National Solar Observatory, Sunspot New Mexico

    flowchart
    I[National Solar Observatory, Sunspot New Mexico]
    PI["Parent Institutions (1)"]
    CI["Child Institutions (0)"]
    AW["Affiliated Works (285)"]
    CA["Linked Collaborating Authors (134)"]
    I== skos:broader ==>PI
    CI== skos:broader ==>I
    AW== affil ==>I
    AW== author ==>CA
    click PI "#parent-institutions"
    click CI "#child-institutions"
    click AW "#affiliated-works"
    click CA "#collaborating-authors"

ADS ID [?]

A03667

Abbreviation [?]

NSO

Parent Institutions [?]

• Association of Universities for Research in Astronomy, Washington DC

Child Institutions [?]

Affiliated Works

sorted by decreasing year, and then by display-name

• The Impact of NPOESS on Mesoscale Forecasts
• Current Helicity of Emerging Active Regions
• Long-Term Solar Irradiance Variations From Solar Cycle 21 to 23
• Multi-wavelength Structure of an Active Region Filament
• The Right Amount of Glue: Technologies and Standards Relevant to a Future Solar-Terrestrial Data Environment
• CoSEC: Orchestrated Web Services for Living with a Star
• Coronal Radio Magnetography of Solar Active Region 8365
• DASL--Data and Activities for Solar Learning
• Data Integration in the Virtual Solar Observatory
• Diagnostics of the Solar Coronal Magnetic Field: 1878 - 2010
• First Results from SOLIS
• Solar Astronomy as a Means to Promote Authentic Science Research in a Teacher Professional Development Program
• Synergy of Research and EPO Programs at NSO
• The Virtual Solar Observatory -- the Why, What, How and Where
• Virtual Solar Observatory Distributed Query Construction
• Doing Science with the VSO: Signatures of CME Initiation
• Mapping the Velocity Distribution of Neutral Sodium Near Io
• Solar Torsional Oscillations and the Extended Solar Cycle
• Solving Science Use Cases that relate to the Sun and Heliosphere with EGSO
• Temporal Variations in the Evershed Flow
• Case Study of A Sequential Chromospheric Brightening (SCB) Associated with May 6, 2005 event.
• High Resolution Optical Spectroscopy, Spectropolarimetry and Spectral Imaging of Filament and Flaring Atmospheres
• ISOON H-alpha Survey of Sequential Chromospheric Brightenings
• My Teacher got a Trip to Kitt Peak Observatory, but all I got was This Lousy Data CD: Lessons Learned in Optimizing a Teacher Professional Development Program for Solar Research
• Bayesian Feature Recognition for Multidimensional NSO Imagery
• Enchancements to the Virtual Solar Observatory
• Multiwavelength Study of Flow Fields in Flaring Super Active Region NOAA 10486
• The Virtual Solar Observatory and the Heliophysics Meta-Virtual Observatory
• The current and future roles of virtual observatories serving the heliophysical data environment
• Alfven Waves in the Solar Corona
• Application of Statistical Image Segmentation to Recognition of Solar Magnetic Network
• Callable Virtual Observatory Functionality: Sample Use Cases
• Dealing with Large Dataset Queries in the Virtual Solar Observatory
• Design Considerations for Data Catalogs
• GONG Synoptic Magnetograms and Coronal Magnetic Field Modeling
• Mexican Virtual Solar Observatory
• SOLIS: status, data products & science
• Sources of fast solar wind streams observed on STEREO and at L1
• Sunspot Numbers and Sunspot Irradiance Reductions as Obtained with OSPAN Semi- automatic Analysis
• The Magnetic Structure of X-Ray Bright Points
• A Magnetohydrodynamic (MHD) Analyses of Energy and Magnetic flux Transport from Sub-photosphere to the Corona
• Comparison of Exospheric Observations by the Mercury Atmospheric and Surface Composition Spectrometer during the First and Second MESSENGER Flybys with Concurrent Ground-based Observations
• Dynamics of Quiet Solar Chromosphere at the Limb
• Polar Magnetic Field Distribution as Observed by SOLIS and its relation with coronal structures
• Recent studies of the behavior of the Sun's white-light corona over time
