Results 21 to 30 of about 4,735 (200)
Six pieces of evidence against the corotation enforcement theory to explain the main aurora at Jupiter [PDF]
, 2020 The most remarkable feature of the ultraviolet auroras at Jupiter is the ever present and almost continuous curtain of bright emissions centered on each magnetic pole and called the main emissions.
Bonfond, Bertrand +2 more
core +1 more source
The Astrophysical Journal, 2023 Although the majority of hot magnetic stars have extremely stable, ∼kilogauss strength surface magnetic fields with simple topologies, a subset undergoes small-scale explosions due to centrifugal breakout.
Emil Polisensky +5 more
doaj +1 more source
Earth and Planetary Physics, 2022 Locating the source of decametric (DAM) radio emissions is a key step in the use of remote radio observations to understand the Jovian magnetospheric dynamics and their interaction with the planet’s moons. Wang YM et al.
YuMing Wang +5 more
doaj +1 more source
Detecting Magnetospheric Radio Emission from Giant Exoplanets
The Astrophysical Journal, 2022 Abstract As radio astronomy enters a golden age, ground-based observatories are reaching sensitivities capable of unlocking a new and exciting field of exoplanet observation. Radio observation of planetary auroral emission provides unique and complementary insight into planetary science not available via orthodox exoplanet observation ...
Reza Ashtari +3 more
openaire +1 more source
A Blind Search for Magnetospheric Emissions from Planetary Companions to Nearby Solar-type Stars
, 2009 This paper reports a blind search for magnetospheric emissions from planets around nearby stars. Young stars are likely to have much stronger stellar winds than the Sun, and because planetary magnetospheric emissions are powered by stellar winds ...
Aubier +33 more
core +1 more source
Cassini observations of narrowband radio emissions in Saturn's magnetosphere [PDF]
Journal of Geophysical Research: Space Physics, 2010 The Radio and Plasma Wave Science instrument (RPWS) on board the Cassini spacecraft has detected numerous narrowband radio emissions in Saturn's magnetosphere from September 2005 to May 2007. Typically, the narrowband radio emissions occur after an intensification of Saturn kilometric radiation (SKR) and last for several days.
Z. Wang +7 more
openaire +1 more source
The Astrophysical Journal Letters, 2023 The presence of magnetic fields in the late inspiral of black hole–neutron star binaries could lead to potentially detectable electromagnetic precursor transients.
Elias R. Most, Alexander A. Philippov
doaj +1 more source
The Saturnian Kilometric Radiation before the Cassini Grand Finale
, 2017 The Saturnian Kilometric Radiation (SKR) is radiated from the auroral regions surrounding the kronian magnetic poles, above the ionosphere up to a few planetary radii.
Lamy, Laurent
core +2 more sources
On the Transition from Accretion Powered to Rotation Powered Millisecond Pulsars [PDF]
, 2010 The heating associated with the deposition of $\gamma$-rays in an accretion disk is proposed as a mechanism to facilitate the transformation of a low mass X-ray binary to the radio millisecond pulsar phase. The $\gamma$-ray emission produced in the outer
Archibald +14 more
core +2 more sources
Cyclotron absorption of radio emission within pulsar magnetospheres [PDF]
Monthly Notices of the Royal Astronomical Society, 2001 ABSTRA C T Absorption of radio emission through normal cyclotron resonance within pulsar magnetospheres is considered. The optical depth for cyclotron damping is calculated using a plasma distribution with an intrinsically relativistic spread. We argue that such a broad distribution is plausible for pulsar plasmas and that it implies that a class of ...
Q. Luo, D. B. Melrose
openaire +1 more source