Minyi Long
YOU?
Author Swipe
View article: A slot region in the magnetosphere of Jupiter
A slot region in the magnetosphere of Jupiter Open
Understanding the balance between charged particle acceleration and loss is central to radiation belt research. Jupiter’s Galilean moons orbit within its intense radiation environment and can act both as sources and sinks of energetic part…
View article: Spatial Distribution of Ion Cyclotron Waves at Io
Spatial Distribution of Ion Cyclotron Waves at Io Open
Ion cyclotron waves at Io are important for understanding the complex interactions between Io and Jupiter's magnetosphere. In this study, we analyze the spatial distributions of ion cyclotron waves at Io using data from seven close flybys …
View article: Long-term enhancing of Jupiter’s electrostatic waves as diagnostic of Io’s mass loading activity
Long-term enhancing of Jupiter’s electrostatic waves as diagnostic of Io’s mass loading activity Open
http://dx.doi.org/10.13039/501100012166 National Key Research and Development Program of China
View article: Resonant Scattering of Radiation Belt Electrons by Saturnian Z‐Mode Waves
Resonant Scattering of Radiation Belt Electrons by Saturnian Z‐Mode Waves Open
We investigated the resonant interactions between Z‐mode waves and radiation belt electrons at Saturn via constructing an empirical model of the frequency spectral and wave normal angle distributions of 5 and 20 kHz Saturnian Z‐mode waves …
View article: Modulation of suprathermal electron fluxes by ultra-low-frequency magnetic field fluctuations in the Martian foreshock
Modulation of suprathermal electron fluxes by ultra-low-frequency magnetic field fluctuations in the Martian foreshock Open
Ultra-low-frequency (ULF) waves are ubiquitous in terrestrial and planetary environments, playing a crucial role in energy transfer and dissipation through wave–particle interactions within space plasmas. By performing a detailed event stu…
View article: Generation of 30 s Waves Observed Upstream of the Martian Bow Shock: A Case Study
Generation of 30 s Waves Observed Upstream of the Martian Bow Shock: A Case Study Open
The foreshock region filled with turbulences is a natural lab for studying interactions between plasma and waves. The underlying processes are vital for dissipating the energy carried by the solar wind into the Martian environment. In this…
View article: Formation of an Extended Equatorial Shadow Zone for Low‐Frequency Saturn Kilometric Radiation
Formation of an Extended Equatorial Shadow Zone for Low‐Frequency Saturn Kilometric Radiation Open
Saturn Kilometric Radiation (SKR), being the dominant radio emission at Saturn, has been extensively investigated. The low‐frequency extension of SKR is of particular interest due to its strong association with Saturn's magnetospheric dyna…
View article: Whistler-mode and ULF waves and their association with solar wind plasmas observed upstream of Martian bow shock
Whistler-mode and ULF waves and their association with solar wind plasmas observed upstream of Martian bow shock Open
Whistler-mode and ULF waves upstream of planetary bow shock play important role in energy transfer and dissipation processes in the planetary environment. A series of whistler-mode waves with their frequencies centered at ~0.4 Hz, accompan…
View article: Unusually Low-frequency Whistler-mode Waves and Their Association with High-energy Protons Observed Upstream of Martian Bow Shock
Unusually Low-frequency Whistler-mode Waves and Their Association with High-energy Protons Observed Upstream of Martian Bow Shock Open
Whistler-mode waves upstream of planetary bow shock are often referred to as “1-Hz waves” due to the center of their observed frequency range being at ∼1 Hz. A series of whistler-mode waves were observed upstream of the Martian bow shock b…
View article: Loss of energetic electrons in the vicinity of Io
Loss of energetic electrons in the vicinity of Io Open
Io plays a dual role in the Jovian magnetosphere, that is, its active volcanism provides a main plasma source of the magnetosphere, and it loses energetic particles within radiation belts as well which has been observed by spacecraft (Gali…
