Nicholeen Viall
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American solar physicist
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Nicholeen Viallphysics Degrees
Physics
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Astrophysics
#959
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#1044
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Physics
Nicholeen Viall's Degrees
- PhD Astrophysics University of California, Berkeley
- Masters Physics Stanford University
- Bachelors Physics Stanford University
Why Is Nicholeen Viall Influential?
(Suggest an Edit or Addition)According to Wikipedia, Nicholeen Viall is an American solar physicist who is the Chair of the American Astronomical Society's Solar Physics Division. Viall is known for her work on connecting dynamics of the solar corona to dynamics of the solar wind, based on observed variability of the corona-heliosphere system with both remote-sensing instruments and in-situ probes, and for her work on understanding evolution of the plasma in the inner heliosphere. She is the mission scientist for NASA's PUNCH mission, and a co-investigator on the ISS/CODEX and Parker Solar Probe/WISPR coronal imaging instruments.
Nicholeen Viall's Published Works
Published Works
- EVIDENCE FOR WIDESPREAD COOLING IN AN ACTIVE REGION OBSERVED WITH THE SDO ATMOSPHERIC IMAGING ASSEMBLY (2012) (98)
- Relative occurrence rates and connection of discrete frequency oscillations in the solar wind density and dayside magnetosphere (2009) (93)
- PATTERNS OF NANOFLARE STORM HEATING EXHIBITED BY AN ACTIVE REGION OBSERVED WITH SOLAR DYNAMICS OBSERVATORY/ATMOSPHERIC IMAGING ASSEMBLY (2011) (92)
- The Highly Structured Outer Solar Corona (2018) (80)
- Near-Sun observations of an F-corona decrease and K-corona fine structure (2019) (74)
- PERIODIC DENSITY STRUCTURES AND THE ORIGIN OF THE SLOW SOLAR WIND (2014) (66)
- MODELING THE LINE-OF-SIGHT INTEGRATED EMISSION IN THE CORONA: IMPLICATIONS FOR CORONAL HEATING (2013) (51)
- FADING CORONAL STRUCTURE AND THE ONSET OF TURBULENCE IN THE YOUNG SOLAR WIND (2016) (44)
- Examining Periodic Solar-Wind Density Structures Observed in the SECCHI Heliospheric Imagers (2010) (44)
- Implications of L1 observations for slow solar wind formation by solar reconnection (2016) (43)
- Relating Streamer Flows to Density and Magnetic Structures at the Parker Solar Probe (2020) (39)
- Nine Outstanding Questions of Solar Wind Physics (2020) (39)
- Are periodic solar wind number density structures formed in the solar corona? (2009) (37)
- Observations of Solar Coronal Rain in Null Point Topologies (2019) (34)
- Inherent length-scales of periodic solar wind number density structures (2008) (30)
- Dressing the Coronal Magnetic Extrapolations of Active Regions with a Parameterized Thermal Structure (2018) (28)
- A Survey of Nanoflare Properties in Active Regions Observed with the Solar Dynamics Observatory (2017) (27)
- The Heliospheric Current Sheet and Plasma Sheet during Parker Solar Probe’s First Orbit (2020) (26)
- The effect of magnetopause motion on fast mode resonance (2014) (26)
- PATTERNS OF ACTIVITY IN A GLOBAL MODEL OF A SOLAR ACTIVE REGION (2016) (26)
- MEASURING TEMPERATURE-DEPENDENT PROPAGATING DISTURBANCES IN CORONAL FAN LOOPS USING MULTIPLE SDO/AIA CHANNELS AND THE SURFING TRANSFORM TECHNIQUE (2013) (23)
- The Source, Significance, and Magnetospheric Impact of Periodic Density Structures Within Stream Interaction Regions (2019) (22)
- THE TRANSITION REGION RESPONSE TO A CORONAL NANOFLARE: FORWARD MODELING AND OBSERVATIONS IN SDO/AIA (2015) (22)
- Helios Observations of Quasiperiodic Density Structures in the Slow Solar Wind at 0.3, 0.4, and 0.6 AU (2019) (17)
- Understanding Heating in Active Region Cores through Machine Learning. I. Numerical Modeling and Predicted Observables (2019) (15)
- SIGNATURES OF STEADY HEATING IN TIME LAG ANALYSIS OF CORONAL EMISSION (2016) (15)
- Patterns of Nanoflare Storm Heating Exhibited by an Active Region Observed with SDO/AIA (2011) (11)
- Inherent Length Scales of Periodic Mesoscale Density Structures in the Solar Wind Over Two Solar Cycles (2020) (10)
- Power Spectral Density Background Estimate and Signal Detection via the Multitaper Method (2020) (9)
- Mesoscale Structure in the Solar Wind (2021) (8)
- On the Relationship between Magnetic Expansion Factor and Observed Speed of the Solar Wind from Coronal Pseudostreamers (2020) (6)
- Connecting the Low to the High Corona: A Method to Isolate Transients in STEREO/COR1 Images (2021) (6)
- New Insights into the First Two PSP Solar Encounters Enabled by Modeling Analysis with ADAPT-WSA (2022) (4)
- The Multiview Observatory for Solar Terrestrial Science (MOST) (2023) (4)
- SPD_MTM: a spectral analysis tool for the SPEDAS framework (2020) (4)
- The Solaris Solar Polar Mission (2020) (4)
- On Differentiating Multiple Types of ULF Magnetospheric Waves in Response to Solar Wind Periodic Density Structures (2021) (4)
- Using SDO/AIA to Understand the Thermal Evolution of Solar Prominence Formation (2016) (3)
