Solar Physics

Papers
(The median citation count of Solar Physics is 2. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2020-04-01 to 2024-04-01.)
ArticleCitations
The Daniel K. Inouye Solar Telescope – Observatory Overview155
Progress in Solar Cycle Predictions: Sunspot Cycles 24–25 in Perspective77
Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)64
Overlapping Magnetic Activity Cycles and the Sunspot Number: Forecasting Sunspot Cycle 25 Amplitude55
A New View of the Solar Interface Region from the Interface Region Imaging Spectrograph (IRIS)51
Forecasting Solar Cycle 25 Using Deep Neural Networks39
ICME Evolution in the Inner Heliosphere36
On the Prediction of Solar Cycles32
EMD and LSTM Hybrid Deep Learning Model for Predicting Sunspot Number Time Series with a Cyclic Pattern31
Upflows in the Upper Solar Atmosphere27
Recalibration of the Sunspot-Number: Status Report25
Weakest Solar Cycle of the Space Age: A Study on Solar Wind–Magnetosphere Energy Coupling and Geomagnetic Activity25
Role of Compressive Viscosity and Thermal Conductivity on the Damping of Slow Waves in Coronal Loops with and Without Heating–Cooling Imbalance22
Dispersion of Slow Magnetoacoustic Waves in the Active Region Fan Loops Introduced by Thermal Misbalance22
Forecasting of Sunspot Time Series Using a Hybridization of ARIMA, ETS and SVM Methods21
Extreme Space-Weather Events and the Solar Cycle21
Shaken and Stirred: When Bond Meets Suess–de Vries and Gnevyshev–Ohl21
The Visible Spectro-Polarimeter of the Daniel K. Inouye Solar Telescope21
Solar X-Ray Monitor on Board the Chandrayaan-2 Orbiter: In-Flight Performance and Science Prospects21
Probabilistic Drag-Based Ensemble Model (DBEM) Evaluation for Heliospheric Propagation of CMEs20
High-Resolution Spectral and Anisotropy Characteristics of Solar Protons During the GLE N∘73 on 28 October 2021 Derived with Neutron-Monitor Data Analysis20
Robustness of Solar-Cycle Empirical Rules Across Different Series Including an Updated Active-Day Fraction (ADF) Sunspot Group Series20
Time Lag Between Cosmic-Ray and Solar Variability: Sunspot Numbers and Open Solar Magnetic Flux19
On the Radial and Longitudinal Variation of a Magnetic Cloud: ACE, Wind, ARTEMIS and Juno Observations19
Randomness in Sunspot Number: A Clue to Predict Solar Cycle 2519
CNN-Based Deep Learning Model for Solar Wind Forecasting19
Coronal Photopolarimetry with the LASCO-C2 Coronagraph over 24 Years [1996 – 2019]19
Mixed Properties of Slow Magnetoacoustic and Entropy Waves in a Plasma with Heating/Cooling Misbalance19
Coronal Quasi-periodic Fast-mode Propagating Wave Trains19
The STIX Aspect System (SAS): The Optical Aspect System of the Spectrometer/Telescope for Imaging X-Rays (STIX) on Solar Orbiter19
How Good Is the Bipolar Approximation of Active Regions for Surface Flux Transport?18
Evolution of Coronal Mass Ejections and the Corresponding Forbush Decreases: Modeling vs. Multi-Spacecraft Observations18
Development of a Confined Circular-Cum-Parallel Ribbon Flare and Associated Pre-Flare Activity18
Prediction of Amplitude and Timing of Solar Cycle 2517
GLE # 67 Event on 2 November 2003: An Analysis of the Spectral and Anisotropy Characteristics Using Verified Yield Function and Detrended Neutron Monitor Data17
Empirical Model of 10 – 130 MeV Solar Energetic Particle Spectra at 1 AU Based on Coronal Mass Ejection Speed and Direction17
The Evolution of Coronal Holes over Three Solar Cycles Using the McIntosh Archive17
Science Highlights and Final Updates from 17 Years of Total Solar Irradiance Measurements from the SOlar Radiation and Climate Experiment/Total Irradiance Monitor (SORCE/TIM)16
On the Expansion Speed of Coronal Mass Ejections: Implications for Self-Similar Evolution16
Assessing the Predictability of Solar Energetic Particles with the Use of Machine Learning Techniques16
Solar Flare Effects on the Earth’s Lower Ionosphere16
