Results 71 to 80 of about 2,743,097 (252)
Abstract A new proton radiation belt was identified during the geomagnetic superstorm of 10–11 May 2024. To investigate its origin, we use an MHD‐test particle simulation to model solar energetic proton (SEP) trapping and the evolution of the initial trapped proton population during the storm.
Murong Qin +10 more
wiley +1 more source
First Results From Sonification and Exploratory Citizen Science of Magnetospheric ULF Waves: Long‐Lasting Decreasing‐Frequency Poloidal Field Line Resonances Following Geomagnetic Storms [PDF]
Magnetospheric ultralow‐frequency (ULF) waves contribute to space weather in the solar wind‐magnetosphere‐ionosphere system. The monitoring of these waves by space‐ and ground‐based instruments, however, produces big data, which are difficult to navigate,
M. Archer +5 more
semanticscholar +1 more source
Modeling ULF waves in a compressed dipole magnetic field
This paper presents the results of a linear model for global scale magneto-hydrodynamic (MHD) waves in a compressed dipole model magnetosphere. We examine scenarios where a localized monochromatic source along the magnetopause boundary launches MHD fast ...
Kabin, Konstantin +4 more
core +1 more source
Abstract Ground‐based very low frequency transmitters emit signals that primarily propagate within the Earth–ionosphere waveguide, and some of their energy can propagate into the magnetosphere. Ionospheric observations from the DEMETER satellite reveal a distinct concentric rings pattern of the wave power distribution of the North West Cape transmitter
Zhiyang Xia +8 more
wiley +1 more source
Listening to the Magnetosphere: How Best to Make ULF Waves Audible
Observations across the heliosphere typically rely on in situ spacecraft observations producing time-series data. While often this data is analysed visually, it lends itself more naturally to our sense of sound.
Martin O. Archer +8 more
doaj +1 more source
Resonant ULF waves: A new interpretation
Many important properties of ultra‐low frequency (ULF) magnetic pulsations (∼1 to 10 minute periods) observed in the magnetosphere and by ground‐based magnetometers have been interpreted successfully in terms of resonant field line models. These models describe the pulsations as transverse hydromagnetic waves standing on dipole flux tubes with fixed ...
Margaret G. Kivelson, David J. Southwood
openaire +1 more source
Multisatellite studies of ULF waves
Multisatellite studies of ULF waves are reviewed, with a special emphasis on compressional Pc 5 waves. The observations of the radial extent, azimuthal wave number and the field-aligned standing wave structure of the waves are described. When combined with plasma data, the waves appear to be consistent with drift-mirror waves originating from the ...
openaire +1 more source
Precipitation of MeV and Sub‐MeV Electrons Due to Combined Effects of EMIC and ULF Waves
We explore the mechanism of MeV and sub‐MeV electron precipitations into the atmosphere in the outer radiation belt, through quasi‐linear pitch‐angle scattering by electromagnetic ion cyclotron (EMIC) waves, when strong compressional Pc4–Pc5 ultralow ...
X.‐J. Zhang +4 more
semanticscholar +1 more source
A Case Study of Nonresonant Mode 3‐s ULF Waves Observed by MMS
The nature of the 3‐s ultralow frequency (ULF) wave in the Earth's foreshock region and the associated wave‐particle interaction are not yet well understood. We investigate the 3‐s ULF waves using Magnetospheric Multiscale (MMS) observations.
Shan Wang +7 more
semanticscholar +1 more source
We investigate the propagation of whistler-mode waves in ultralow frequency (ULF) wave-derived magnetic ducts using ray tracing simulations in a two-dimensional dipole coordinate system on the meridian plane. The refractive index modulation caused by the
Kohki Tachi, Yuto Katoh
doaj +1 more source