• STEREO ICMEs and their Solar Source Regions Near Solar Minimum
• Spectral Irradiance Variations and Magnetic Field Changes During Solar Cycle 23.
• The Role of Heavy Ions as Coronal Diagnostics: Recent Results from Total Solar Eclipse Observations
• The Whole Heliosphere Interval: Campaign Summaries and Early Results
• The application of Gaussian Mixture and Histogram-based Bayesian methods to NSO/Kitt Peak VT data.
• The dynamic lunar exosphere: clues from sodium
• Understanding and forecasting solar EUV and UV irradiance variations
• Variations in Mercury's Sodium Exosphere Taken at the McMath-Pierce Solar Telescope in January 2008 in Support of the MESSENGER Flybys
• What Are We Tracking ... and Why?
• Automated Characterization of Sequential Chromospheric Brightenings
• Enabling Distributed access to SDO Data with VSO
• Large-Scale Solar Subsurface Flows During Solar Cycle Minimum
• New Global Solar Magnetic Field Maps Using the ADAPT Data Assimilation and Flux Transport Model
• Observations of Metallic Species in Mercury’s Exosphere During the Three MESSENGER Flybys
• Recent Progress in Detecting Meridional Flows Deep within the Sun
• Reconstructing the 3-D Structure and Trajectory of ICMEs: Physical and Forecasting Implications
• Simulations of the Evolution of Vapor Ejected by the LCROSS Impact on the Moon
• The Advanced Technology Solar Telescope: Science Goals, Design and Project Status. (Invited)
• The Torsional Oscillation and the Solar Minimum
• The VSO Interface to SDO Data - On Top and Underneath
• The Variation of Solar Chromospheric H-alpha Plage 2002-2009
• The internal dynamics and magnetism of the sun -- the perspective from global helioseismology (Invited)
• Using subsurface helicity measurements to predict flare occurrence
• Vorticity of Granular Flows from NST Observations
• Coronal Mass Ejections from Empty Filament Channels
• Development of a Statistical Diagnostic Scheme for Flare Probability
• End-to-End Observations and Modeling of the 17-21 January 2010 CME/ICME
• Ensemble Solar Global Magnetic Field Modeling
• Evolution of magnetic field in flaring active regions
• Forecasting Earth Arrivals of CMEs with Heliospheric Imagers (Invited)
• Forecasting Solar EUV Irradiance, Validation and Automation
• Global and Local Helioseismology from HMI and AIA
• Helioseismic Studies of a Sunspot using HMI Data
• Improving the Far-Side Seismic Maps
• Magnetic Field Measurements at the Photosphere and Coronal Base
• Non-polar Coronal Holes and Solar Wind
• Photospheric synoptic magnetograms, potential-field models and observed global coronal structure
• Predictions of active region flaring probability using subsurface helicity measurements
• Scientific Revelations on Coronal Mass Ejections Using Heliospheric Imagers and In-Situ Data
• Solar Dynamo: Comparing Models with Observations. (Invited)
• Solar Subsurface Flows derived with Ring-Diagram Analysis
• Subsurface Flows from SDO, SOHO, and GONG (Invited)
• The Flare Patrol Augmentation Tool (FPAT)
• The Impact of Different Global Photospheric Magnetic Field Maps on Coronal Models
• The automatic detection and tracking of interplanetary coronal mass ejections (CMEs) using heliospheric imager data
• WSA Derived Coronal Hole Comparison with STEREO EUVI Observations
• What is the relationship between solar torsional oscillations and solar activity?
• 3D Solar Wind Structure Features Characterizing the Rise of Cycle 24
• Chromospheric Observations of a Kink Wave in an On-disk Active Region Fibril
• Comparison of STEREO's Farside Observations of Solar Activity and Predictions from the Global Oscillations Network Group (GONG)
• Correlation between flare related photospheric magnetic field changes and X-ray flare location
• Detecting the Large Scale Magnetic Helicity Patterns on the Sun using SOLIS/VSM and SDO/HMI fulldisk vector magnetograms
• Evolution of active and polar photospheric magnetic fields during the rise of Cycle 24 compared to previous cycles