CME-Driven and Flare-Ignited Fast Magnetosonic Waves Detected in a Solar Eruption16
Effect of Thermal Conductivity, Compressive Viscosity and Radiative Cooling on the Phase Shift of Propagating Slow Waves with and Without Heating–Cooling Imbalance15
Propagating Conditions and the Time of ICME Arrival: A Comparison of the Effective Acceleration Model with ENLIL and DBEM Models15
Overview of the Solar Radiation and Climate Experiment (SORCE) Seventeen-Year Mission15
Predicting the Amplitude of Solar Cycle 25 Using the Value 39 Months Before the Solar Minimum15
Three-Dimensional Simulations of Solar Wind Preconditioning and the 23 July 2012 Interplanetary Coronal Mass Ejection15
Role of Non-ideal Dissipation with Heating–Cooling Misbalance on the Phase Shifts of Standing Slow Magnetohydrodynamic Waves14
Active Region Contributions to the Solar Wind over Multiple Solar Cycles14
Solar-Cycle Variability Results from the Solar Radiation and Climate Experiment (SORCE) Mission14
Solar-Cycle Characteristics in Kodaikanal Sunspot Area: North–South Asymmetry, Phase Distribution and Gnevyshev Gap14
Sunspot Positions and Areas from Observations by Cigoli, Galilei, Cologna, Scheiner, and Colonna in 1612 – 161414
First Hard X-Ray Imaging Results by Solar Orbiter STIX14
Transverse Coronal-Loop Oscillations Induced by the Non-radial Eruption of a Magnetic Flux Rope14
Ring of Stations Method in Cosmic Rays Variations Research14
Temporal and Periodic Variation of the MCMESI for the Last Two Solar Cycles; Comparison with the Number of Different Class X-ray Solar Flares13
Coronal Elemental Abundance: New Results from Soft X-Ray Spectroscopy of the Sun13
Group Sunspot Numbers: A New Reconstruction of Sunspot Activity Variations from Historical Sunspot Records Using Algorithms from Machine Learning13
Corotating Interaction Regions during Solar Cycle 24: A Study on Characteristics and Geoeffectiveness13
Short-Term Periodicities Observed in Neutron Monitor Counting Rates13
Predicting the Shape of Solar Cycle 25 Using a Similar-Cycle Method13
Distinguishing the Rigidity Dependences of Acceleration and Transport in Solar Energetic Particles13
Analysis of Large Deflections of Prominence–CME Events during the Rising Phase of Solar Cycle 2413
CMEs in the Heliosphere: III. A Statistical Analysis of the Kinematic Properties Derived from Stereoscopic Geometrical Modelling Techniques Applied to CMEs Detected in the Heliosphere from 2008 to 20113
Measurements of Solar Differential Rotation Using the Century Long Kodaikanal Sunspot Data13
Detections of Multi-Periodic Oscillations During a Circular Ribbon Flare13
In-flight Calibration and Data Reduction for the WISPR Instrument On Board the PSP Mission12
A Search for the Counterparts of Quiet-Sun Radio Transients in Extreme Ultraviolet Data12
The Balloon-Borne Investigation of Temperature and Speed of Electrons in the Corona (BITSE): Mission Description and Preliminary Results12
LASCO-C3 Observations of the K- and F-Coronae over 24 Years (1996 – 2019): Photopolarimetry and Electron Density Distribution12
About the Altitude Profile of the Atmospheric Cut-Off of Cosmic Rays: New Revised Assessment12
Trajectory Determination for Coronal Ejecta Observed by WISPR/Parker Solar Probe12
A Catalog of Bipolar Active Regions Violating the Hale Polarity Law, 1989 – 201812
Solar Cycle Dependence of ICME Composition12
Comparison of Geomagnetic Indices During Even and Odd Solar Cycles SC17 – SC24: Signatures of Gnevyshev Gap in Geomagnetic Activity12
Simulating the Coronal Evolution of Bipolar Active Regions to Investigate the Formation of Flux Ropes12
Transiting Exoplanet Survey Satellite (TESS) Observations of Flares and Quasi-Periodic Pulsations from Low-Mass Stars and Potential Impact on Exoplanets12
Investigation of the Middle Corona with SWAP and a Data-Driven Non-Potential Coronal Magnetic Field Model11
Coronal Electron Density Fluctuations Inferred from Akatsuki Spacecraft Radio Observations11
