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Empirical Measurement of Diffusive Heating across a Discontinuity in the Solar Wind
AGU 2024
spa-solar and heliospheric physics | 13 december 2024
Tamar Ervin, Trevor Bowen, Abigail Azari, Philip A...
A main goal of Parker Solar Probe (PSP) is to characterize the heating and acceleration mechanisms within the Suns corona and solar wind. The SPANi in...
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Novel Time-Frequency Representation: Gaussianity Scalogram
AGU 2024
spa-magnetospheric physics | 12 december 2024
Zesen Huang, Chen Shi, Marco C. Velli, Nikos Sioul...
Recent studies on the in situ measurements of the Parker Solar Probe have shown that the scale-dependent Gaussianity of the magnetic field contains su...
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On the phase space cascade evolution with Parker Solar Probe
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Andrea Larosa, Oreste Pezzi, Trevor Bowen, Domenic...
In space plasmas, due to the absence of collisions, the phase space shows a complex structuring and strong deviations from the thermal equilibrium. Pr...
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3-Minute Oscillations in the Upper Corona Observed by Parker Solar Probe
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Zesen Huang, Marco C. Velli, Chen Shi, YINGJIE ZHU...
Recent observations of Parker Solar Probe (PSP) from around the Alfven surface have shown that the trace magnetic power spectrum density (PSD) is ofte...
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Identifying the Traveling Atmospheric Disturbance (TAD) - related Traveling Ionospheric Disturbances (TIDs) in the Storm Time Ionosphere with NASA GDC AETHER
AGU 2024
spa-aeronomy | 11 december 2024
Lauren Christenson, Naomi Maruyama, Laila Andersso...
Geospace Dynamics Constellation (GDC) is an upcoming NASA mission that aims to understand the response of Earths upper atmosphere to magnetic storms. ...
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Assessing the Impact of Imbalance on Turbulent Dynamics at Inertial and Sub-Ion Scales in the Solar Wind
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Nikos Sioulas, Trevor Bowen, Alfred Mallet, John W...
Recent theoretical advances suggest that the statistical properties of sub-ion scale turbulence may vary significantly depending on the degree of imba...
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Employing Probabilistic Machine Learning in Understanding Wave-Particle Interactions
AGU 2024
spa-solar and heliospheric physics | 10 december 2024
Trevor Bowen, Abigail Azari, Kristopher G Klein, T...
Velocity distribution functions (VDFs) in collisionless plasmas often deviate significantly from Maxwellian distributions via the presence of secondar...
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Evolution of Alfven Wave and Turbulence Amplitude in the Sub-Alfvenic Solar Wind and its Relationship to Switchbacks
AGU 2024
spa-solar and heliospheric physics | 10 december 2024
Nikos Sioulas, Marco C. Velli, Chen Shi, Anna Tene...
Measurements from the Parker Solar Probe and Solar Orbiter are utilized to examine the evolution of turbulence amplitude as a function of the Alfvenic...
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