• Far-side seismic maps with HMI
• Flux Ropes and Small-Scale Interplanetary Transients - New Revelations from STEREO/SECCHI
• Heliospheric Space Weather at the Start of Cycle 24
• Improvements to the Virtual Solar Observatory
• Properties of Magnetic Neutral Lines and Filament Formation
• Science Highlights Utilizing SOLIS VSM Vector Magnetic Field Data
• Solar Coronal Temperature and Line Emission During the Long Minimum and the Rise of Cycle 24
• Solar Magnetic Flux Transport Modeling with Far-side Data
• Solar dynamics at high latitudes and deep in the convection zone
• The Longitudinal Solar Magnetic Field Measured by SOLIS
• The Rising Phase of Solar Cycle 24: General Solar Wind, Large-Scale Solar Wind Structures, and Sector Asymmetry
• A Coral Sea Rehearsal for the Eclipse Megamovie
• Coronal Activity and Extended Solar Cycles
• Revelations on Heliospheric Imaging of Polarized Light
• Comet C/2012 S1 (ISON): Observations of the Dust Grains from SOFIA and of the Atomic Gas from NSO Dunn and McMath-Pierce Solar Telescopes (Invited)
• Counting Sunspots from Space (Invited)
• Global Solar Photospheric Magnetic Field Modeling (Invited)
• Modeling the corona and solar wind using ADAPT maps with data assimilated helioseismic detected active regions (Invited)
• Observing Molecular Hydrogen with IRIS
• Solar Active Region Morphologies Selected From Near-Side Helioseismic Data
• Solar Coronal Temperature During the Long Minimum and the Rise of Cycle 24
• Testing the Reliability of Far-side Active Region Predictions from Helioseismology using STEREO Far-side Observations
• The Mg II h&k lines as seen by IRIS: what do they tell us about the solar chromosphere? (Invited)
• Chromospheric Acoustic Oscillations in Active Flaring Regions
• Current and Kinetic Helicity of Long-Lived Activity Complexes
• Dynamical behaviour of photospheric bright points during merging
• Estimating the Global Solar Magnetic Field Distribution Using ADAPT
• First High-resolution Spectroscopic Observations by IRIS of a Fast, Helical Prominence Eruption Associated with a Coronal Mass Ejection
• Fitting of Intensity-Velocity Cross Spectrum using GONG and HMI Oscillation Data
• Forecasting Solar UV & F10.7 with ADAPT
• High-resolution Observations of the X-flare on 2014-03-29
• Measurement and Interpretation of Travel-Time Shifts in the context of Time-Distance Helioseismic Detection of Meridional Flows in the Solar Convection Zone
• Next-generation Solar Data and Data Services from the Daniel K. Inouye Solar Telescope
• Observational Evidence of Resonant Absorption in Oscillating Prominence
• Quantifying Photospheric Processes Using a New Pixel Dynamics Model
• The DKIST Operations Lifecycle: From Proposal Preparation to Completion
• The VAULT2.0 Observing Campaign: A Comprehensive Investigation of the Chromosphere-Corona Interface at Sub-arcsecond scales
• Three Dimensional Chromospheric Temperature Structure of Sunspot
• Contextualizing Solar Cycle 24: Report on the Development of a Homogenous Database of Bipolar Active Regions Spanning Four Cycles
• Cylindrical Symmetry of Sunspots as a Proxy for Flare-Related Changes in Pseudo-Vector Magnetic Field Derived from Line-of-Sight Magnetograms
• H-alpha Off-limb Carrington Synoptic Charts
• Pixel Analysis and Plasma Dynamics Characterized by Photospheric Spectral Data
• Remote Observations of the Lunar Sodium Exosphere
• Response of Solar Oscillations to Magnetic Activity in Cycle 24
• Solar Subsurface Flows During Solar Cycle 24
• Transitioning GONG data processing to NOAA SWPC operations
• A PDS Archive for Observations of Mercury's Na Exosphere
• Absorption by Mercury's Exosphere During the May 9th, 2016 Solar Transit.
• Blending of Ground- and Space-Based Magnetograms: Application to L1-L5 Solar Wind and Coronal Hole Predictions
• CATE 2016 Indonesia: Image Calibration, Intensity Calibration, and Drift Scan
• CATE 2016 Indonesia: Optics and Focus Strategy