A Dynamo-Based Prediction of Solar Cycle 2511
Identifying Flux Rope Signatures Using a Deep Neural Network11
Tidally Synchronized Solar Dynamo: A Rebuttal11
Dependence of Great Geomagnetic Storm ($\Delta $SYM-H$\le -200$ nT) on Associated Solar Wind Parameters11
Invited Review: Short-term Variability with the Observations from the Helioseismic and Magnetic Imager (HMI) Onboard the Solar Dynamics Observatory (SDO): Insights into Flare Magnetism11
Solar Flare Forecasting Using Time Series and Extreme Gradient Boosting Ensembles11
The Advanced Space-Based Solar Observatory (ASO-S)11
Quasi-Periodic Pulsations Detected in Ly $\alpha $ and Nonthermal Emissions During Solar Flares11
A Statistical Study of Low-Frequency Solar Radio Type III Bursts11
Forward Synthesis of Polarized Emission in Target DKIST Coronal Lines Applied to 3D MURaM Coronal Simulations11
The Daniel K. Inouye Solar Telescope (DKIST)/Visible Broadband Imager (VBI)11
Kanzelhöhe Observatory: Instruments, Data Processing and Data Products10
Solar Wind Helium Abundance Heralds Solar Cycle Onset10
Statistical Approach on Differential Emission Measure of Coronal Holes using the CATCH Catalog10
Irradiance Variations of the Sun and Sun-Like Stars – Overview of Topical Collection10
On the Correlation between Energy Spectra and Element Abundances in Solar Energetic Particles10
A Simple Radial Gradient Filter for Batch-Processing of Coronagraph Images10
Solar Cycle 25 Prediction Using an Optimized Long Short-Term Memory Mode with F10.710
Predicting the Maximum Amplitude of Solar Cycle 25 Using the Early Value of the Rising Phase10
The Solar Event of 14 – 15 July 2012 and Its Geoeffectiveness10
Correlations of Sunspot Physical Characteristics during Solar Cycle 2310
Automated Detection of Accelerating Solar Eruptions Using Parabolic Hough Transform10
The Evolution over Time and North–South Asymmetry of Sunspots and Solar Plages for the Period 1910 to 1937 Using Data from Ebro Catalogues10
Imaging and Spectral Observations of a Type-II Radio Burst Revealing the Section of the CME-Driven Shock That Accelerates Electrons10
Solar Wind Plasma Particles Organized by the Flow Speed10
Deciphering Solar Magnetic Activity: 140 Years of the ‘Extended Solar Cycle’ – Mapping the Hale Cycle10
Two Classes of Eruptive Events During Solar Minimum10
Forecasting the Daily 10.7 cm Solar Radio Flux Using an Autoregressive Model10
Predicting Extreme Solar Flare Events Using Lu and Hamilton Avalanche Model10
Possible Signature of Sausage Waves in Photospheric Bright Points9
Calibrating GONG Magnetograms with End-to-End Instrument Simulation III: Comparison, Calibration, and Results9
Solar Event Detection Using Deep-Learning-Based Object Detection Methods9
Solar wind transient currents: statistical properties and impact on Earth’s magnetosphere9
Analysis of the Helical Kink Stability of Differently Twisted Magnetic Flux Ropes9
The Diffraction-Limited Near-Infrared Spectropolarimeter (DL-NIRSP) of the Daniel K. Inouye Solar Telescope (DKIST)9
Common Origin of Quasi-Periodic Pulsations in Microwave and Decimetric Solar Radio Bursts9
Multi-Wavelength Observations of Quasi-Periodic Pulsations in a Solar Flare9
Exploring the Circular Polarisation of Low–Frequency Solar Radio Bursts with LOFAR9
Investigation of the Hemispheric Asymmetry in Solar Flare Index During Solar Cycle 21 – 24 from the Kandilli Observatory9
Estimate of Plasma Temperatures Across a CME-Driven Shock from a Comparison Between EUV and Radio Data9
Magnetohydrodynamic Spectroscopy of a Non-adiabatic Solar Atmosphere9
Dependence of Major Geomagnetic Storm Intensity ($\mathrm{Dst}\le -100$ nT) on Associated Solar Wind Parameters9
Thermodynamic Structure of the Solar Corona: Tomographic Reconstructions and MHD Modeling9
Coherence of Coronal Mass Ejections in Near-Earth Space9
Identification and Extraction of Solar Radio Spikes Based on Deep Learning9
