Results 61 to 70 of about 475 (211)
Temporal Variations of Jupiter's Plasma Disk Observed by Juno
Abstract In Jupiter's magnetosphere, a key question is how plasma is transported outward from its source near Io to the distant magnetotail. Since 2016, the plasma disk has been extensively observed by the Juno mission. Using plasma data from the JADE instrument, we perform an analysis revealing significant temporal variation. For different Juno orbits,
Jian‐Zhao Wang +9 more
wiley +1 more source
Sporadic E-like Topside Layer Driven by Wind Shear in the Martian Ionosphere
Ionospheric plasma density disturbances significantly affect radio wave propagation, impacting communication and planetary exploration. At Earth, sporadic E layers (Es) are commonly observed. They are characterized by thin, high-density plasma structures
Rong Tian +10 more
doaj +1 more source
Excitation of planetary electromagnetic waves in the inhomogeneous ionosphere [PDF]
Abstract. In this paper we develop a new method for the analysis of excitation and propagation of planetary electromagnetic waves (PEMW) in the ionosphere of the Earth. The nonlinear system of equations for PEMW, valid for any height, from D to F regions, including intermediate altitudes between D and E and between E and F regions, is derived.
Yu. Rapoport +6 more
openaire +3 more sources
Unprecedented Extreme Dust Storm Triggered by Stratosphere‐Troposphere Interactions
Abstract An unprecedented dust storm struck southern China in April 2025, affecting hundreds of millions of people in regions rarely impacted by dust storms and challenging existing understanding of lower‐latitude dust storms. Here, we show that polar stratospheric signals enabled this event by modulating tropospheric teleconnection, revealing an ...
Wenqi Zhang +6 more
wiley +1 more source
Ionospheres and atmospheres of non-magnetic planets and solar wind interaction: Part I – Venus [PDF]
349-356The solar-planetary interaction is unique for non-magnetic planets, since the solar wind interacts directly with the atmospheres and ionospheres of these planets.
Dwivedi, A K, Mahajan, K K
core
Solar activity variations of the ionospheres of Venus and Mars [PDF]
Extreme ultraviolet and X-ray photons from the Sun generate a partially ionized region in the atmosphere of a planet called an ionosphere. Solar activity, including solar flares, coronal mass ejections, and changes in the ionizing irradiance affect ...
Hensley, Kerrin G.
core
Abstract We present conjugate observations of ionospheric small‐scale magnetic perturbations (dB) $(dB)$ and GPS scintillations from the Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) and the Canadian High Arctic Ionospheric Network (CHAIN) during a storm‐time substorm on 9 August 2025 in the nightside auroral region ...
Yangyang Shen +12 more
wiley +1 more source
A Study of the reactions of Al⁺ ions with O₃, N₂, O₂, CO₂ and H₂O: influence on Al⁺ chemistry in planetary ionospheres [PDF]
The reactions between Al+(31S) and O3, O2, N2, CO2 and H2O were studied using the pulsed laser ablation at 532 nm of an aluminium metal target in a fast flow tube, with mass spectrometric detection of Al+ and AlO+.
Plane, JMC, Bones, DL, Daly, SM
core +1 more source
Magnetic Reconnection inside a Martian Ion Plume: MAVEN Observations
The Martian ion plume is an important escape channel that influences the long-term evolution of the planet’s atmosphere, yet the small-scale dynamics within plumes remain poorly constrained by in situ observations.
Pu Yang +7 more
doaj +1 more source
Pre‐Existing Plasmaspheric Density Structure
Abstract We perform a basic model experiment: we run two nearly identical plasmapause simulations, differing only by their initial conditions. The first run contains initial fine‐scale and mesoscale structure, and the second run is initialized with a featureless, circular plasmapause.
J. Goldstein, M. F. Thomsen
wiley +1 more source