• CATE 2016 Indonesia: Science goals and student training for 2017
• Modeling the Global Coronal Field with Simulated Synoptic Magnetograms from L1 and L5
• On the Origin of Long-duration Solar Gamma-ray Flares and Their Connection with SEPs
• Signatures of coronal rain observed in the chromosphere of an Active Region Filament
• Sub-Pixel Magnetic Field Dynamics Derived from Photospheric Spectral Line Profiles
• The DKIST Data Center: Meeting the Data Challenges for Next-Generation, Ground-Based Solar Physics
• The extreme space weather event of 1859: A case of historical and physical alignment
• Citizen CATE: Evaluating Outcomes of a Solar Eclipse Citizen Science Project
• Coronagraphic Observations of the Lunar Sodium Exosphere
• Formation of the UV Spectrum of Molecular Hydrogen in the Sun
• Harmonizing Mangnetograph Data with end-to-end Instrument Simulations
• Polarization Observations of the Total Solar Eclipse of August 21, 2017
• Quantized Advantages to a Proposed Satellite at L5 from Simulated Synoptic Magnetograms
• SunPy: Python for Solar Physics
• The Solar Wind Source Cycle: Relationship to Dynamo Behavior
• Bridging the gap between Hawai'i students and solar astronomy in preparation for the Daniel K. Inouye Solar Telescope
• Engineering of the HiWIND Thermospheric Wind Observatory
• Evaluating the Performance of a Non-LTE Archive for Fast Inversion of Chromospheric Spectra
• Exploring the Cool Pockets in the Solar Atmosphere
• Formation of a Kilogauss Magnetic Flux Rope Prior to an X9-Class Flare
• How will DKIST Help Us Understand the Magnetic Connectivity Between the Sun and the Earth?
• Multi-wavelength Fourier Observations of Solar Acoustic Waves Near Active Regions with GONG and SDO AIA
• Properties of sunspot oscillations and wave propagation in NOAA AR 12470 as observed with ALMA and BBSO instruments
• An Erupting Solar Filament Observed at the DST
• Calibrating GONG Magnetograms Using an End-to-end Magnetograph Model
• Progression of Solar Cycle 24 As Seen in Acoustic Mode Frequencies of the Sun
• Quantifying Properties of Photospheric Magnetic Field Cancellation Events in the Quiet Sun Internetwork
• Solar Cycle-Related Variability of Sun-as-a-Star Spectral Line Profiles
• Stokes Line Parameters as Possible Indicators of Flaring Activity: A Comparison of Flaring and Non-Flaring Active Regions
• SunPy v1.0, the community-developed, free and open-source solar data analysis environment for Python.
• Time dependent properties of Inverse Evershed Flow and Perspectives with Daniel K. Inouye Solar Telescope (DKIST)
• Volume-filling Simulations of Coronal Loops Heated by Nanoflares
• A Survey of Computational Tools in Solar Physics
• ALMA observations and spectral inversions - what can we learn about the Sun and our techniques?
• Analysis of Atmospheric Seeing Measurements
• Analysis of DKIST Adaptive Optics Jitter Control
• Automated Single Point Inversions of Infrared Forbidden Lines for DKIST Coronal Observations
• Bringing Together Professionals and Undergraduate Students in a Virtual Environment
• COFFIES - Developing a Reliable Physical Model of the Solar Activity Cycle
• COSPAR International Space Weather Action Teams: Addressing Challenges Across the Field of Space Weather.
• Constraining Global Coronal Models with Multiple Independent Observables
• Constraining wave propagation throughout the solar atmosphere with IBIS, ALMA and IRIS
• Continuous Subsurface Flow Measurements for Solar Cycle 23 from MDI Spherical Harmonic Time Series
• DKIST and Advances in Chromospheric Polarimetry: Connecting the Trees with the Forest
• Derivation of Toroid Patterns from Analysis of Magnetograms And Inferring Their Deep-origin
• Estimation of Low-energy Cutoff of Non-thermal Electrons from a Spectro-polarimetric Observation
• Evaluating Model Advancements for Predicting CME Arrival Time - CCMC/NOAA SWPC Partnership Final Report
