SG
Member Since 1994
Sarah E. Gibson
Senior Scientist, National Center for Atmospheric Research
AGU Research
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WHPI Coordination for the April 8th 2024 Total Solar Eclipse
SOLAR ECLIPSE SCIENCE: WHAT WE LEARNED FROM THE GREAT AMERICAN ECLIPSES AND WHAT IS NEXT IV ORAL
spa-solar and heliospheric physics | 13 december 2024
Daniela Lacatus, Ian M. Hewins, Robert C. Allen, D...
The Whole Heliosphere and Planetary Interactions (WHPI) initiative organized a focused campaign supporting the 2024 Total Solar Eclipse and aimed to f...
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Radio Coronal Cavities at 1.2 GHz: Diagnosing the Pre-existing phase of a Magnetic Flux Rope
DIAGNOSING HELIOSPHERIC AND TERRESTRIAL PLASMA WITH RADIO OBSERVATIONS II ORAL
spa-solar and heliospheric physics | 13 december 2024
Shaheda Begum Shaik, Devojyoti Kansabanik, Sarah E...
Investigating coronal cavities, which trace the magnetic structure of flux ropes surrounding the filament material, provides insights into the pre-exi...
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Beyond Flatland: A Star of Many Dimensions
2024 EUGENE PARKER LECTURE
spa-solar and heliospheric physics | 12 december 2024
Sarah E. Gibson
The more we learn about the Sun, the more we can appreciate its essential complexity. Multi-wavelength observations reveal its structured coronal atmo...
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Polarimeter to UNify the Corona and Heliosphere (PUNCH): Plans for Launch and Open Science
COMBINING CORONAL AND HELIOSPHERIC IMAGING, IN SITU OBSERVATIONS, AND MODELING TO UNDERSTAND THE YOUNG SOLAR WIND II POSTER
spa-solar and heliospheric physics | 10 december 2024
Craig E. DeForest, Ronnie Killough, Sarah E. Gibso...
The Polarimeter to UNify the Corona and Heliosphere (PUNCH) is a NASA mission to image the outer reaches of the solar corona and inner reaches of the ...
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White-light Polarization in the Corona and Heliosphere: Putting the "P" in PUNCH
COMBINING CORONAL AND HELIOSPHERIC IMAGING, IN SITU OBSERVATIONS, AND MODELING TO UNDERSTAND THE YOUNG SOLAR WIND I ELIGHTNING
spa-solar and heliospheric physics | 10 december 2024
Sarah E. Gibson, Craig E. DeForest, Curt de Koning...
The polarization of Thomson-scattered white light provides a powerful tool for localizing substructures in the solar corona and inner heliosphere, and...
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Dynamic CME Sheath and Shock Properties in High-Resolution Simulation and Predictions for the PUNCH Mission
COMBINING CORONAL AND HELIOSPHERIC IMAGING, IN SITU OBSERVATIONS, AND MODELING TO UNDERSTAND THE YOUNG SOLAR WIND I ELIGHTNING
spa-solar and heliospheric physics | 10 december 2024
Elena Provornikova, Viacheslav G. Merkin, Andrew J...
Recent close-up imaging observations of CMEs at a few tens of solar radii from the Sun reveal abundant substructures in CMEs, raising questions about ...
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MHD Simulation of Prominence-Cavity System
DATA-DRIVEN MODELING OF THE MAGNETIC FIELD EVOLUTION IN SOLAR ERUPTIONS (JETS, FLARES, CMES) POSTER
spa-solar and heliospheric physics | 09 december 2024
Yuhong Fan, Hongyang Luo, Jie Zhao, Sarah E. Gibso...
We present MHD simulations of a twisted coronal flux rope under a coronal streamer with the formation of prominence condensations, and the development...
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An Ancient and Modern Sun-Watching Theme as a Rallying Point for Collaboration among NASA PUNCH Outreach, Parker Solar Probe, CATE 2024, and a SciAct project called Science through Shadows
THE SOLAR ECLIPSES OF 2023 AND 2024: RESULTS FROM PARTICIPATORY SCIENCE EFFORTS, THE NATIONWIDE ECLIPSE BALLOONING PROJECT (NEBP), AND RELATED ENGAGEMENT ACTIVITIES I POSTER
union sessions | 09 december 2024
Cherilynn A. Morrow, John M. Keller, Craig E. DeFo...
The multi-institutional, multicultural, and multigenerational public engagement team embedded in the NASA PUNCH mission to study the Sun collaborates ...
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