Short-duration Electron Precipitation Studied by Test Particle Simulation [PDF]
Journal of Astronomy and Space Sciences, 2015 Energy spectra of electron microbursts from 170 keV to 340 keV have been measured by the solid-state detectors aboard the low-altitude (680 km) polar-orbiting Korean STSAT-1 (Science and Technology SATellite).
Jaejin Lee, Kyung-Chan Kim, Jong-Gil Lee
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Anisotropic pitch angle distribution of ~100 keV microburst electrons in the loss cone: measurements from STSAT-1 [PDF]
Annales Geophysicae, 2012 Electron microburst energy spectra in the range of 170 keV to 360 keV have been measured using two solid-state detectors onboard the low-altitude (680 km), polar-orbiting Korean STSAT-1 (Science and Technology SATellite-1).
J. J. Lee +9 more
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Large-Eddy Simulation of a microburst [PDF]
Atmospheric Chemistry and Physics, 2011 The three-dimensional structure and evolution of an isolated and stationary microburst are simulated using a time-dependent, high resolution Large-Eddy-Simulation (LES) model.
V. Anabor +3 more
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Catching the Microburst Culprits with Snappy [PDF]
Proceedings of the Afternoon Workshop on Self-Driving Networks, 2018 Short-lived traffic surges, known as microbursts, can cause periods of unexpectedly high packet delay and loss on a link. Today, preventing microbursts requires deploying switches with larger packet buffers (incurring higher cost) or running the network at low utilization (sacrificing efficiency).
Xiaoqi Chen +4 more
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Microbursts at Meter-Decameter Wavelengths [PDF]
Symposium - International Astronomical Union, 1990 A statistical analysis of Clark Lake microbursts was performed using a data base consisting of ~ 100 bursts. The results are: (1) Microburst sources are well correlated with coronal streamers and active regions. (2) The peak brightness temperature (T^) of the microbursts is in the range 6 × 105 K to 6 × 107 K (see Fig.
G. Thejappa, N. Gopalswamy, M. R. Kundu
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Relativistic Microburst Scale Size Induced by a Single Point‐Source Chorus Element
Geophysical Research Letters, 2022 Relativistic microbursts are impulsive, sub‐second precipitation bursts of relativistic electrons. They are one of the main loss mechanisms of outer radiation belt electrons, and are driven by chorus waves.
Ning Kang +4 more
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Micrometeorological Observations of a Microburst in Southern Finland [PDF]
Boundary-Layer Meteorology, 2007 On the afternoon of 3 July 2004 in Hyytiälä (Juupajoki, Finland), convective cells produced a strong downburst causing forest damage. The SMEAR II field station, situated near the damage site, enabled a unique micrometeorological analysis of a microburst with differences above and inside the canopy.
Järvi, Leena +9 more
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Quantifying the Size and Duration of a Microburst‐Producing Chorus Region on 5 December 2017
Geophysical Research Letters, 2022 Microbursts are impulsive (30 keV) precipitation (FIREBIRD II and AC6 CubeSats, POES) to determine the size of the microburst‐producing chorus source region beginning on 5 December 2017.
S. S. Elliott +20 more
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Simulation of Atmospheric Microbursts Using a Numerical Mesoscale Model at High Spatiotemporal Resolution [PDF]
, 2020 [EN] Atmospheric microbursts are low-level meteorological events that can produce significant damage on the surface and pose a major risk to aircraft flying close to the ground.
Bolgiani, Pedro Mariano +6 more
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Evidence of Microbursts Observed Near the Equatorial Plane in the Outer Van Allen Radiation Belt
Geophysical Research Letters, 2018 We present the first evidence of electron microbursts observed near the equatorial plane in Earth's outer radiation belt. We observed the microbursts on 31 March 2017 with the Magnetic Electron Ion Spectrometer and Radiation Belt Storm Probes Ion ...
Mykhaylo Shumko +9 more
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