• Global Solar Flows and Magnetic Fields: Observing, Simulating and Predicting Their Impact on the Heliosphere and Terrestrial Atmosphere
• Helioseismic Constraints on the Solar Interior Dynamics and Dynamo
• Inferring Plasma Flows in the Solar Photosphere & Chromosphere using Deep Learning and Surface Observations
• Investigating Solar Minimum Below and Above the Solar Surface: Is the Current Solar Minimum Different from the Previous Minimum?
• Investigation of the X1.6 Flare Occurred in the Great Active Region 12192
• Multi-Wavelength Modeling and Analysis of the Center-to-Limb Effects of Solar Spectroscopy and Helioseismology
• On Recurrent Active Region Coronal Jets: Coronal Geyser Sources of Electron Beams and Interplanetary Type-III Radio Bursts
• Solar-Cycle Variation of the Subsurface Flows of Active and Quiet Regions
• Spectroscopic Inversions & Calibrations for DKIST Coronal Observations
• SunPy 2.0: the community-developed open-source solar data analysis environment for Python
• The CO Fundamental Band as an LTE Diagnostic of the Temperature Minimum
• The Solaris Solar Polar Mission: Exploring one of the last Unexplored Regions of the Solar System
• The Virtual Boulder Solar Alliance REU
• The challenges of cohort development during a virtual internship program in response to COVID-19
• The formation and dissipation of current sheets and shocks due to compressive waves in a stratified atmosphere containing a magnetic null
• The off-limb polarized corona at high-resolution: new synthetic views for the DKIST era
• A Comparative Study of Measurements of the Suns Axisymmetric Flows: A COFFIES Effort
• AWSoM MHD simulation of a solar active region with realistic spectral synthesis
• Adapting Software, Hardware, and Programming Support in a Virtual Environment for the Boulder Solar Alliance Research Experience for Undergraduates Program
• An Alternative Approach to Measuring Solar Velocities on the Solar Dynamics Observatory (SDO) Using the Helioseismic and Magnetic Imager (HMI)
• CLEDB - An Algorithm for Inverting Vector Magnetic Fields in The Solar Corona
• Characteristic based data-driven boundary conditions suitable for rapidly evolving solar active regions
• Chromospheric Heating Mechanisms in a Plage Region Constrained by Comparison of Magnetic Field and Mg II h & k Flux Measurements with Theoretical Studies
• Estimation of projection effects in the solar polar magnetic flux measurements from an ecliptic view.
• Exploration of the Physical and Spectroscopic Characteristics of Coronal Rain
• FETCH Concept: Investigating Quiescent and Transient Magnetic Structures in the Inner Heliosphere using Faraday Rotation of Spacecraft Radio Signals
• From 1973 to the 2020s, from SKYLAB to 3D vector magnetic fields in prominences
• Global solar flows and their impact on magnetic activity
• Heating of the solar atmosphere by electric currents
• Horizontal Flows Associated with Anti-Hale Active Regions
• Implementing general and robust non-reflecting boundary conditions for MHD simulations
• Increasing the Accessibility of Solar Science through Interactive Demonstration
• Kinetic and Magnetic Helicity in Solar Active Regions
• Novel Magnetic Field and Electron Density Measurements of CMEs (within AU) with the Proposed Multiview Observatory for Solar Terrestrial Science (MOST) Mission
• Polarized forbidden coronal line emission in the presence of active regions
• Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE): II. Flares and Eruptions
• Quantifying Magnetic Energy Flux in the Quiet Sun Photosphere using Sunrise/IMaX Observations
• Recent observations of stellar flares on G-, K-, and M-dwarf stars and possible mass ejections
• Solar Atmosphere Radiative Transfer Model Comparison based on 3D MHD Simulations
• Spectral Runway: An Analysis of Solar Balmer Lines through both Observations and Models
• Spectroscopic survey of infrared 1-4 m spectra in regions of prominent solar coronal emission lines of Fe XIII, Si X, and Si IX
