activity
19972026
most citedNew Mass Loss Measurements from Astrospheric Lyman-alpha Absorption

469 citations · 4.2k across the 106 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

32 papers · 1 filter

astro-ph.SR2026

Signatures of Reconnection and a Split Heliospheric Tail in High-Energy Energetic Neutral Atoms

M. Kornbleuth, M. Opher, J. F. Drake +10

The shape of the heliosphere, regarded as comet-like since the 1960s, has recently been the subject of intense debate in the last decade. There is disagreement whether the heliosph…

astro-ph.SR2026

Conversion Layer Controls the Evolution of Magnetic Deflections Near the Alfven Surface

Dominic Payne, Mojtaba Akhavan-Tafti, Joshua Goodwill +10

We examine the statistics of Alfvenic deflections in both sub-Alfvenic and super-Alfvenic solar wind with particular focus on a common parameter that underlies the definition of sw…

astro-ph.SR2025

Nature of Transonic Sub-Alfvénic Turbulence and Density Fluctuations in the Near-Sun Solar Wind: Insights from Magnetohydrodynamic Simulations and Nearly-Incompressible Models

Giuseppe Arrò, Hui Li, Gary P. Zank +2

Recent Parker Solar Probe measurements have revealed that solar wind (SW) turbulence transits from a subsonic to a transonic regime near the Sun, while remaining sub-Alfvénic. Thes…

astro-ph.SR2025

Solar Coronal Heating: Role of Kinetic and Inertial Alfvén Waves in Heating and Charged Particle Acceleration

Syed Ayaz, Gary P. Zank, Imran A. Khan +3

A comprehensive understanding of solar coronal heating and charged particle acceleration remains one of the most critical challenges in space and astrophysical plasma physics. In t…

astro-ph.SR2025★ 15 cited

Electromagnetic Electron Kelvin-Helmholtz Instability

H. Che, G. P. Zank

On electron kinetic scales, ions and electrons decouple, and electron velocity shear on electron inertial length can trigger electromagnetic (EM) electron Kelvin-Helmhol…

astro-ph.SR2024★ 9 cited

A study of particle acceleration, heating, power deposition, and the damping length of kinetic Alfvén waves in non-Maxwellian coronal plasma

S. Ayaz, Gary P. Zank, Imran A. Khan +2

The heating of the solar corona and solar wind, through suprathermal particles and kinetic Alfvén waves within the 0 - 10 range, has been a subject of great interest…