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Open AccessMachine learning emulator for physics-based prediction of ionospheric potential response to solar wind variations
Physics-based simulations are important for elucidating the fundamental mechanisms behind the time-varying complex ionospheric conditions, such as ionospheric potential, against unprecedented solar wind variat...
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Article
Open AccessLocalized mesospheric ozone destruction corresponding to isolated proton aurora coming from Earth’s radiation belt
Relativistic electron precipitation (REP) from the Earth’s radiation belt plays an important role in mesospheric ozone loss as a connection between space weather and the climate system. However, the rapid (ten...
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Open AccessPSTEP: project for solar–terrestrial environment prediction
Although solar activity may significantly impact the global environment and socioeconomic systems, the mechanisms for solar eruptions and the subsequent processes have not yet been fully understood. Thus, mode...
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Open AccessSpace weather benchmarks on Japanese society
We surveyed the relationship between the scale of space weather events and their occurrence rate in Japan, and we discussed the social impact of these phenomena during the Project for Solar–Terrestrial Environ...
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Open AccessCorrection to: Small-Scale Dynamic Aurora
A Correction to this paper has been published: https://doi.org/10.1007/s11214-021-00821-y
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Open AccessEditorial: Topical Collection on Auroral Physics
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Open AccessSmall-Scale Dynamic Aurora
Small-scale dynamic auroras have spatial scales of a few km or less, and temporal scales of a few seconds or less, which visualize the complex interplay among charged particles, Alfvén waves, and plasma instab...
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Open AccessExtreme geomagnetic activities: a statistical study
Statistical distributions are investigated for magnetic storms, sudden commencements (SCs), and substorms to identify the possible amplitude of the one in 100-year and 1000-year events from a limited data set ...
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Diffuse and Pulsating Aurora
This chapter reviews fundamental properties and recent advances of diffuse and pulsating aurora. Diffuse and pulsating aurora often occurs on closed field lines and involves energetic electron precipitation by...
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Dayside Aurora
Dayside aurora is related to processes in the dayside magnetosphere and especially at the dayside magnetopause. A number of dayside aurora phenomena are driven by reconnection between the solar wind interplane...
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Open AccessTransient ionization of the mesosphere during auroral breakup: Arase satellite and ground-based conjugate observations at Syowa Station
Transient mesospheric echo in the VHF range was detected at an altitude of 65–70 km during the auroral breakup that occurred from 2220 to 2226 UT on June 30, 2017. During this event, the footprint of the Arase...
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Open AccessVisualization of rapid electron precipitation via chorus element wave–particle interactions
Chorus waves, among the most intense electromagnetic emissions in the Earth’s magnetosphere, magnetized planets, and laboratory plasmas, play an important role in the acceleration and loss of energetic electro...
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Open AccessGround-based instruments of the PWING project to investigate dynamics of the inner magnetosphere at subauroral latitudes as a part of the ERG-ground coordinated observation network
The plasmas (electrons and ions) in the inner magnetosphere have wide energy ranges from electron volts to mega-electron volts (MeV). These plasmas rotate around the Earth longitudinally due to the gradient an...
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Open AccessExtreme geomagnetically induced currents
We propose an emergency alert framework for geomagnetically induced currents (GICs), based on the empirically extreme values and theoretical upper limits of the solar wind parameters and of dB/dt, the time deriva...
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Open AccessExtremely severe space weather and geomagnetically induced currents in regions with locally heterogeneous ground resistivity
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Open AccessInterplanetary particle transport simulation for warning system for aviation exposure to solar energetic particles
Solar energetic particles (SEPs) are one of the extreme space weather phenomena. A huge SEP event increases the radiation dose received by aircrews, who should be warned of such events as early as possible. We...
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Open AccessGlobal MHD simulation of magnetospheric response of preliminary impulse to large and sudden enhancement of the solar wind dynamic pressure
A sudden increase in the dynamic pressure of solar wind generates a prominent and transient change in ground-based magnetometer records worldwide, which is called a sudden commencement (SC). The magnetic field...
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Open AccessEstimating the solar wind conditions during an extreme geomagnetic storm: a case study of the event that occurred on March 13–14, 1989
The solar wind conditions of an extreme geomagnetic storm were examined using magnetic field observations obtained from geosynchronous satellites and the disturbance storm-time (Dst) index. During geosynchrono...
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Open AccessWhat caused the rapid recovery of the Carrington storm?
The geomagnetic storm during the Carrington event, which occurred on 2 September 1859, displayed extremely rapid recovery. The geomagnetic field increased by approximately 650 nT/h at Bombay, India, and by >30...
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Open AccessCompound auroral micromorphology: ground-based high-speed imaging
Auroral microphysics still remains partly unexplored. Cutting-edge ground-based optical observations using scientific complementary metal-oxide semiconductor (sCMOS) cameras recently enabled us to observe the ...