On the Possibility of Heating the Solar Corona by Heat Fluxes from Coronal Magnetic Structures8
Decayless Kink Oscillations Excited by Random Driving: Motion in Transitional Layer8
The Interconnection between the Periodicities of Solar Wind Parameters Based on the Interplanetary Magnetic Field Polarity (1967–2018): A Cross Wavelet Analysis8
Temporal and Spatial Scales in Coronal Rain Revealed by UV Imaging and Spectroscopic Observations8
Thermal Trigger for Solar Flares I: Fragmentation of the Preflare Current Layer8
Calibrating GONG Magnetograms with End-to-end Instrument Simulation I: Background, the GONG Instrument, and End-to-end Simulation8
SOLar-STellar Irradiance Comparison Experiment II (SOLSTICE II): End-of-Mission Validation of the SOLSTICE Technique8
DH Type II Radio Bursts During Solar Cycles 23 and 24: Frequency-Dependent Classification and Their Flare-CME Associations8
Long-Term Variations in Solar Activity: Predictions for Amplitude and North–South Asymmetry of Solar Cycle 258
Simulating White-Light Images of Coronal Structures for Parker Solar Probe/WISPR: Study of the Total Brightness Profiles8
Intense Geomagnetically Induced Currents (GICs): Association with Solar and Geomagnetic Activities7
Defining the Middle Corona7
Physical Characteristics of Umbral Dots Derived from a High-Resolution Observations7
Magnetic Field, Electron Density and Their Spatial Scales in Zebra Pattern Radio Sources7
Resonant Damping of Kink Modes in Solar Coronal Slabs7
Magnetic Reconnections in the Presence of Three-Dimensional Magnetic Nulls and Quasi-Separatrix Layers7
Long–Term Variations in Solar Differential Rotation and Sunspot Activity, II: Differential Rotation Around the Maxima and Minima of Solar Cycles 12 – 247
Analyses of Early Sunspot Records by Jean Tarde (1615 – 1617) and Jan Smogulecki (1621 – 1625)7
Thermal Trigger for Solar Flares II: Effect of the Guide Magnetic Field7
Automated Detection of Chromospheric Swirls Based on Their Morphological Characteristics7
Recalculation of the Wolf Series from 1877 to 18937
September 2017 Space-Weather Events: A Study on Magnetic Reconnection and Geoeffectiveness7
Thermal Misbalance Influence on the Nonlinear Shear Alfvén Waves Under Solar Atmosphere Conditions7
VLA Measurements of Faraday Rotation Through a Coronal Mass Ejection Using Multiple Lines of Sight7
Amplitude of the Observational Forbush Decreases in the Presence of Cosmic Ray Diurnal Anisotropy During High Solar Activity in 19727
Properties of High-Frequency Type II Radio Bursts and Their Relation to the Associated Coronal Mass Ejections7
Motion Magnification in Solar Imaging Data Sequences in the Sub-pixel Regime7
Properties and Energetics of Magnetic Reconnection: I. Evolution of Flare Ribbons7
A Modern Reconstruction of Richard Carrington’s Observations (1853–1861)7
Three-Dimensional Reconstructions of Coronal Wave Surfaces Using a New Mask-Fitting Method7
Revisiting the Amplitude of Solar Cycle 9: The Case of Sunspot Observations by W.C. Bond6
Undetected Minority-Polarity Flux as the Missing Link in Coronal Heating6
Estimating the Open Solar Flux from In-Situ Measurements6
A Geoeffective CME Caused by the Eruption of a Quiescent Prominence on 29 September 20136
Variation of Chromospheric Features as a Function of Latitude and Time Using Ca-K Spectroheliograms for Solar Cycles 15 – 23: Implications for Meridional Flow6
Flare Index Prediction with Machine Learning Algorithms6
Error Estimation of Linear Polarization Data from Coronagraphs – Application to STEREO-A/SECCHI-COR1 Observations6
Large-Scale Vortex Motion and Multiple Plasmoid Ejection Due to Twisting Prominence Threads and Associated Reconnection6
Longitudinal Plasma Motions Generated by Shear Alfvén Waves in Plasma with Thermal Misbalance6
Disambiguation of Vector Magnetograms by Stereoscopic Observations from the Solar Orbiter (SO)/Polarimetric and Helioseismic Imager (PHI) and the Solar Dynamic Observatory (SDO)/Helioseismic and Magne6