• Subsurface Flow Measurements in the Near Surface Shear Layer over Two Solar Cycles
• Subsurface Plasma Flows and the Flare Productivity of Solar Active Regions
• The Daniel K Inouye Solar Telescope (DKIST) Data Center: Cyber-infrastucture for a next generation ground based solar telescope.
• The Multiview Observatory for Solar Terrestrial Science (MOST)
• The Next Generation GONG (ngGONG) Project: Ground-based Synoptic Studies of the Sun
• Visualizing the Solar Corona in Virtual Reality
• What Deep and Extended Minima Tell us about Magnetism Below the Surface?
• A First Look at Solar Prominences using the DKIST/CryoNIRSP
• Calibrating DKIST Data
• Chromospheric Horizontal Propagating Waves Revealed by Fast-Cadence Imaging in Ca II K with DKIST's Visible Broadband Imager
• Contribution to Solar Brightness of small-size magnetic elements
• Coordinated ground and airborne extended observations of TSE 2024 with Citizen CATE and NASA's WB-57s
• Coronal Polarimetric Calibration Using Thomson Scattering and Emissive Polarization above Solar Active Regions
• CryoNIRSP Commissioning Observations of Si X 1430 nm: Opening up a New Diagnostic
• DKIST Science Operations during the Operations Commissioning Phase
• Evolution of Kinetic and Magnetic Helicities in Solar Active Regions
• First Analysis of DL-NIRSP Integral Field Spectropolarimetry
• First Observation of Chromospheric Waves in a Sunspot by DKIST/ViSP
• First Observations from the DKIST/Cryogenic Near-IR Spectropolarimeter (CryoNIRSP)
• First Results of Non-LTE Spectro-Polarimetric Inversions of Magnetic Fine Structure as Observed with ViSP/DKIST
• Forward Modeling of Forbidden Coronal Lines in Synthetic Flares
• Horizontal Flows in and around "Rogue" Active Regions
• Improving the Detection of Active Regions near Solar Limbs in GONG Farside Helioseismic Maps
• Inferring three-dimensional magnetic structure of a sunspot using multi-wavelength measurements.
• Investigating Magnetic Structure in the Inner Heliosphere using Faraday Rotation, the FETCH instrument on the MOST mission
• Investigating Ohmic Heating as a Solar Active Region Atmosphere Heating Mechanism
• Large Photospheric Doppler Shift in Solar Active Region 12673
• MHD Simulation Uncertainties Imposed by Boundary Condition Choices
• Measurements of Reconnecting Magnetic Fields with DKIST
• Navigating the Challenges of a Hybrid REU Program to Optimize Student Experience and Value
• Observations and Simulations of Solar Flows and Their Roles in Magnetic Activity Patterns at the Surface
• Progressing Towards Faraday Rotation Tomography of Coronal Mass Ejections
• Properties of Chromospheric Flow Channels Around a Sunspot
• Reconciling Subsurface Flow Measurements from GONG, HMI and MDI
• Small-scale, internetwork magnetism in the quiet Sun: first look using the Visible Spectropolarimeter at DKIST
• Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SpIN4D): Magnetohydrodynamic Modeling and Forward Synthesis Pipeline
• Stellar Wind and the Exoplanetary Magnetosphere Compression in Sun-like Stars
• Sunspots at 0.03" Resolution
• The Coronal Solar Magnetism Observatory: Overview and Recent Progress
• The Sun's Global Flows: Differential Rotation
• Total Solar Irradiance During the Last Five Centuries and the Maunder Minimum
• Transient Events in the Chromosphere and Corona with IBIS, ALMA, IRIS, and XRT
• Uncertainty Estimates of Solar Wind Prediction: Significance and Impacts
• Unlocking Coronal Mysteries with DKIST: The First Chapter
• Upflows in solar active regions - producing a mix of abundances that can feed into the solar wind
• Using Infrared Extreme Limb spectropolarimetry with DKIST and CryoNIRSP to Understand the Photospheric Shear Layer
• Validation of novel a 3D magnetohydrodynamic data-driven simulation code using an expanding spheromak ground truth simulation
• Variability of High-degree Acoustic Mode Frequencies of the Sun and their Connection with the Surface Magnetic Activity

