activity
19972019
most citedTurbulent coronal heating and the distribution of nanoflares

95 citations · 524 across the 17 of their papers we have counts for

collaborators

18 papers

physics.space-ph2019★ 11 cited

[Plasma 2020 Decadal] The essential role of multi-point measurements in turbulence investigations: the solar wind beyond single scale and beyond the Taylor Hypothesis

W. H. Matthaeus, R. Bandyopadhyay, M. R. Brown +46

This paper briefly reviews a number of fundamental measurements that need to be made in order to characterize turbulence in space plasmas such as the solar wind. It has long been k…

physics.plasm-ph2018★ 4 cited

Normal Modes in Magnetized Two-Fluid Spin Quantum Plasmas

Daniel O. Gomez, Alejandra Kandus

We extend the classical two-fluid magnetohydrodynamic (MHD) formalism to include quantum effects such as electron Fermi pressure, Bohm pressure and spin couplings. At scales smalle…

physics.plasm-ph2018★ 34 cited

Turbulent electromagnetic fields at sub-proton scales: two-fluid and full-kinetic plasma simulations

C. A. González, T. Parashar, D. Gomez +2

Plasma dynamics is a multi-scale problem that involves many spatial and temporal scales. Turbulence connects the disparate scales in this system through a cascade that is establish…

physics.space-ph2014★ 22 cited

The ULF wave foreshock boundary: Cluster observations

Nahuel Andres, Karim Meziane, Christian Mazelle +2

The interaction of backstreaming ions with the incoming solar wind in the upstream region of the bow shock gives rise to a number of plasma instabilities from which ultra-low frequ…

astro-ph.SR2014

Simulations of the Kelvin-Helmholtz instability driven by coronal mass ejections in the turbulent corona

Daniel O. Gomez, Edward E. DeLuca, Pablo D. Mininni

Recent high resolution AIA/SDO images show evidence of the development of the Kelvin-Helmholtz instability, as coronal mass ejections (CMEs) expand in the ambient corona. A large-s…

astro-ph.EP2014★ 23 cited

Steady-State Magnetohydrodynamic Flow Around an Unmagnetized Conducting Sphere

Norberto Romanelli, Daniel Gomez, Cesar Bertucci +1

The non-collisional interaction between conducting obstacles and magnetized plasma winds can be found in different scenarios, from the interaction occurring between regions inside…