Solar Radiation and Climate Experiment (SORCE) X-Ray Photometer System (XPS): Final Data-Processing Algorithms6
The Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near-Infrared Spectro-Polarimeter6
Evidence Against Carbonization of the Thin-Film Filters of the Extreme Ultraviolet Variability Experiment Onboard the Solar Dynamics Observatory6
The First Survey of Quiet Sun Features Observed in Hard X-Rays with NuSTAR6
“Generative” Indices of Sunspot Solar Activity: 145-Year Composite Series6
Energy Partition in Four Confined Circular-Ribbon Flares6
Response to “Limitations in the Hilbert Transform Approach to Locating Solar Cycle Terminators” by R. Booth6
Energy Spectra vs. Element Abundances in Solar Energetic Particles and the Roles of Magnetic Reconnection and Shock Acceleration6
Coronal Elemental Abundances During A-Class Solar Flares Observed by Chandrayaan-2 XSM6
Properties of Type III and Type IIIb Bursts in the Frequency Band of 8 – 80 MHz During PSP Perihelion at the Beginning of April 20196
Long-Term Trend Analysis in the Solar Radiation and Climate Experiment (SORCE)/Spectral Irradiance Monitor (SIM)6
Sun-to-Earth Observations and Characteristics of Isolated Earth-Impacting Interplanetary Coronal Mass Ejections During 2008 – 20146
Solar Irradiance Variability Due to Solar Flares Observed in Lyman-Alpha Emission6
Working Principle of the Calibration Algorithm for High Dynamic Range Solar Imaging with the Square Kilometre Array Precursor6
Observation of the Solar Corona Using Radio Scintillation with the Akatsuki Spacecraft: Difference Between Fast and Slow Wind6
Calibrating GONG Magnetograms with End-to-End Instrument Simulation II: Theory of Calibration6
Characteristics of Suprathermal Electrons in Small-Scale Magnetic Flux Ropes and Their Implications on the Magnetic Connection to the Sun6
Long- and Short-Term Evolutions of Magnetic Field Fluctuations in High-Speed Streams6
Analysis of the Evolution of a Multi-Ribbon Flare and Failed Filament Eruption5
Model Fitting of Wind Magnetic Clouds for the Period 2004 – 20065
Comparison of Solar Wind Speed Estimates from Nearly Simultaneous IPS Observations at 327 and 111 MHz5
How to Estimate the Far-Side Open Flux Using STEREO Coronal Holes5
Extracting the Heliographic Coordinates of Coronal Rays Using Images from WISPR/Parker Solar Probe5
A New Tool for Predicting the Solar Cycle: Correlation Between Flux Transport at the Equator and the Poles5
An Optimization Principle for Computing Stationary MHD Equilibria with Solar Wind Flow5
Origin and Characteristics of the Southward Component of the Interplanetary Magnetic Field5
Relationships Between the Spectra of Near-Earth Proton Enhancements, Hard X-Ray Bursts, and CME Speeds5
White-Light Coronal Imaging at the 21 August 2017 Total Solar Eclipse5
The Effect of Thermal Misbalance on Slow Magnetoacoustic Waves in a Partially Ionized Prominence-Like Plasma5
Solar Wind Discontinuity Interaction with the Bow Shock: Current Density Growth and Dawn-Dusk Asymmetry5
A Reanalysis of the Number of Sunspot Groups Recorded by Pierre Gassendi in the Cycle Before the Maunder Minimum5
Thermal Trigger for Solar Flares III: Effect of the Oblique Layer Fragmentation5
A Review of the Extended EUV Corona Observed by the Sun Watcher with Active Pixels and Image Processing (SWAP) Instrument5
Limitations in the Hilbert Transform Approach to Locating Solar Cycle Terminators5
Separating the aa-index into Solar and Hale Cycle Related Components Using Principal Component Analysis5
A Critical Comment on “Can Solar Cycle 25 Be a New Dalton Minimum?”5
On the Magnetoacoustic Waves and Physical Conditions in Zebra Radio Sources5
Source Locations and Solar-Cycle Distribution of the Major Geomagnetic Storms ($\mathrm{Dst} \le -100$ nT) from 1932 to 20185
Nonaxisymmetric Component of Solar Activity: the Vector of the Longitudinal Asymmetry5
