Wave-induced loss of ultra-relativistic electrons in the Van Allen radiation belts [PDF]
The processes that lead to losses of highly energetic particles from Earth’s radiation belts remain poorly understood. Here the authors compare observations and models of a 2013 event to show that electromagnetic ioncyclotron waves provide the dominant ...
Alexander Y Drozdov +2 more
exaly +3 more sources
Discovery and insights from DSX mission’s high-power VLF wave transmission experiments in the radiation belts [PDF]
Space weather phenomena can threaten space technologies. A hazard among these is the population of relativistic electrons in the Van Allen radiation belts.
P. Song +20 more
doaj +2 more sources
Formation of electron radiation belts at Saturn by Z-mode wave acceleration [PDF]
Radial diffusion is the only mechanism considered to accelerate trapped electrons to relativistic energies in Saturn’s magnetic field, forming radiation belts.
E. E. Woodfield +5 more
doaj +2 more sources
Ganymede's Radiation Cavity and Radiation Belts
While planetary radiation belts are all embedded within the low energy solar wind, Ganymede is in the unique situation of being surrounded by the energetic particles of Jupiter's magnetosphere.
P. Kollmann +6 more
doaj +2 more sources
Van Allen Radiation Belts: An Important Challenge for Astrobiology Missions [PDF]
Manned space missions account for a large proportion of future space travel missions.Van Allen radiation belts are major challenges of space missions with an astrobiology approach.
Iman Shafieenejad +2 more
doaj +1 more source
EVIDENCE OF THE EARTH’S INNER RADIATION BELTS DURING THE LOW SOLAR AND GEOMAGNETIC ACTIVITY OBTAINED WITH THE STEP-F INSTRUMENT [PDF]
Purpose: The subject of research is the spatio-temporal charged particles in the Earth’s magnetosphere outside the South Atlantic magnetic Anomaly during the 11-year cycle of solar activity minimum.
O. V. Dudnik, O. V. Yakovlev
doaj +1 more source
The magnetic field of the solar corona has a large-scale dipole character, which maps into the bipolar field in the solar wind. Using standard representations of the coronal field, we show that high-energy ions can be trapped stably in these large-scale closed fields.
Hudson, H. S. +3 more
openaire +2 more sources
Radial Transport in the Earth’s Radiation Belts: Linear, Quasi-linear, and Higher-order Processes
Observational studies of the Earth’s radiation belts indicate that Alfvénic fluctuations in the frequency range of 2–25 mHz accelerate electrons to relativistic energies.
Adnane Osmane +4 more
doaj +1 more source
Reconstruction of the Radiation Belts for Solar Cycles 17–24 (1933–2017)
We present a reconstruction of the dynamics of the radiation belts from solar cycles 17 to 24 which allows us to study how radiation belt activity has varied between the different solar cycles.
A. A. Saikin +5 more
doaj +1 more source
OMEP-EOR: A MeV proton flux specification model for electric orbit raising missions
Electric Orbit Raising (EOR) for telecommunication satellites significantly reduced on-board fuel mass at the price of extended transfer durations. These relatively long transfers, which usually span a few months, cross large spans of the radiation belts,
Brunet Antoine +4 more
doaj +1 more source