Linked Collaborating Authors [?]

• A. A. Norton
• A. A. Pevtsov
• A. G. de Wijn
• A. N. Zhukov
• A. Prasad
• A. Tritschler
• A. W. Merkel
• Aatiya Ali
• Adam Kobelski
• Albert Y. Shih
• Alexei A. Pevtsov
• Alin Rǎzvan Paraschiv
• Alina-Catalina Donea
• Alphonse C. Sterling
• Amir Caspi
• André Fehlmann
• B. Poduval
• Bart De Pontieu
• Bradley W. Hindman
• Brian E. Wood
• Brigitta Sipőcz
• C. E. Fischer
• C. J. Henney
• Carolus J. Schrijver
• Christoph U. Keller
• Cooper Downs
• D. A. Lacatus
• D. B. Jess
• D. J. Christian
• Daniel B. Seaton
• David B. Wexler
• David M. Long
• Debi Prasad Choudhary
• Dibyendu Nandy
• E. A. Jensen
• E. E. DeLuca
• F. Berrilli
• F. Giorgi
• F. Zuccarello
• G. Cauzzi
• Gábor Tóth
• H. M. Antia
• H. Uitenbroek
• Haosheng Lin
• Hardi Peter
• I. Ermolli
• Ignacio Ugarte-Urra
• Irina Kitiashvili
• J. E. Leake
• J. M. da Silva Santos
• J. P. Morgenthaler
• J. Schou
• J. T. Hoeksema
• J. Zhang
• Jack Jenkins
• James Paul Mason
• James R. A. Davenport
• Jason Kooi
• Kosuke Namekata
• Krishna M. Jain
• Krzysztof Barczynski
• L. Golub
• L. K. Harra
• L. K. Jian
• L. P. Chitta
• L. Teriaca
• Lisa Upton
• Lucas A. Tarr
• M. Falco
• M. H. Burger
• M. Haberreiter
• M. I. Desai
• M. Snow
• M. Stangalini
• Marc L. DeRosa
• Maria D. Kazachenko
• Martin A. Reiss
• Matthew J. West
• Mattia Di Mauro
• Mausumi Dikpati
• Meng Jin
• N. D. Kee
• N. E. Raouafi
• N. Gopalswamy
• N. M. Viall
• N. Nitta
• P. H. Scherrer
• P. Romano
• P. W. Schuck
• Paola Testa
• Peter H. Keys
• Petrus C. Martens
• Qian Gong
• R. Howe
• R. K. Ulrich
• Ryan Hofmann
• Ryan J. French
• S. C. Tripathy
• S. D. Bale
• S. E. Gibson
• S. F. Fung
• S. K. Solanki
• S. Parenti
• S. Tomczyk
• S. Vargas Domínguez
• S. Yashiro
• Sabrina Savage
• Sanjay Gosain
• Sanjiv K. Tiwari
• Sarah A. Kovac
• Sarbani Basu
• Shadia Rifai Habbal
• Shea Hess Webber
• Shuo Wang
• Steven Christe
• Sushant S. Mahajan
• Suzanne L. Hawley
• T. A. Kucera
• T. N. Woods
• Teresa Nieves‐Chinchilla
• Tetsu Anan
• Thomas A. Schad
• Thomas Berger
• V. Bernstein
• V. H. Hansteen
• V. Mangano
• V. Martínez Pillet
• Vasyl Yurchyshyn
• W. H. Carande
• W. T. Reach
• Xudong Sun
• Yunqian Zhu
• Yuta Notsu
• É. Buchlin