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Marco Velli
University of California Los AngelesMeeting roles in:
Properties of Current Sheets in 2D Tearing-Mediated MHD Turbulence
Linear Growth Rate of Compressible Tearing Instability in a Force-Free Current Sheet
SOHO/LASCO Wide Coronal Outflows and Pseudostreamers
Fundamental Physics of the Solar Corona and Inner Heliosphere I Oral
Fundamental Physics of the Solar Corona and Inner Heliosphere II Oral
Investigating hemispheric asymmetries in coronal hole solar wind structured by magnetolatitude
Spherically polarized Alfvénic fluctuations and solar wind acceleration: the Gosling boost.
Fundamental Physics of the Solar Corona and Inner Heliosphere III Poster
Evolution and Acceleration of Solar Wind during Fast Radial Scans of Parker Solar Probe
In situ evidence of 5-minute oscillations from Parker Solar Probe
On the Formation and Evolution of Secondary Conical Heliospheric Current Sheets
Radial velocity fluctuations at Parker Solar Probe during closest approach in encounter 22
The NASA Living With a Star Heliophysics Summer School: Exposing the next generation of researchers to Machine Learning Use Cases
The Sun reversed its decades-long weakening trend in 2008
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