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This page provides a simple browsing interface for finding entities described by a property and a named value. Other available search interfaces include the page property search, and the ask query builder.
List of results
- Precise timing of flare footpoint sources from mid-infrared observations + (October 23, 2023)
- Impact of nanoflare heating in the lower solar atmosphere + (October 30, 2023)
- Bouncing motions of fast electrons using Nobeyama Radioheliograph + (November 6, 2023)
- Search for a Flare Anticipation Index (FAI) + (November 13, 2023)
- Aurora-like Radio Emission from a Sunspot + (November 20, 2023)
- Coronal Bright Points + (November 27, 2023)
- Pre-impulsive and Impulsive Phases of the March 28, 2022 Sub-Terahertz Flare + (December 11, 2023)
- Solar flares: evaporation and simulation + (December 18, 2023)
- When it rippled in one place and exploded in another + (December 25, 2023)
- Unexpected Asymmetry in GeV Emission + (January 15, 2024)
- Sun-as-a-star Analysis of the M8.7 Flare on 2022 October 2 Using H-alpha and EUV Spectra Taken by SMART/SDDI and SDO/EVE + (February 19, 2024)
- Is there HOPE for Hyder flares... + (March 18, 2024)
- The warm-target model and kappa distributions + (September 16, 2024)
- All microflares that accelerate electrons to high energies are rooted in sunspots + (September 30, 2024)
- An X9.9 flare and its huge crochet (SFE) + (October 7, 2024)
- An X9 flare and its huge crochet (SFE) + (October 7, 2024)
- An extremely complex active region with very strong non-neutralized electric currents + (October 14, 2024)
- Unveiling CME Dynamics: Rare Rotations of CMEs in the Heliosphere + (December 30, 2024)
- Magnetic topology of quiet-Sun Ellerman bombs and associated ultraviolet brightenings + (January 6, 2025)
- Energetic neutral atoms detected in the large solar energetic particle event of February 2022 + (January 20, 2025)
- From Chromospheric Evaporation to Coronal Rain: An Investigation of the Mass and Energy Cycle of a Flare + (February 3, 2025)
- Solar Gamma-Ray Evidence for a Distinct Population of MeV Flare-Accelerated Electrons + (February 10, 2025)