RHESSI Nugget List

	RHESSI Nugget Index	RHESSI Nugget Date
Can EUV Power-Spectral Indices Reveal Imminent Solar Flares?	521	6 April 2026
How energetic can solar flares become?	520	23 March 2026
Hinode EIS Observations of Plasma Composition Evolution and Radiative Cooling of Flare Loops	519	16 March 2026
When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps	518	9 March 2026
Observational Evidence Linking Loop Length and Thermal/Nonthermal Peak Timing in Solar Flares	517	23 February 2026
A fine-scale bright kernel captured by Hi-C 3 in the post-maximum phase of an M-class solar flare	516	9 February 2026
On the Relationship Between Nanoflare Energy and Delay in the Closed Solar Corona	515	19 January 2026
Fine structures in solar flare ribbons	514	12 January 2026
The M- and X-class White-light Flares in Super Active Region NOAA 13664/13697	513	5 January 2026
Iron Fluorescence in X-class Solar Flares	512	8 December 2025
Sun-as-a-star Analysis of a Solar Eruption Source Region Using H-alpha Spectroscopic Observations from CHASE	510	24 November 2025
On the Origin of Solar Long-Duration Gamma-Ray Flares	509	3 November 2025
FAI and GOES eclipses	508	20 October 2025
The EUV Late Phase	507	13 October 2025
Time evolution of flare-accelerated electrons using the warm-target model	506	6 October 2025
Time evolution of flare-accelerated electrons in the warm-target model	506	6 October 2025
SOLSTICE observes flare Doppler shifts in Si III	505	30 September 2025
Flare Phases and the Earth's Ionospheric Response	504	16 September 2025
Neupertianity	503	25 August 2025
Synchrotron Radiation and the Foundations for a Cosmic Bridge	502	4 August 2025
The Aulanier Effect: drifting footpoints of CME flux ropes	501	21 July 2025
Five Hundred Nuggets	500	14 July 2025
Quasiperiodic Pulsations in the Balmer Continuum in an X-class Solar White-light Flare	499	30 June 2025
High-Resolution Observations of a C3 class White-Light Flare	498	16 June 2025
The Sun's open-closed flux boundary and the origin of the slow solar wind	497	26 May 2025
Delay of Near-Relativistic Electrons	496	19 May 2025
A Multi-Site Telescope for Multi-Height for Synoptic Observations	495	12 May 2025
Multi-Height Multi-site Synoptic Observations	495	12 May 2025
On turbulent magnetic reconnection: fast and slow mean steady-states	494	28 April 2025
Quasi-Periodic Pulsations in Ionospheric TEC and Flare EUV	493	21 April 2025
Metis observations of Alfvenic outflows driven by interchange reconnection in a pseudostreamer	492	7 April 2025
Solar Rollercoaster: looping-the-loop in the solar corona	491	31 March 2025
Proton Beam Energy Deposition as a Mechanism of Deep Photospheric Heating	490	17 March 2025
New insights into the proton precipitation sites in solar flares	489	10 February 2025
Solar Gamma-Ray Evidence for a Distinct Population of MeV Flare-Accelerated Electrons	488	10 February 2025
From Chromospheric Evaporation to Coronal Rain: An Investigation of the Mass and Energy Cycle of a Flare	487	3 February 2025
Energetic neutral atoms detected in the large solar energetic particle event of February 2022	486	20 January 2025
Magnetic topology of quiet-Sun Ellerman bombs and associated ultraviolet brightenings	485	6 January 2025
Unveiling CME Dynamics: Rare Rotations of CMEs in the Heliosphere	484	30 December 2024
Spatial and Spectral Evolution of Microwave and X-Ray Sources During the Limb Flare SOL2023-02-05	483
High-resolution observational analysis of flare ribbon fine structures	482
Advection and super-diffusive expansion as the model of flare accelerated electron transport in type III solar radio bursts	481
Faraday's Law in Solar Flares: A Cautionary Message	480
Remarkable NUV Spectrum of an M-star Megaflare	479
Revised Point-Spread Functions of AIA and their effect on DEM analyses	478
How much of the energy in flare-accelerated electrons reaches the chromosphere?	477
Spatially resolved plasma composition evolution in a solar flare	476
HOPE during high activity	475
Simulated heliospheric electron spectra show sensitivity to plasma properties of a source region in the flaring corona	474
An extremely complex active region with very strong non-neutralized electric currents	473	14 October 2024
... further results