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Latitude Variations in Primary and Secondary Polar Crown Polarity Inversion Lines and Polar Coronal Hole Boundaries over Five Solar Cycles

High latitude polarity inversion lines (PILs)

Magnetic field and plasma diagnostics for solar coronal mass ejections: A case study using the forward modeling approach

Liu Fe xiii 10747 line and CME eruption

Coronal spectral diagnostics: The Coronal Solar Magnetic Observatory (COSMO)

UCOMP daily temperature map

Synthetic Lyman-α Emissions for the coronagraph aboard the ASO-S mission I: an Eruptive Prominence-cavity System

Lyman-alpha emission

Coronal Cavities in CoMP Observations

Cavity widths observed by SDO/AIA

Tracking Movement Of Long-lived Equatorial Coronal Holes From Analysis Of Long-term McA Data

all Coronal Holes centroids

Sarah Gibson is a 2022 AGU Fellow

Sarah Gibson smiling

Study of Coronal Hole Lifetimes

Coronal hole centroid latitude vs. Carrington Rotation

Designing a New Coronal Magnetic Field Energy Diagnostic

Non-potentiality diagnostics of the energized flux-rope simulation at time step 89

Global Maps of the Magnetic Field in the Solar Corona

Magnetic field of the Sun

Pagination

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This material is based upon work supported by the NSF National Center for Atmospheric Research, a major facility sponsored by the U.S. National Science Foundation and managed by the University Corporation for Atmospheric Research. Any opinions, findings and conclusions or recommendations expressed in this material do not necessarily reflect the views of the U.S. National Science Foundation.