A Survey of Computational Tools in Solar Physics5
Quasi-Periodic Energy Release in a Three-Ribbon Solar Flare5
Forecasting Solar Cycle 25 with Physical Model-Validated Recurrent Neural Networks5
HATS: A Ground-Based Telescope to Explore the THz Domain5
On the Reflection of Torsional Alfvén Waves from the Solar Transition Region5
Polarization of the Corona Observed During the 2017 and 2019 Total Solar Eclipses5
Dark Dots on the Photosphere and Their Counting in the Sunspot Index5
Equation of State of the Kappa-Distributed Solar Wind Particles in the Earth’s Magnetopause5
Type-III Electron Beams: 3D Quasilinear Effects5
Relationships between Interplanetary Coronal Mass Ejection Characteristics and Geoeffectiveness in the Declining Phase of Solar Cycles 23 and 245
Rapid Rotation of an Erupting Prominence and the Associated Coronal Mass Ejection on 13 May 20135
Occurrence Rate of Radio-Loud and Halo CMEs in Solar Cycle 25: Prediction Using their Correlation with the Sunspot Number5
Johann Christoph Müller’s Sunspot Observations in 1719 – 1720: Snapshots of the Immediate Aftermath of the Maunder Minimum5
The Shape of Sunspots and Solar Activity Cycles5
Solar Cycle Pairing and Prediction of Cycle 255
Optimal Fitting of the Freidberg Solution to In Situ Spacecraft Measurements of Magnetic Clouds5
Degradation Correction of TSIS SIM5
Response to Comment on “Tidally Synchronized Solar Dynamo: A Rebuttal”4
Scale Transfer in 1849: Heinrich Schwabe to Rudolf Wolf4
Solar Soft X-ray Irradiance Variability, I: Segmentation of Hinode/XRT Full-Disk Images and Comparison with GOES (1 – 8 Å) X-Ray Flux4
Long-Term Evolution of the Solar Corona Using PROBA2 Data4
Image Desaturation for SDO/AIA Using Deep Learning4
Small Size Ground Level Enhancements During Solar Cycle 244
Center–Limb Variation of Solar Photospheric Microturbulence4
Reconstruction of the Sunspot Number Source Database and the 1947 Zurich Discontinuity4
Aurora Observations from the Principality of Transylvania from the 16th to the 18th Century CE4
The Possible Cause of Most Intense Geomagnetic Superstorm of the 21st Century on 20 November 20034
Solar Type U Burst Associated with a High Coronal Loop4
Solar Energetic-Particle Ground-Level Enhancements and the Solar Cycle4
Two-Stage Evolution of an Extended C-Class Eruptive Flaring Activity from Sigmoid Active Region NOAA 12734: SDO and Udaipur-CALLISTO Observations4
Solar 11-Year Cycle Signal in Stratospheric Nitrogen Dioxide—Similarities and Discrepancies Between Model and NDACC Observations4
On the Relationship Between the Transit Time of ICMEs and Strength of the Initiated Geomagnetic Storms4
On Identifying and Mitigating Bias in Inferred Measurements for Solar Vector Magnetic-Field Data4
Comment on “Tidally Synchronized Solar Dynamo: A Rebuttal” by Nataf (Solar Phys. 297, 107, 2022)4
Near-Earth Interplanetary Coronal Mass Ejections and Their Association with DH Type II Radio Bursts During Solar Cycles 23 and 244
Observation of Alfvén Waves in an ICME-HSS Interaction Region4
Subsurface Horizontal Flows During Solar Cycles 24 and 25 with Large-Tile Ring-Diagram Analysis4
A Theoretical Estimate of the Pole-Equator Temperature Difference and a Possible Origin of the Near-Surface Shear Layer4
Rate of Change of Large-Scale Solar-Wind Structure4
Solar-Wind High-Speed Stream (HSS) Alfvén Wave Fluctuations at High Heliospheric Latitudes: Ulysses Observations During Two Solar-Cycle Minima4
Formation of Isolated Radio Type II Bursts at Low Frequencies4
On the Hemispheric Bias Seen in Vector Magnetic Field Data4
Propagating Oscillations in the Lower Atmosphere Under Coronal Holes4
Can Solar Cycle 25 Be a New Dalton Minimum?4
Statistical Analysis of Interplanetary Shocks from Mercury to Jupiter4
Probing Upflowing Regions in the Quiet Sun and Coronal Holes4
Multiwavelength Observations of a Partial Filament Eruption on 13 June 20114
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