72 citations · 377 across the 15 of their papers we have counts for
15 papers
Two-fluid numerical model of chromospheric heating and plasma outflows in a quiet-Sun
K. Murawski, Z. E. Musielak, S. Poedts +2
\textbf{Purpose:} This paper addresses long-standing solar physics problems, namely, the heating of the solar chromosphere and the origin of the solar wind. Our aim is to reveal th…
Ultra-high-energy cosmic ray acceleration by magnetic reconnection in relativistic jets and the origin of very high energy emission
E. De Gouveia Dal Pino, T. E. Medina-Torrejon, L. H. S. Kadowaki +2
Relativistic jets are believed to be born magnetically dominated. Very and ultra-high energy cosmic rays can be efficiently accelerated by magnetic reconnection in these sources. W…
Magnetic Field Orientation in Self-Gravitating Turbulent Molecular Clouds
Lucas Barreto-Mota, Elisabete M. de Gouveia Dal Pino, Blakesley Burkhart +3
Stars form inside molecular cloud filaments from the competition of gravitational forces with turbulence and magnetic fields. The exact orientation of these filaments with the magn…
Fast magnetic reconnection structures in Poynting-flux dominated jets
Luís H. S Kadowaki, Elisabete M. de Gouveia Dal Pino, Tania E. Medina Torrejon +2
The ubiquitous relativistic jet phenomena associated with black holes play a major role in high and very-high-energy (VHE) astrophysics. In particular, observations have demonstrat…
Particle acceleration by relativistic magnetic reconnection driven by kink instability turbulence in Poynting flux dominated jets
Tania E. Medina-Torrejon, Elisabete M. de Gouveia Dal Pino, Luis H. S. Kadowaki +3
Particle acceleration in magnetized relativistic jets still puzzles theorists, specially when one tries to explain the highly variable emission observed in blazar jets or gamma-ray…
A statistical study of fast magnetic reconnection in turbulent accretion disks and jets
Luís H. S. Kadowaki, Elisabete M. de Gouveia Dal Pino, Tania E. Medina-Torrejón
Fast magnetic reconnection events can play an important role in accretion disk systems. A potential model to explain the non-thermal very-high-energy (VHE) emission (from GeV to Te…
Particle acceleration and the origin of the very high energy emission around black holes and relativistic jets
Elisabete de Gouveia Dal Pino, Grzegorz Kowal, Luis Kadowaki +3
Particle acceleration induced by fast magnetic reconnection may help to solve current puzzles related to the interpretation of the very high energy (VHE) and neutrino missions from…
MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection
Luis H. S. Kadowaki, Elisabete M. de Gouveia Dal Pino, James M. Stone
Magnetohydrodynamic instabilities play an important role in accretion disks systems. Besides the well-known effects of the magnetorotational instability (MRI), the Parker-Rayleigh-…
Magnetic Reconnection on Jet-Accretion disk Systems
Elisabete M. de Gouveia Dal Pino, Maria Victoria del Valle, Luis H. S. Kadowaki +4
Fast Magnetic Reconnection is currently regarded as an important process also beyond the solar system, specially in magnetically dominated regions of galactic and extragalactic sou…
On the role of fast magnetic reconnection in accreting black hole sources
C. B. Singh, E. M. de Gouveia Dal Pino, L. H. S. Kadowaki
We attempt to explain the observed radio and gamma-ray emission produced in the surrounds of black holes by employing a magnetically-dominated accretion flow (MDAF) model and fast…
The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and low luminosity AGNs
L. H. S. Kadowaki, E. M. de Gouveia Dal Pino, Chandra B. Singh
Fast magnetic reconnection events can be a very powerful mechanism operating in the core region of microquasars and AGNs. In earlier work, it has been suggested that the power rele…
The role of fast magnetic reconnection in acceleration zones of microquasars and AGNs
L. H. S. Kadowaki, E. M. de Gouveia Dal Pino
Fast magnetic reconnection events can be a very powerful mechanism operating at the jet launching region of microquasars and AGNs. We have recently found that the power released by…
The role of magnetic reconnection on jet/accretion disk systems
E. M. de Gouveia Dal Pino, P. P. Piovezan, L. H. S. Kadowaki
It was proposed earlier that the relativistic ejections observed in microquasars could be produced by violent magnetic reconnection episodes at the inner disk coronal region. Here…
Magnetic Field Effects near the launching region of Astrophysical Jets
E. M. de Gouveia Dal Pino, G. Kowal, L. H. S. Kadowaki +2
One of the fundamental properties of astrophysical magnetic fields is their ability to change topology through reconnection and in doing so, to release magnetic energy, sometimes v…
On the role of magnetic reconnection in jet/accretion disk systems
Elisabete M. de Gouveia Dal Pino, Pamela P. Piovezan, Luis H. S. Kadowaki +2
The most accepted model for jet production is based on the magneto-centrifugal acceleration out off an accretion disk that surrounds the central source (Blandford & Payne, 1982). T…