while compressing spatial information. Furthermore, we built FlareBench, a new public benchmark for solar flare prediction covering a full 11-year solar activity cycle, to validate our method. Our method outperformed baseline methods and even human expert performance on standard metrics in terms of performance and reliability. The project page can be found at https://keio-smilab25.github.io/DeepSWM.
Shunya Nagashima, Komei Sugiura
ICCV1