View article: Phase locking among Saturn radio emissions revealed by<i>Cassini</i>observations
Phase locking among Saturn radio emissions revealed by<i>Cassini</i>observations Open
Context. Rotational modulation has been observed in different magnetospheric phenomena at Saturn, including radio emissions, which reflect the fundamental plasma processes in key regions. Though previous studies have shown Saturn’s kilomet…
View article: Formation of Electron Butterfly Pitch Angle Distributions in Saturn's Magnetosphere Due To Scattering by Equatorial ECH Waves
Formation of Electron Butterfly Pitch Angle Distributions in Saturn's Magnetosphere Due To Scattering by Equatorial ECH Waves Open
The features of electron pitch angle distributions (PADs) often imply different physical mechanisms in planetary magnetospheres. We report a simultaneous equatorial electrostatic electron cyclotron harmonic (ECH) wave event with butterfly …
View article: Excitation of Saturnian ECH Waves Within Remote Plasma Injections: Cassini Observations
Excitation of Saturnian ECH Waves Within Remote Plasma Injections: Cassini Observations Open
Based on Cassini observations, we report representative electrostatic electron cyclotron harmonic (ECH) wave events observed in Saturn's magnetosphere within remote plasma injections. Unlike local injections, remote injections are “older” …
View article: Resonant Scattering of Radiation Belt Electrons at Saturn by Ion Cyclotron Waves
Resonant Scattering of Radiation Belt Electrons at Saturn by Ion Cyclotron Waves Open
By constructing an empirical model of the spectral and latitudinal distribution of ion cyclotron waves on the basis of Cassini datasets, we investigate the resonant interactions between ion cyclotron waves and radiation belt electrons at S…
View article: <strong>Formation of electron butterfly pitch angle distributions in Saturn’s magnetosphere due to scattering by ECH waves</strong>
<strong>Formation of electron butterfly pitch angle distributions in Saturn’s magnetosphere due to scattering by ECH waves</strong> Open
The data can be used to reproduce results in our study. If you have any other questions, please email to [email protected].
View article: <strong>Formation of electron butterfly pitch angle distributions in Saturn’s magnetosphere due to scattering by equatorial ECH waves</strong>
<strong>Formation of electron butterfly pitch angle distributions in Saturn’s magnetosphere due to scattering by equatorial ECH waves</strong> Open
The data can be used to reproduce results in our study. If you have any other questions, please email to [email protected].
View article: Reflection and Refraction of the L-O Mode 5 kHz Saturn Narrowband Emission by the Magnetosheath&#160;
Reflection and Refraction of the L-O Mode 5 kHz Saturn Narrowband Emission by the Magnetosheath  Open
<div class="page" title="Page 1"> <div class="layoutArea"> <div class="column"> <p>The reflection-by-sheath mechanism of 5 kHz narrowband emissions (NB) at Saturn is confirmed…
View article: Saturn Anomalous Myriametric Radiation, a New Type of Saturn Radio Emission Revealed by Cassini
Saturn Anomalous Myriametric Radiation, a New Type of Saturn Radio Emission Revealed by Cassini Open
A new radio component namely Saturn Anomalous Myriametric Radiation (SAM) is reported. A total of 193 SAM events have been identified by using all the Cassini Saturn orbital data. SAM emissions are L‐O mode radio emission and occasionally …
View article: Statistics of Water-group Band Ion Cyclotron Waves in Saturn's Inner Magnetosphere Based on 13 yr of Cassini Measurements
Statistics of Water-group Band Ion Cyclotron Waves in Saturn's Inner Magnetosphere Based on 13 yr of Cassini Measurements Open
Based on Cassini observations from 2004 to 2016, we perform a comprehensive analysis of the statistical distribution of the occurrence rate, averaged amplitude, wave normal angle (WNA), ellipticity, and power spectral intensity of ion cycl…
View article: Statistical distribution of ion cyclotron waves in Saturn&#8217;s inner magnetosphere: A survey of Cassini measurements between 2004 and 2016
