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New TGFs Found in the RHESSI Data	New Views of Global Solar Magnetic Field Evolution Over Four Solar Cycles	No Hard X-rays from Comet Lovejoy
Non-Maxwellian Diagnostics from SDO/EVE Spectra of an X-class Flare	Non-radial jets on the edges of active regions	Non-thermal recombination in solar flares and microflares
Nonequilibrium Ionization of Flare Plasma Observed by Hinode/EIS	Novel X-ray Spectrograms	NuSTAR Observations of 11 Microflares
NuSTAR detects X-ray flares in the quiet Sun	Nugget 100	OSPEX Documentation
OSPEX GUI Users Guide	OSPEX Users Guide	Observation of Cosmic Ray Spallation Events from SoHO
Observational evidence for breakout reconnection	Observing Solar Flare X-ray Polarization with Prospective CubeSat Missions	Observing the Crab Nebula
Octupolar out-of-plane magnetic field structure generation during magnetic reconnection	Offpointing	Oft and Hard X-rays, Flares, and the Corona
On the Correlation of HXR and WL Emission in Solar Flares	One small step for a photon...	OngoingProblems
Ongoing Issues	Ongoing Problems	Ops Meeting Presentations
Other Discoveries from Carrington's Flare	PFSS, SEPs, and RHESSI	Parameterized Flare Models with Chromospheric Compressions
Partial Segmentation and Splitting of the Annihilation Line	Particle Acceleration due to a Plasmoid-Looptop Collision	Particle Acceleration in Two Coronal Jets
Passages of Electron Beams	Passes	Peristaltic Shocks: a model
Persistent Quasi-Periodic Pulsations Detected During the Large X8.2 Solar Flare	Pervasive Faint Fe XIX: Evidence for Nanoflare Heating	Phenomena in the unusually long pre-impulsive phase of SOL2011-06-07
Photospheric Electric Fields and Energy Fluxes in the Eruptive Active Region NOAA 11158	Photospheric Temperature Gradient	Photospheric response to a flare
Pierre Kaufmann	Pileup mod - Pseudo function for correcting pileup	Pixon
Pixon Results Summary	Plot Objects	Post 2016 Anneal Detector Operations
Pre-impulsive and Impulsive Phases of the March 28, 2022 Sub-Terahertz Flare	Precise timing of flare footpoint sources from mid-infrared observations	Prediction of Solar Cycle 25
PrepServer Architecture	PrepServer Documentation	PrepServer Installation Instructions
PrepServer Maintenance and Diagnostic	Probing chromospheric current sheets using SST and ALMA co-observations	Probing the solar coronal heating function with slow magnetoacoustic waves
Python	Quantum of Solar	Quasi-Periodic Pulsations: Fermi/GBM Results
Quasi-periodic pulsations as indicators of oscillatory processes in solar flares	Quiet Sun III	RHESSI
RHESSI's 15th Anniversary	RHESSI's 5th Anneal	RHESSI's Anneal Adventure
RHESSI's Re-entry	RHESSI's Tenth Anniversary	RHESSI, Hinode, and Spin
RHESSI - Concept to Fruition	RHESSI Catches Gamma-Ray Bursts	RHESSI Deep Integrations
RHESSI Detection of X-ray Emission from a Quiet-Sun Filament Eruption	RHESSI Detector Channel vs Energy	RHESSI GUI Guide
RHESSI Imaging	RHESSI Imaging on Short Timescales	RHESSI Major Events
RHESSI Microflare List	RHESSI Nugget Event List	RHESSI Nugget List
RHESSI Nugget Subject List	RHESSI Optical Images	RHESSI Resumes Observations
RHESSI Science Nuggets	RHESSI Science Nuggets/Quiet Sun III	RHESSI Science Nuggets 100 to 199
RHESSI Science Nuggets 200 to 299	RHESSI Simulations of Complicated Flares	RHESSI Software
RHESSI Spectroscopy - OSPEX User Guide	RHESSI Visibilities	RHESSI Workshop 9
RHESSI Workshop Series	RHESSI and General Relativity	RHESSI and IRIS
RHESSI and Type III Radio Bursts	RHESSI and quasi-periodic pulsations	RHESSI and submillimeter waves
RHESSI and tether-cutting	RHESSI and the Megamovie	RHESSI and the Transit of Venus I
RHESSI and the Wilson effect	RHESSI has resumed operations	RHESSI in Cycle 24
RHESSI is Annealing Now	RHESSI microflares - Flare Cartoons and Reality	RHESSI observes a magnetar
Radiation damage	Radio Emissions from Double RHESSI TGFs	Radio polarization signatures in twisted flare loops
Rapid variations of Si IV spectra in a flare observed by IRIS at a sub-second cadence	Reflection of Coronal Global Waves	Rejuvenating Solar Flare Termination Shocks as Particle Accelerators
