MC
Member Since 1998
Marco C M Velli
Professor, University of California Los Angeles
Marco Velli is Professor of Space Physics at the EPSS, UCLA. A student of the Univ. of Pisa and Scuola Normale Superiore, I spent research periods at the University of St. Andrews, Scotland, the Observatoire de Paris, France, UniCal, Italy, and the Smithsonian CfA, Mass., as well as JPL CalTec, where I remain a Senior Scientist. My research focuses on space plasma physics and solar magnetic activity, with emphasis on coronal heating, mhd turbulence and magnetic reconnection.
Professional Experience
University of California Los Angeles
Professor
2014 - Present
University of Florence
Associate Professor
1993 - 2014
NASA Jet Propulsion Laboratory
Senior Research Scientist
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Education
Scuola Normale Superiore
Doctorate
1985
Honors & Awards
Eugene Parker Lecture
Received December 2022
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Union Fellow
Received December 2014
Citation
For his pioneering work on coronal heating, the origin of the solar wind, and the theory of solar wind turbulence driven by wave reflections.
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Publications
Parker Solar Probe Observations of Solar Wind Energetic Proton Beams Produced by Magnetic Reconnecti...

We report observations of reconnection exhausts in the Heliospheric Current Sheet (HCS) during Parker Solar Probe Encounters 08 and 07, at 16 Rs an...

May 04, 2022
AGU Abstracts
The Evolution of the 1/f Range Within a Single Fast-Solar-Wind Stream Between 17.4 and 45.7 Solar Radii
FUNDAMENTAL PHYSICS OF THE SOLAR CORONA AND INNER HELIOSPHERE IV POSTER
spa-solar and heliospheric physics | 15 december 2023
Nooshin Davis, Benjamin D. Chandran, Trevor Bowen...
MHD turbulence accounts for many of the temporal and spatial variations in the fluid variables observed in the solar wind and other plasmas. The turbu...
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Evolution of MHD turbulence in the expanding solar wind: residual energy and intermittency
MAGNETIC STRUCTURES AND WAVES IN SOLAR WIND TURBULENCE II ORAL
spa-solar and heliospheric physics | 15 december 2023
Chen Shi, Nikos Sioulas, Zesen Huang, Marco C. Vel...
We conduct 3D MHD simulations of decaying turbulence in the solar wind context. To account for the spherical expansion of the solar wind, we implement...
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Investigating the Structure and Dynamics of the Heliospheric Current Sheet
FUNDAMENTAL PHYSICS OF THE SOLAR CORONA AND INNER HELIOSPHERE IV POSTER
spa-solar and heliospheric physics | 15 december 2023
Lizet Casillas, Marco C. Velli
The heliospheric current sheet (HCS) is the boundary between open magnetic field lines of opposite polarity in the solar wind that are also rooted in ...
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Volunteer Experience
2015 - 2016
Member
Space Physics and Aeronomy Fellows Committee
2010 - 2011
Associate Editor
JGR Space Physics Section
Check out all of Marco C M Velli’s AGU Research!
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