RHESSI Nugget List

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 RHESSI Nugget IndexRHESSI Nugget DateRHESSI Nugget First AuthorRHESSI Nugget Second Author
On the Relationship Between Nanoflare Energy and Delay in the Closed Solar Corona51519 January 2026Shanwlee SOW MONDAL et al.
Fine structures in solar flare ribbons51412 January 2026Jonas THOEN FABER
The M- and X-class White-light Flares in Super Active Region NOAA 13664/136975135 January 2026Zhichen JINGand Ying LI
Iron Fluorescence in X-class Solar Flares5128 December 2025Abhilash SARWADEet al.
Sun-as-a-star Analysis of a Solar Eruption Source Region Using H-alpha Spectroscopic Observations from CHASE51024 November 2025Xiaofeng LIUYijun HOU
On the Origin of Solar Long-Duration Gamma-Ray Flares5093 November 2025Alessandro BRUNOet al.
FAI and GOES eclipses50820 October 2025Hugh HUDSON
The EUV Late Phase50713 October 2025Sascha ORNIG
Time evolution of flare-accelerated electrons using the warm-target model5066 October 2025Debesh BHATTACHARJEE,Eduard KONTAR and Yinjie LUO
Time evolution of flare-accelerated electrons in the warm-target model5066 October 2025Debesh BHATTACHARJEE,Eduard KONTAR and Yinjie LUO
SOLSTICE observes flare Doppler shifts in Si III50530 September 2025Luke MAJURY
Flare Phases and the Earth's Ionospheric Response50416 September 2025Susanna BEKKER
Neupertianity50325 August 2025Hugh HUDSON
Synchrotron Radiation and the Foundations for a Cosmic Bridge5024 August 2025Immanuel Jebaraj
The Aulanier Effect: drifting footpoints of CME flux ropes50121 July 2025Jaroslav DUDÍK,Juraj LÖRINČÍK and Brigitte SCHMIEDER
Five Hundred Nuggets50014 July 2025Hugh HUDSON
Quasiperiodic Pulsations in the Balmer Continuum in an X-class Solar White-light Flare49930 June 2025De-Chao SONGet al.
High-Resolution Observations of a C3 class White-Light Flare49816 June 2025Zhe XUXiaoli YAN
The Sun's open-closed flux boundary and the origin of the slow solar wind49726 May 2025Chloe WILKINSDavid PONTIN
Delay of Near-Relativistic Electrons49619 May 2025Grant MITCHELL
A Multi-Site Telescope for Multi-Height for Synoptic Observations49512 May 2025Fallon KONOW
Multi-Height Multi-site Synoptic Observations49512 May 2025Fallon KONOW
On turbulent magnetic reconnection: fast and slow mean steady-states49428 April 2025Sage STANISHDavid MacTAGGART
Quasi-Periodic Pulsations in Ionospheric TEC and Flare EUV49321 April 2025Aisling O'HARE
Metis observations of Alfvenic outflows driven by interchange reconnection in a pseudostreamer4927 April 2025Paolo ROMANOthe Metis team
Solar Rollercoaster: looping-the-loop in the solar corona49131 March 2025Mohamed NEDALet al.
Proton Beam Energy Deposition as a Mechanism of Deep Photospheric Heating49017 March 2025Samuel GRANOVSKYAlexander KOSOVICHEV
New insights into the proton precipitation sites in solar flares48910 February 2025Andrea Francesco BATTAGLIASäm KRUCKER
Solar Gamma-Ray Evidence for a Distinct Population of MeV Flare-Accelerated Electrons48810 February 2025Gerry Share
From Chromospheric Evaporation to Coronal Rain: An Investigation of the Mass and Energy Cycle of a Flare4873 February 2025Seray ŞAHINPatrick ANTOLIN
Energetic neutral atoms detected in the large solar energetic particle event of February 202248620 January 2025Christina COHEN
Magnetic topology of quiet-Sun Ellerman bombs and associated ultraviolet brightenings4856 January 2025Aditi BHATNAGAR
Unveiling CME Dynamics: Rare Rotations of CMEs in the Heliosphere48430 December 2024Sandeep KUMARNandita SRIVASTAVA
Spatial and Spectral Evolution of Microwave and X-Ray Sources During the Limb Flare SOL2023-02-05483Julia N. SHAMSUTDINOVA
High-resolution observational analysis of flare ribbon fine structures482Jonas THOEN FABER
Advection and super-diffusive expansion as the model of flare accelerated electron transport in type III solar radio bursts481Eduard KONTARFrancesco AZZOLLINI, Olena LYUBCHYK
Faraday's Law in Solar Flares: A Cautionary Message480Michael FARADAY
Remarkable NUV Spectrum of an M-star Megaflare479Adam KOWALSKI
Revised Point-Spread Functions of AIA and their effect on DEM analyses478Stefan HOFMEISTER,Daniel Wolf SAVIN, and Michael HAHN
How much of the energy in flare-accelerated electrons reaches the chromosphere?477M. ALAOUIG. HOLMAN
Spatially resolved plasma composition evolution in a solar flare476Andy S. H. TO et al.
HOPE during high activity475Hugh HUDSONAlphonse STERLING
Simulated heliospheric electron spectra show sensitivity to plasma properties of a source region in the flaring corona474Ross PALLISTERNatasha JEFFREY
An extremely complex active region with very strong non-neutralized electric currents47314 October 2024Ioannis KONTOGIANNIS
An X9 flare and its huge crochet (SFE)4727 October 2024Hugh HUDSON
An X9.9 flare and its huge crochet (SFE)4727 October 2024Hugh HUDSON
All microflares that accelerate electrons to high energies are rooted in sunspots47130 September 2024Andrea Francesco BATTAGLIA
The warm-target model and kappa distributions47016 September 2024Yingjie LUO
Is there HOPE for Hyder flares...46818 March 2024Hugh HUDSON
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/EVE46719 February 2024Takato OTSU
... further results
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