Results 81 to 90 of about 4,707 (204)
RAMBO. I. Project Introduction and First Results with uGMRT
Magnetic hot stars can emit both coherent and incoherent nonthermal radio emission. Understanding the nature of these emissions and their connection to stellar rotation and magnetic field characteristics remains incomplete.
Z. Keszthelyi +6 more
doaj +1 more source
Anthropogenic effects on the space environment started in the late 19th century and reached their peak in the 1960s when high-altitude nuclear explosions were carried out by the USA and the Soviet Union.
A. Finkbeiner +157 more
core +1 more source
Differentiating Plumes and Local Torus Segments of Enceladus
Abstract Enceladus's south polar plumes and their surrounding torus segments (local plasma regions formed by plume material diffusion) are key to understanding its magnetospheric interaction; however, clear observational criteria to distinguish them remain lacking.
Shangchun Teng +6 more
wiley +1 more source
Evaluating Star–Planet Interactions with Zeeman Doppler Imaging: Case Study in YZ Ceti
The recent detections of radio emission from the nearby exoplanet host, YZ Ceti, suggest that the star is possibly interacting with its rocky innermost planet.
J. Sebastian Pineda +5 more
doaj +1 more source
Onsite analysis of data from the Dynamics Explorer (DE) spacecraft [PDF]
The tasks performed by ARC Professional Services Group, Inc. fell into five parts: (1) dynamics explorer (DE) data analysis and modeling; (2) DE project support; (3) chemical release observations support; (4) VLF emissions and plasma instability studies;
Candey, Robert M. +2 more
core +1 more source
Radio emission altitudes in the pulsar magnetosphere
Multifrequency timing measurements of four pulsars were used to search for propagation delays predicted by the radius-to-frequency mapping (RFM) model of pulsar radio emission. The RFM model specifies that emissions at different frequencies are produced at different altitudes in the pulsar magnetosphere.
openaire +1 more source
We analyze and model rapid rotations of polarization orientations in PSR B1919+21’s single pulses based on Five-hundred-meter Aperture Spherical radio Telescope observation data.
Shunshun Cao +7 more
doaj +1 more source
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
doaj +1 more source
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
Saturn’s Radio Emissions and their Relation to Magnetospheric Dynamics (invited) [PDF]
With the arrival of the Cassini spacecraft at Saturn in July 2004, there have been quasi-continuous observations of Saturn Kilometric Radiation (SKR) emissions. In this paper we review the response of these emissions to dynamics in Saturn’s magnetosphere, driven by factors internal and external to the system.
openaire +1 more source