Relation of Non-neutralized electric currents and the activity in active regions	Relative and (maybe) Absolute RHESSI Detector Efficiency: 2002-2008	Remembering John Brown
Remembering Marcos Machado via his research	Resolution	Resolving two distinct thermal X-ray components in a compound solar flare
Return-current Model Spectra and Enhanced Plasma Resistivity	Return currents and soft-hard-soft spectral evolution	Reuven Ramaty High Energy Solar Spectroscopic Imager
Revisiting the SHH and SEP Link	Ribbon-like hard X-ray source	Richard Schwartz
Roll Angle System	Rotational Phases of Stellar Flares	SDO EVE Flare Observation
SEPs Link not Confirmed	SOL2013-11-10 Eruptive Circular-ribbon Flare with Extended Remote Brightenings	SOL2017-09-04 (M5.5) 2017 as a Source of Relativistic Electrons and Protons
SPD 2009	SSR	STEREO observations of flares and their associations with CMEs
STEREO observed stealth CME	STIX, the Hard X-Ray Telescope on board Solar Orbiter	Sandbox
Saturation of Nonthermal Hard X-ray Emission in Solar Flares	Scattered Light: Inverse Compton Scattering and Coronal Hard X-ray Sources	Scattering Polarization in Solar Flares
Science Objectives	Science Questions	Scratch Pad
Search for a Flare Anticipation Index (FAI)	Searching SOLfully within the Nuggets	Sector Boundaries and RHESSI Flares
Selecting Background for RHESSI Spectra	Self-Consistent Flare Model	Short-Period Waves
Show synop	Simulating Images	Simulation Control Parameters
Sixty-Five Years of Solar Radioastronomy	Slow Magnetoacoustic Waves in Two-Ribbon Flares	Slowly but surely towards the huge amount of energy I
Slowly but surely towards the huge amount of energy II	Small is steep	Soft-Hard-Harder
Soft X-ray emission in kink-unstable coronal loops	Soft and Hard X-rays, Flares, and the Corona	Solar Aspect System
Solar Cosmic Rays, Neutrons, and Fermi Gamma-Rays	Solar Cosmic Rays of the GLE on 20 January 2005	Solar Cycle 24
Solar Cycle 24 BCHIJ	Solar Cycle 24 Group B	Solar Cycle 24 Group C
Solar Cycle 24 Group E	Solar Cycle 24 Group F	Solar Cycle 24 Group G
Solar Cycle 24 Group H	Solar Cycle 24 Group I	Solar Cycle 24 Intro
Solar Cycle 24 at hand!	Solar Electron Events	Solar Hard X-ray Albedo
Solar Hard X-rays with Insight	Solar Max Arrives	Solar Physics during the March 2015 Solar Eclipse
Solar X-rays from axions	Solar effects in the local interstellar medium	Solar energetic electron events over one solar cycle
Solar flare hard X-rays from the anchor points of an eruptive filament	Solar flare neutrons observed on the ground and in space	Solar flares: evaporation and simulation
Solar radiation belts?	Spacecraft Bus	Spatial Distribution of Magnetic Reconnection Rate in an M6.5 Solar Flare
Spatio-Temporal Dynamics of Flare Hard X-ray Pulsations	Spectral Evolution in Stochastic Acceleration Models	Spectropolarimetric Insight into Plasma-Sheet Dynamics of a Solar Flare
Spectroscopy - OSPEX User Guide	Spotlessness returns	Statistical Link Between Electrons Emitting X-rays and Type III Radio Bursts
Statistical study of Type III bursts and associated HXR emissions	Stealth Coronal Mass Ejections from Active Regions	Stellar Flares and Starspots
Stereoscopic Flares and CMEs	Submerged Flare Acoustic Sources	Submillimeter Radiation as the Thermal Component of the Neupert Effect
Subsecond Spikes in Solar Flare X-ray Flux as Seen by Fermi GBM	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	Sun-as-a-star spectroscopic observations of the line-of-sight velocity of a solar eruption on October 28, 2021
Sunquakes: Seismic Transients from Solar Flares	Sunspot Differential Rotation in an X-class Flare	Suppression of Hydrogen Emission in an X-class White-light Solar Flare
Supra-Arcade Downflows	Suzaku Microflares	Syrovatskii's "constant density" approximation
TeV Gamma rays from the Quiescent Sun	Tecumseh's Eclipse and Astrophysics	Temp
Temporal and Spatial Characteristics of Hard X-Ray Sources in Flare Model with Vertical Current Sheet	Test-2020-09-11	Test-20201018
TestSMW	Test https://	Testing Semantic Search
The "Last Best" Flares	The 15.11 MeV Gamma-ray Line Detected?	The 1859 Space Weather Event Revisited
The 3D standard model for eruptive flares	The Alfven Speed above a Sunspot, and Gamma-rays	The Balmer continuum observed from IRIS!
