HR
Member Since 1999
Holly Robin Gilbert
Director, High Altitude Observatory, National Center for Atmosperic Research
AGU Research
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Revealing how free magnetic energy build-up at the base of the corona leads to eruptions through spectropolarimetric observations in the NUV
NEW INSIGHTS INTO CORONAL PHYSICS FROM EUV AND UV SPECTROSCOPY I POSTER
spa-solar and heliospheric physics | 13 december 2023
Alfred de Wijn, Holly R. Gilbert, Paul Bryans, Reb...
The solar magnetic field evolves from the β >> 1 photosphere to the β << 1 corona to form twisted, non-potential flux ropes in the corona ...
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The power of ground-based coronagraphs
INTERPRETING REMOTE SENSING AND IN SITU OBSERVATIONS TO BUILD A GLOBAL VIEW OF THE CORONA AND SOLAR WIND POSTER
spa-solar and heliospheric physics | 12 december 2023
Sarah E. Gibson, Joan Burkepile, Holly R. Gilbert,...
For decades, we have observed the middle corona with instruments from the Mauna Loa Solar Observatory, including the white light K-Coronagraph (K-Cor)...
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The Chromospheric Magnetism Explorer (CMEx)
MEASUREMENT TECHNIQUES FOR SPACE PLASMA II ORAL
spa-solar and heliospheric physics | 12 december 2023
Holly R. Gilbert
CMEx is a mission concept submitted to NASA's Heliophysics SMEX program that, if selected, will fly in 2028. CMEx uses ultraviolet spectropolarimetry ...
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The COMPLETE mission concept for comprehensive 3D understanding of coronal magnetic energy storage and release
HELIOPHYSICS RESEARCH OUTLOOK: THE NEED FOR MULTI-VIEWPOINT OBSERVATIONS I ORAL
spa-solar and heliospheric physics | 15 december 2022
Amir Caspi, Daniel B. Seaton, Roberto Casini, Coop...
How magnetic energy is stored and impulsively released to power plasma heating, particle acceleration, and bulk flows in solar eruptions (flares, CMEs...
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The Coronal Solar Magnetism Observatory: Overview and Recent Progress
HIGH-ENERGY SOLAR INVESTIGATIONS THROUGH NEXT-GENERATION REMOTE SENSING: SPECTROSCOPY, IMAGING, AND BEYOND I ORAL
spa-solar and heliospheric physics | 13 december 2022
Steven Tomczyk, Joan Burkepile, Alfred de Wijn, Sa...
Magnetism is the dominant force in the solar corona. It plays a key role in structuring the corona on all spatial scales, in heating the corona, and a...
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The Chromospheric Magnetism Explorer (CMEx)
HIGH-ENERGY SOLAR INVESTIGATIONS THROUGH NEXT-GENERATION REMOTE SENSING: SPECTROSCOPY, IMAGING, AND BEYOND IV POSTER
spa-solar and heliospheric physics | 13 december 2022
Holly R. Gilbert
We discuss a new mission that uses ultraviolet spectropolarimetry to diagnose magnetism from the solar photosphere to the transition region. CMEx expl...
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The COMPLETE mission concept for the Heliophysics Decadal Survey
HIGH-ENERGY SOLAR INVESTIGATIONS THROUGH NEXT-GENERATION REMOTE SENSING: SPECTROSCOPY, IMAGING, AND BEYOND II ORAL
spa-solar and heliospheric physics | 17 december 2021
Daniel B. Seaton, Amir Caspi, Roberto Casini, Coop...
We present the COMPLETE mission concept, currently under study for the upcoming Heliophysics Decadal Survey. COMPLETE would provide the first comprehe...
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From 1973 to the 2020s, from SKYLAB to 3D vector magnetic fields in prominences
OBSERVING AND MODELING THE SOLAR ATMOSPHERE: RECENT FINDINGS AND FUTURE CHALLENGES I ORAL
spa-solar and heliospheric physics | 16 december 2021
Daniela Lacatus, Philip G. Judge, Holly R. Gilbert...
Routine measurement of the vector magnetic fields threading prominences would mark a significant advance in our ability to determine the dynamics of t...
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