Comparison between Hinode/SOT and SDO/HMI, AIA data for the study of the solar flare trigger process
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/66/SP1/S16/6912831/psu091.pdf
Reference21 articles.
1. A Model for Solar Coronal Mass Ejections
2. STUDY ON THE TRIGGERING PROCESS OF SOLAR FLARES BASED ONHINODE/SOT OBSERVATIONS
3. The Role of Transient Brightenings in Heating the Solar Corona
4. Initial Results on Line-of-Sight Field Calibrations of SP/NFI Data Taken by SOT/Hinode
5. An Emerging Flux Trigger Mechanism for Coronal Mass Ejections
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2. Properties of Flare-imminent versus Flare-quiet Active Regions from the Chromosphere through the Corona. I. Introduction of the AIA Active Region Patches (AARPs);The Astrophysical Journal;2023-01-01
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4. Improving the Spatial Resolution of Solar Images Based on an Improved Conditional Denoising Diffusion Probability Model;The Astrophysical Journal Supplement Series;2022-11-22
5. Super-Resolution of Solar Active Region Patches Using Generative Adversarial Networks;Image Analysis and Processing – ICIAP 2022;2022
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