The Cosmic-Ray Shadow and Coronal Magnetism	The Curious First Sunquake of Solar Cycle 25	The Evaporating Sun
The Fastest Flare	The Fe and Fe/Ni line features I	The Fe and Fe/Ni line features II
The Flare that Time Forgot	The Flares of the RHESSI Monograph	The Formation of Kappa Distributions in Solar Flares
The Gamma-Ray Imager/Polarimeter for Solar flares (GRIPS)	The Good Guys and the Rascals	The Greatest GOES Flares
The HEROES Mission: High Energy Replicated Optics to Explore the Sun	The Halloween Flares and Large-Scale Correlations	The IAU Solar Target Identifier - A Good Thing
The Interesting RHESSI/SAS Archive	The Jakimiec Diagnostic Diagram	The Jakimiec Track
The Kelvin Force and Loop-Top Concentration	The Last Best Flare of Cycle 24?	The Low-High-Low Starting Frequency Trend in Groups of Type III Bursts
The M5.5 Solar Flare on September 4, 2017 as a Source of Relativistic Electrons and Protons	The McClymont Jerk	The Morphology of Flare Time Profiles
The Neupert Effect Revisited	The Next Generation - FOXSI	The Post-Burst Increase
The Power of Turbulence	The RHESSI Flare Catalog	The RHESSI fifth anniversary: X-flares persist!
The Redistribution of Nonthermal Electron Energy	The Rise and Fall of The Low Energy Cut Off	The Slowest Flare
The Solar X-ray Limb II	The Solar X-ray Limb III	The SphinX Instrument on CORONAS-PHOTON
The Superflare SOL2017-09-06: from submm to mid-IR	The Temporal and Spatial Extension of Gamma-ray Emission from the Sun	The X-ray Limb
The coronal magnetic field 1	The flight of FOXSI-3	The microflare Height Distribution
The true dawn of multimessenger astronomy	Thermal/Nonthermal with MinXSS and RHESSI	Thermal X-ray Continuum - Free-Free or Free-Bound?
Thick2 - Thick Target Bremsstrahlung Version 2	Thick - Thick Target Bremsstrahlung	Thin - Thin Target Bremsstrahlung
Thoban Schedule	Thomson scattering near sunspots	Three-phase life leads to corpulent X-ray loops
Three is company	Threshold conversions	Thunderstruck
Time Profiles of Solar Flare Densities	Time delay between HXR and Gamma-rays	Tips and Resources
ToBeOrNotToBe	ToBeOrNotToBeThatIsThe?	To Beam or not to beam - that is (still) the question
To be or not to be - the role of projection effects in EUV imaging	To beam or not to beam - that is (still) the question	Tohabn Report 2009-07-01
Tohabn Report 2009-08-05	Tohban	TohbanReport2002-03-01
Tohban Links	Tohban Report 2002-03-01	Tohban Report 2008-10-01
Tohban Report 2008-10-15	Tohban Report 2008-10-22	Tohban Report 2008-10-28
Tohban Report 2008-10-29	Tohban Report 2008-11-05	Tohban Report 2008-11-12
Tohban Report 2008-11-19	Tohban Report 2008-11-26	Tohban Report 2008-12-03
Tohban Report 2008-12-10	Tohban Report 2008-12-17	Tohban Report 2008-12-24
Tohban Report 2009-01-14	Tohban Report 2009-01-21	Tohban Report 2009-02-04
Tohban Report 2009-02-11	Tohban Report 2009-02-18	Tohban Report 2009-02-25
Tohban Report 2009-03-04	Tohban Report 2009-03-11	Tohban Report 2009-03-18
Tohban Report 2009-03-25	Tohban Report 2009-04-01	Tohban Report 2009-04-15
Tohban Report 2009-04-22	Tohban Report 2009-04-29	Tohban Report 2009-05-13
Tohban Report 2009-05-20	Tohban Report 2009-05-27	Tohban Report 2009-06-10
Tohban Report 2009-06-17	Tohban Report 2009-06-24	Tohban Report 2009-07-01
Tohban Report 2009-07-08	Tohban Report 2009-07-15	Tohban Report 2009-07-22
Tohban Report 2009-07-29	Tohban Report 2009-08-05	Tohban Report 2009-08-12
Tohban Report 2009-08-19	Tohban Report 2009-08-26	Tohban Report 2009-09-30
Tohban Report 2009-10-07	Tohban Report 2009-10-14	Tohban Report 2009-10-21
Tohban Report 2009-10-28	Tohban Report 2009-11-04	Tohban Report 2009-11-10
Tohban Report 2009-11-18	Tohban Report 2009-11-25	Tohban Report 2009-12-02