Martin Pessah
Martin Pessah
Professor MSO, Niels Bohr Institute
E-mail confirmado em nbi.dk - Página inicial
TítuloCitado porAno
Sustained magnetorotational turbulence in local simulations of stratified disks with zero net magnetic flux
SW Davis, JM Stone, ME Pessah
The Astrophysical Journal 713 (1), 52, 2010
2322010
Angular momentum transport in accretion disks: scaling laws in MRI-driven turbulence
ME Pessah, C Chan, D Psaltis
The Astrophysical Journal Letters 668 (1), L51, 2007
1552007
The stability of magnetized rotating plasmas with superthermal fields
ME Pessah, D Psaltis
The Astrophysical Journal 628 (2), 879, 2005
782005
On the saturation of the magnetorotational instability via parasitic modes
ME Pessah, J Goodman
The Astrophysical Journal Letters 698 (1), L72, 2009
742009
The signature of the magnetorotational instability in the Reynolds and Maxwell stress tensors in accretion discs
ME Pessah, C Chan, D Psaltis
Monthly Notices of the Royal Astronomical Society 372 (1), 183-190, 2006
642006
Angular momentum transport in protoplanetary and black hole accretion disks: the role of parasitic modes in the saturation of MHD turbulence
ME Pessah
The Astrophysical Journal 716 (2), 1012, 2010
562010
Viscous, resistive magnetorotational modes
ME Pessah, C Chan
The Astrophysical Journal 684 (1), 498, 2008
522008
Local model for angular-momentum transport in accretion disks driven by the magnetorotational instability
ME Pessah, C Chan, D Psaltis
Physical review letters 97 (22), 221103, 2006
482006
The fundamental difference between shear alpha viscosity and turbulent magnetorotational stresses
ME Pessah, C Chan, D Psaltis
Monthly Notices of the Royal Astronomical Society 383 (2), 683-690, 2007
462007
On the time variability of γ‐ray sources: a numerical analysis of variability indices
DF Torres, ME Pessah, GE Romero
Astronomische Nachrichten 322 (4), 223-227, 2001
422001
Characterizing the mean-field dynamo in turbulent accretion disks
O Gressel, ME Pessah
The Astrophysical Journal 810 (1), 59, 2015
372015
Coronae as a consequence of large-scale magnetic fields in turbulent accretion disks
EG Blackman, ME Pessah
The Astrophysical Journal Letters 704 (2), L113, 2009
302009
Statistical mechanics and the description of the early universe.(I). Foundations for a slightly non-extensive cosmology
ME Pessah, DF Torres, H Vucetich
Physica A: Statistical Mechanics and its Applications 297 (1-2), 164-200, 2001
222001
Compact formulae, dynamics and radiation of charged particles under synchro-curvature losses
D Viganò, DF Torres, K Hirotani, ME Pessah
Monthly Notices of the Royal Astronomical Society 447 (2), 1164-1172, 2014
212014
Gravitational microlensing of γ-ray blazars
DF Torres, GE Romero, EF Eiroa, J Wambsganss, ME Pessah
Monthly Notices of the Royal Astronomical Society 339 (2), 335-352, 2003
202003
Gravitational microlensing of γ-ray blazars
DF Torres, GE Romero, EF Eiroa, J Wambsganss, ME Pessah
Monthly Notices of the Royal Astronomical Society 339 (2), 335-352, 2003
202003
On Hydromagnetic Stresses in Accretion Disk Boundary Layers
ME Pessah, C Chan
The Astrophysical Journal 751 (1), 48, 2012
182012
On the anisotropic nature of MRI-driven turbulence in astrophysical disks
GC Murphy, ME Pessah
The Astrophysical Journal 802 (2), 139, 2015
162015
An assessment of the pulsar outer gap model–I. Assumptions, uncertainties, and implications on the gap size and the accelerating field
D Viganò, DF Torres, K Hirotani, ME Pessah
Monthly Notices of the Royal Astronomical Society 447 (3), 2631-2648, 2015
152015
An assessment of the pulsar outer gap model–II. Implications for the predicted γ-ray spectra
D Viganò, DF Torres, K Hirotani, ME Pessah
Monthly Notices of the Royal Astronomical Society 447 (3), 2649-2657, 2015
132015
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