Results 21 to 30 of about 4,707 (204)
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
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Cassini observations of ion and electron beams at Saturn and their relationship to infrared auroral arcs [PDF]
, 2005 We present Cassini Visual and Infrared Mapping Spectrometer observations of infrared auroral emissions from the noon sector of Saturn's ionosphere revealing multiple intense auroral arcs separated by dark regions poleward of the main oval.
Badman, S. V. +16 more
core +4 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
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Radio Emission from UV Cet: Auroral Emission from a Stellar Magnetosphere
The Astrophysical Journal, 2022 Abstract The archetypical flare star UV Cet was observed by MeerKAT on 2021 October 5–6. A large radio outburst with a duration of ∼2 hr was observed between 886 and 1682 MHz, with a time resolution of 8 s and a frequency resolution of 0.84 MHz, enabling sensitive dynamic spectra to be formed. The emission is characterized by three peaks
T. S. Bastian, W. D. Cotton, G. Hallinan
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Radio emission from mini‐magnetospheres on the Moon [PDF]
Geophysical Research Letters, 2004 Small‐scale, localized magnetic anomalies on the surface of planetary satellites effectively create “mini‐magnetospheres”, which can lead to standoff shocks analogous to planetary bow shocks. This gives rise to the tantalizing possibility that radio emission can be produced in the vicinity of such mini‐magnetospheres, since it is well known that radio ...
Zdenka Kuncic, Iver H. Cairns
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Constraints on magnetospheric radio emission from Y dwarfs [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 Abstract As a pilot study of magnetism in Y dwarfs, we have observed the three known infrared variable Y dwarfs WISE J085510.83−071442.5, WISE J140518.40+553421.4, and WISEP J173835.53+273258.9 with the NSF’s Karl G. Jansky Very Large Array in the 4–8 GHz frequency range.
Kao, Melodie M. +2 more
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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
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Stellar wind-magnetosphere interaction at exoplanets: computations of auroral radio powers
, 2016 We present calculations of the auroral radio powers expected from exoplanets with magnetospheres driven by an Earth-like magnetospheric interaction with the solar wind.
Milan, S. E., Nichols, J. D.
core +1 more source
Magnetospheric Radio Emissions from Exoplanets with the SKA [PDF]
Proceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14), 2015 Not ...
Zarka, Philippe +3 more
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High-latitude propagation studies using a meridional chain of LF/MF/HF receivers [PDF]
Annales Geophysicae, 2004 For over a decade, Dartmouth College has operated programmable radio receivers at multiple high-latitude sites covering the frequency range 100-5000kHz with about a 1-s resolution. Besides detecting radio emissions of auroral origin, these receivers
J. LaBelle
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