- Defining the Middle Corona (2022) (3)
- Understanding Heating in Active Region Cores through Machine Learning. II. Classifying Observations (2021) (2)
- Understanding Space Weather: Part III: The Sun’s Domain (2017) (2)
- Exploring the Critical Coronal Transition Region:The Key to Uncovering the Genesis of the Solar Wind and Solar Eruptions (2020) (2)
- The Heating of the Solar Corona (2021) (2)
- An Analysis of Spikes in Atmospheric Imaging Assembly (AIA) Data (2021) (2)
- Deciphering the birth region, formation, and evolution of ambient and transient solar wind using heavy ion observations (2022) (2)
- An analysis of spikes in SDO/AIA data (2021) (1)
- Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum (2023) (1)
- The Solar Wind (2021) (1)
- Periodic Solar Wind Structures Observed in Measurements of Elemental and Ionic Composition in situ at L1 (2022) (1)
- The Heliospheric Current Sheet and Plasma Sheet (2020) (1)
- Investigating the Thermal Evolution of Solar Prominence Formation (2015) (0)
- Elemental building blocks of the slow solar wind (2014) (0)
- Orbital Opportunities for Coordinated Science with Parker Solar Probe, STEREO,and Solar Orbiter (2018) (0)
- Determining the Typical Nanoflare Cadence in Active Regions: Comparing SDO/AIA Observations with Modeled Active Region Light Curves (2012) (0)
- Probing Prominence Formation with Time Series Analysis of Models and AIA Data (2016) (0)
- Nanoflare Heating of the Solar Corona: Comparing SDO/AIA Observations with Modeled Light Curves (2012) (0)
- Near-Sun observations of an F-corona decrease and K-corona fine structure (2019) (0)
- The S-Web Origin of Composition Enhancement in the Slow-to-Moderate Speed Solar Wind (2023) (0)
- Observational Evidence of Coronal Magnetic Reconnection during Quiescent Conditions (2018) (0)
- Methods on Efficiently Relating Data from the Sun to In-situ Data at L1: An Application to the Slow Solar Wind (2017) (0)
- Slow mode waves and quasi-periodic upflows in the multi-temperature solar corona as seen by the SDO (2013) (0)
- Combining Remote and In Situ Observations with MHD models to Understand the Formation of the Slow Solar Wind (2017) (0)
- Study of Type III Radio Bursts in Nanoflares (2018) (0)
- SDO / AIA Observations of Slow Mode Waves in Coronal Fan Loops (2012) (0)
- Solaris: A Focused Solar Polar Discovery-class Mission to achieve the Highest Priority Heliophysics Science Now (2023) (0)
- Identifying Slow Solar Wind Sources (2018) (0)
- Simulations of Thermal Nonequilibrium in Raining Null-Point Topologies (2019) (0)
- Tracing the Origins of the Solar Wind by Tracking Flows and Disturbances in Coronagraph Data (2018) (0)
- Nanoflare Heating of the Quiet Sun (2015) (0)
- Using the fingerprints of solar magnetic reconnection to identify the elemental building blocks of the slow solar wind (2015) (0)
- Imaging the Top of the Solar Corona and the Young Solar Wind (2016) (0)
- COHERENT: Studying the corona as a holistic environment (2019) (0)
- A Survey of Coronal Heating Properties in Solar Active Regions (2014) (0)
- Diagnosing Coronal Heating in a Survey of Active Regions using the Time Lag Method (2017) (0)
- Thinking Outside the Sun-Earth Line: Science and Operational Applications of Alternative Solar Vantage Points I Posters (2019) (0)
- On the Source of Periodic Solar Wind Number Density Structures Using the Alpha to Proton Abundance Ratio (2008) (0)
- Erratum: “On the Relationship between Magnetic Expansion Factor and Observed Speed of the Solar Wind from Coronal Pseudostreamers” (2020, ApJ, 898, 78) (2021) (0)
- Nanoflare Properties throughout Active Regions: Comparing SDO/AIA Observations with Modeled Active Region Light Curves (2012) (0)
- The Coronal Heating Problem (2020) (0)
- Combining Remote and in situ Parker Solar Probe and STEREO Data to Understand Solar Wind Density Structures (2019) (0)
- SDO/AIA Light Curves and Implications for Coronal Heating: Observations (2010) (0)
- Imaging the Solar Corona From Within (2020) (0)
- SDO/AIA Light Curves and Implications for Coronal Heating: Model Predictions (2010) (0)
- Scattered Light in the Hinode/EIS and SDO/AIA Instruments Measured from the 2012 Venus Transit (2022) (0)
- Power spectrum power-law indices as a diagnostic of coronal heating (2018) (0)
- Multipoint Analysis of Meso-scale Structures in the Ambient Solar Wind: STEREO-A, -B, and L1 Observations (2008) (0)
- Parker Solar Probe Observations of the Release of Density Blobs and Flux Ropes at the Heliospheric Current Sheet (2019) (0)
- Thermal Time Evolution of Non-Flaring Active Regions Determined by SDO/AIA (2016) (0)
- Understanding Solar Wind Formation by Identifying the Origins of In Situ Observations (2021) (0)
- Sifting Through SDO's AIA Cosmic Ray Hits to Find Treasure (2017) (0)
- The Dynamics of Open-Field Corridors (2016) (0)
- A Survey of Nanoflare Properties in Solar Active Regions (2013) (0)
- Pulsed Flows Along a Cusp Structure Observed with SOO/AIA (2011) (0)
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