Member Since 2017
Manuel Enrique Cuesta
Postdoctoral Research Associate, Princeton University
AGU Research
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Turbulence relaxation processes in the Earth's magnetosheath
MAGNETIC STRUCTURES AND WAVES IN SOLAR WIND TURBULENCE III ORAL
spa-solar and heliospheric physics | 15 december 2023
Francesco Pecora, Yan Yang, Alexandros Chasapis, S...
In turbulence, nonlinear terms drive energy transfer from large-scale eddies into small scales through the so-called energy cascade. Turbulence often ...
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The Radial Evolution of Turbulence Properties Observed in the Solar Wind
TURCOTTE AWARDEE
nonlinear geophysics | 13 december 2023
Manuel E. Cuesta
Data analysis of in-situ measurements in the solar wind makes it possible to study its dynamics as it expands with increasing heliocentric distance. T...
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Constructing a Basis of Solar Energetic Particle Event Characteristics based on Source and Solar Wind Plasma Conditions
EVOLUTION OF HELIOSPHERIC LARGE-SCALE STRUCTURES USING OBSERVATIONS AND MODELING I POSTER
spa-solar and heliospheric physics | 12 december 2023
Manuel E. Cuesta, David J. McComas, Christina Cohe...
Solar energetic particle (SEP) events have been observed by the Parker Solar Probe (PSP) spacecraft since its launch in 2018. These events include sol...
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Density Fluctuation of Compressible Turbulence in the Solar Wind Near the Sun
COMPRESSIBLE TURBULENCE, DENSITY FLUCTUATIONS, AND THEIR IMPLICATIONS FOR HELIOSPHERIC PLASMAS II POSTER
spa-solar and heliospheric physics | 15 december 2022
Xiangrong Fu, Hui Li, Zhaoming Gan, Senbei Du, Joh...
The solar wind is a magnetized and turbulent plasma. Its turbulence is often dominated by Alfvénic fluctuations and often deemed as nearly incomp...
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Intermittency Statistics in the Expanding Solar Wind: Observations from Parker Solar Probe (0.16 au), Helios 1 (0.3 - 1 au), and Voyager 1 (1 - 10 au)
AMPLIFYING PARKER SOLAR PROBE SCIENCE WITH CONTEXTUAL SIMULATIONS AND SUPPORTING OBSERVATIONS I ORAL
spa-solar and heliospheric physics | 13 december 2021
Manuel E. Cuesta, Tulasi N. Parashar, Rohit Chhibe...
We examine statistics of magnetic field vector components to explore how intermittency evolves from near Sun plasma to radial distances as large as 10...
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Magnetic Field Intermittency Statistics in the Expanding Solar Wind: Parker Solar Probe (Encounters 1-3), Helios 1 (0.3 to 1AU), and Voyager 1 (1 to 10AU)
FUNDAMENTAL PLASMA PHYSICS AND TURBULENCE ENERGY TRANSFER: FROM MHD TO KINETIC SCALES III POSTERS
spa-solar and heliospheric physics | 09 december 2020
Manuel E. Cuesta, Tulasi N. Parashar, Riddhi Bandy...
We perform statistics on magnetic field vector components for Parker Solar Probe, Helios 1, and Voyager 1 spacecraft to explore how intermittency evol...
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Intermittency Statistics of the Expanding Solar Wind: Helios 1 (.3 to 1 AU) and Voyager 1 (1 to 10 AU)
FUNDAMENTAL PHYSICS OF THE SOLAR CORONA AND INNER HELIOSPHERE III POSTERS
spa-solar and heliospheric physics | 13 december 2019
Manuel E. Cuesta, Tulasi N. Parashar, William H. M...
We explore the turbulence statistics of the expanding solar wind plasma in the inner heliosphere (from 0.3 to 10 AU) using data from Helios 1 and Voya...
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Intermittency Statistics in the Expanding Solar Wind
FALL MEETING 2018
11 december 2018
Manuel E. Cuesta, William H. Matthaeus, Tulasi N. ...
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