Results 71 to 80 of about 279 (164)
PSR B0943+10: Mode Switch, Polar Cap Geometry, and Orthogonally Polarized Radiation
As one of the paradigm examples to probe into pulsar magnetospheric dynamics, PSR B0943+10 (J0946+0951) manifests representatively, showing a mode switch, orthogonal polarization, and subpulse drifting, frequently studied below 600 MHz.
Shunshun Cao +12 more
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Many transients believed to originate from magnetars are thought to be triggered by crustal activity, which feeds back on the surrounding magnetosphere. These perturbations, through a variety of proposed mechanisms, can convert a fraction of the magnetic
Louis Burnaz +2 more
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Candidates for detecting exoplanetary radio emissions generated by magnetosphere—ionosphere coupling [PDF]
Abstract In this Letter we consider the magnetosphere—ionosphere (M—I) coupling at Jupiter-like exoplanets with internal plasma sources such as volcanic moons, and we have determined the best candidates for detection of these radio emissions by estimating the maximum spectral flux density expected from planets orbiting stars within 25 pc
openaire +2 more sources
Periodically Modulated Magnetic Reconnection
We present the first evidence for periodically modulated reconnection at the electron scale in space, using unparalleled, high-cadence data from Magnetospheric Multiscale spacecraft.
Chengming Liu +4 more
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Juno in situ observations provide insightful data on plasma, electric, and magnetic fields associated with Jovian decametric (DAM) emission, while remote-sensing observations offer broader spatial and temporal coverage.
Ruobing Zheng +2 more
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HR 5907 (HD 142184) stands out among magnetic OB stars for its rapid rotation, exceptionally hard X-ray emission, and strong magnetic field. High-frequency (>5 GHz) radio emission from the star exhibits an approximately flat spectrum that can be ...
Ayan Biswas +4 more
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Origin of Pulsed Radio Emission from Magnetars
Extended periods of radio pulsations have been observed for six magnetars, displaying characteristics different from those of ordinary pulsars.
Shuzhe Zeng +4 more
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Modeling the transport and anisotropy of energetic electrons in solar flares
Transport of energetic electrons in the flare loop is important to understanding nonthermal emissions in solar flares. In this work, we model the propagation of electrons by numerically solving the particle transport equation which includes the physics ...
Xiangliang Kong +5 more
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ACTIVITY REPORT : Section 7. Magnetospheric Radio Emissions
+12 more sources
Radio Prospects of Extrasolar Aurorae Polaris as a Probe of Planetary Magnetism
Magnetized exoplanets are expected to emit auroral cyclotron radiation in the radio regime due to the interactions between their magnetospheres, the interplanetary magnetic field, and the stellar wind.
Asaf Kaya, Tansu Daylan
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