Results 81 to 90 of about 18,719 (213)
ULF Waves above the Nightside Auroral Oval during Substorm Onset [PDF]
This chapter reviews historical ground-based observations of ultra-low-frequency (ULF) waves tied to substorms, and highlights new research linking these ULF waves explicitly to substorm onset itself.
Rae, I, Rae, IJ, Watt, CEJ
core
Abstract Auroral kilometric radiation (AKR) provides a sensitive probe of magnetospheric dynamics during substorms. We analyze an extended data set of AKR bursts observed by the WIND spacecraft to investigate how the frequency structure of AKR responds to substorm onset and evolution.
Simon James Walker +4 more
wiley +1 more source
Abstract Short Large‐Amplitude Magnetic Structures (SLAMS) are believed to play important roles in the physics governing the formation of quasi‐parallel shocks. These isolated non‐linear structures, frequently observed in the foreshock, have been suggested to be building blocks for the shock and have been shown to drive shock reformation. In this work,
S. Bergman, T. Karlsson, T. K. Wong Chan
wiley +1 more source
The modulation of electromagnetic ion cyclotron waves by Pc 5 ULF waves [PDF]
The modulation of electromagnetic ion cyclotron (EMIC) waves by longer-period ULF waves has been proposed as a method for producing pearl structured Pc 1–2 EMIC waves.
T. M. Loto'aniu +3 more
doaj +1 more source
Abstract From 1974 to 1975, the Mariner 10 spacecraft studied Mercury's environment during three flybys and detected hydrogen, helium, and possibly atomic oxygen in the exosphere using its ultraviolet spectrometer, but no molecular hydrogen. Based on the sensitivity of the occultation instrument, an upper limit for the H2 ${\mathrm{H}}_{2}$ surface ...
F. Weichbold +8 more
wiley +1 more source
Abstract A simulation of the 10 May 2024 geomagnetic storm is used to investigate the theory of cross polar cap potential (CPCP) saturation in Earth's magnetosphere‐ionosphere system. THEMIS B (ARTEMIS P1) satellite magnetic field and plasma measurements at lunar distance upstream in the solar wind drives the Space Weather Modeling Framework (SWMF) in ...
A. Brenner +7 more
wiley +1 more source
Ultra-relativistic electron flux enhancement under persistent high speed solar wind stream
The physical mechanisms usually applied to explain the relativistic electron enhancement have been delved into to elucidate non-adiabatic electron acceleration resulting in the ultra-relativistic electron population observed in the outer radiation belt ...
L. R. Alves +8 more
doaj +1 more source
Chiral dynamics in few-nucleon systems [PDF]
We employ the chiral nucleon-nucleon potential derived using the method of unitary transformation up to next-to-next-to-leading order (NNLO) to study bound and scattering states in the two-nucleon system.
Elster, C. +6 more
core +4 more sources
INPRESS: INvasive PRESSure Monitoring Knowledge and Practice Survey
ABSTRACT Background In patients on Intensive Care Units (ICU), invasive arterial pressure monitoring with closed transducer systems is widely used, yet the accuracy of measurement depends on correct zeroing, levelling and interpretation of arterial waveforms.
Oliver Coolens +4 more
wiley +1 more source
Role of ULF Waves in Reforming the Martian Bow Shock
Understanding the nature of planetary bow shocks is beneficial for advancing our knowledge of solar wind interactions with planets and fundamental plasma physics processes.
Chi Zhang +12 more
doaj +1 more source