Statistical distribution of ion cyclotron waves in Saturn’s inner magnetosphere: A survey of Cassini measurements between 2004 and 2016 Open
<p>Based on Cassini observations from 2004 to 2016, we perform a comprehensive analysis of the statistical distribution of the occurrence rate, averaged amplitude, wave normal angle (WNA), ellipticity and power spectral intensity of …
View article: Reflection and Refraction of the L‐O Mode 5 kHz Saturn Narrowband Emission by the Magnetosheath
Reflection and Refraction of the L‐O Mode 5 kHz Saturn Narrowband Emission by the Magnetosheath Open
The reflection‐by‐sheath mechanism of 5 kHz narrowband emissions (NB) at Saturn is confirmed by Cassini observations during several crossings of the magnetopause, which show that the 5 kHz NB can be prevented from escaping Saturn's magneto…
View article: Losses of Radiation Belt Energetic Particles by Encounters With Four of the Inner Moons of Jupiter
Losses of Radiation Belt Energetic Particles by Encounters With Four of the Inner Moons of Jupiter Open
Based on an improved model of the moon absorption of Jovian radiation belt particles, we investigate quantitatively and comprehensively the absorption probabilities and particle lifetimes due to encounters with four of the inner moons of J…
View article: Excitation of Saturnian ECH waves within remote plasma injections: Cassini Observations
Excitation of Saturnian ECH waves within remote plasma injections: Cassini Observations Open
The date can be used to reproduce results in our papers.
View article: Distribution of O<sup>+</sup> and ${\text{O}}_{\text{2}}^{\text{+}}$ fluxes and their escape rates in the near-Mars magnetotail: A survey of MAVEN observations
Distribution of O<sup>+</sup> and ${\text{O}}_{\text{2}}^{\text{+}}$ fluxes and their escape rates in the near-Mars magnetotail: A survey of MAVEN observations Open
Tailward ion outflows in the Martian-induced magnetotail are known to be one of the major channels for Martian atmospheric escape. On the basis of nearly 6.5 years of observations from the Mars Atmosphere and Volatile EvolutioN (MAVEN) mis…
View article: Excitation of Saturnian ECH waves within remote plasma injections: Cassini Observations
Excitation of Saturnian ECH waves within remote plasma injections: Cassini Observations Open
The data can be used to reproduce results in our paper.
View article: Excitation of Saturnian ECH waves within remote plasma injections: Cassini Observations
Excitation of Saturnian ECH waves within remote plasma injections: Cassini Observations Open
The data can be used to reproduce results in our paper.
View article: Statistical Study on Spatial Distribution and Polarization of Saturn Narrowband Emissions
Statistical Study on Spatial Distribution and Polarization of Saturn Narrowband Emissions Open
The spatial distribution and polarization of Saturn narrowband (NB) emissions have been studied by using Cassini Radio and Plasma Wave Sciences data and goniopolarimetric data obtained through an inversion algorithm with a preset source lo…
View article: Losses of radiation belt energetic particles by encounters with four of the inner moons of Jupiter
Losses of radiation belt energetic particles by encounters with four of the inner moons of Jupiter Open
The database are helpful, if anyone would like to reproduce our results in this work.
View article: Losses of radiation belt energetic particles by encounters with four of the inner moons of Jupiter
Losses of radiation belt energetic particles by encounters with four of the inner moons of Jupiter Open
The database are helpful, if anyone would like to reproduce our results in this work.
View article: Statistical distribution of ion cyclotron waves in Saturn’s inner magnetosphere: A survey of Cassini measurements between 2004 and 2016
Statistical distribution of ion cyclotron waves in Saturn’s inner magnetosphere: A survey of Cassini measurements between 2004 and 2016 Open
These data help to reproduece results in our manuscript. If you have any question, please email to [email protected].