Results 11 to 20 of about 2,303,549 (257)
Nuclear β-decays in plasmas: how to correlate plasma density and temperature to the activity [PDF]
Magnetized plasmas in compact traps may become experimental en-vironments for the investigation of nuclear beta-decays of astrophysical inter-est. In the framework of the project PANDORA (Plasmas for Astrophysics, Nuclear Decays Observation and Radiation
Naselli Eugenia +12 more
doaj +1 more source
Tearing Modes in Partially Ionized Astrophysical Plasma [PDF]
In many astrophysical environments the plasma is only partially ionized, and therefore the interaction of charged and neutral particles may alter both the triggering of reconnection and its subsequent dynamical evolution.
F. Pucci +3 more
semanticscholar +1 more source
Magnetohydrodynamic instabilities are related to different characteristics and behavior of fluids. Here the authors report an experiment and simulation combined study of a global non-axisymmetric MHD instability that exists at sufficiently large rotation
Yin Wang +6 more
doaj +1 more source
Astrophysical jets are plasma flows, which are observed to substantially maintain their transverse size while travelling distances orders-of-magnitude larger.
S.K.H. Auluck, A.B. Blagoev
doaj +1 more source
Plasmoid-mediated reconnection during nonlinear peeling–ballooning edge-localized modes
Plasmoid-mediated reconnection is investigated for nonlinear peeling–ballooning edge-localized modes (P-B ELMs). The formation of current sheets and the transition to 3D current sheet instability is demonstrated through fully nonlinear resistive MHD ...
Fatima Ebrahimi, Amitava Bhattacharjee
doaj +1 more source
Behavior of substorm auroral arcs and Pi2 waves: implication for the kinetic ballooning instability [PDF]
We present synoptic observations of the 21 December 2006 substorm event by the THEMIS ground-based All-Sky-Imagers, the ISUAL CCD Imager aboard the FORMOSAT-2 satellite, the geosynchronous satellites and the ground-based magnetometers, and discuss the
T. F. Chang +6 more
doaj +1 more source
The study of relativistic electron–positron pair plasmas is both of fundamental physics interest and important to understand the processes that shape the magnetic field dynamics, particle acceleration, and radiation emission in high-energy astrophysical ...
Hui-Hwa Chen, F. Fiuza
semanticscholar +1 more source
Acoustic oscillations in a field-free cavity under solar small-scale bipolar magnetic canopy [PDF]
Observations show the increase of high-frequency wave power near magnetic network cores and active regions in the solar lower atmosphere. This phenomenon can be explained by the interaction of acoustic waves with a magnetic field.
D. Kuridze +4 more
doaj +1 more source
Nonlinear coupling of electromagnetic and electron acoustic waves in multi-species degenerate astrophysical plasma [PDF]
Nonlinear wave-coupling is studied in a multispecies degenerate astrophysical plasma consisting of two electron species (at different temperatures): a highly degenerate main component plus a smaller classical relativistic flow immersed in a static ...
N. Shatashvili +2 more
semanticscholar +1 more source
Plasma environment effects on K lines of astrophysical interest [PDF]
Aims.Within the framework of compact-object accretion disks, we calculate plasma environment effects on the atomic structure and decay parameters used in the modeling of K lines in lowly charged iron ions, namely Fe II–Fe VIII.Methods.For this study, we ...
J. Deprince +7 more
semanticscholar +1 more source

