RHESSI Nugget List: Difference between revisions

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Latest revision as of 04:44, 30 November 2010

 RHESSI Nugget IndexRHESSI Nugget DateRHESSI Nugget First AuthorRHESSI Nugget Second Author
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
Unexpected Asymmetry in GeV Emission46615 January 2024Bruno ARSIOLI and Elena ORLANDO
When it rippled in one place and exploded in another46525 December 2023Ivan ZIMOVETS
Solar flares: evaporation and simulation46418 December 2023Malcolm DRUETT
Pre-impulsive and Impulsive Phases of the March 28, 2022 Sub-Terahertz Flare46311 December 2023Galina G. MOTORINA
Coronal Bright Points46227 November 2023Daniel Nóbrega-Siverio
Aurora-like Radio Emission from a Sunspot46120 November 2023Sijie YU
Search for a Flare Anticipation Index (FAI)46013 November 2023Hugh HUDSONJim McTIERNAN
Bouncing motions of fast electrons using Nobeyama Radioheliograph4596 November 2023Keitarou MATSUMOTO
Impact of nanoflare heating in the lower solar atmosphere45830 October 2023Helle BAKKE
Precise timing of flare footpoint sources from mid-infrared observations45723 October 2023Paulo SIMÕES et al.
... further results
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