☆ 4.3 Review

Space Plasma Physics: A Review

IEEE TRANSACTIONS ON PLASMA SCIENCE (2022)

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Article Astronomy & Astrophysics

Near-Earth Sub-Alfvenic Solar Winds: Interplanetary Origins and Geomagnetic Impacts

Rajkumar Hajra et al.

Summary: The near-Earth solar wind is typically faster than the Alfvenic and magnetosonic speeds. However, sub-Alfvenic solar winds have been identified, with the majority occurring within interplanetary coronal mass ejection magnetic clouds (MCs). These events are characterized by low plasma densities, temperatures, enhanced magnetic field intensities, and speeds. The remaining sub-Alfvenic intervals occur in the trailing portions of solar wind high-speed streams (HSSs), with low plasma densities and temperatures. These sub-Alfvenic solar winds have minimal impact on Earth's magnetosphere and outer radiation belt relativistic electrons.

ASTROPHYSICAL JOURNAL (2022)

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Article Geosciences, Multidisciplinary

Acceleration of Electrons by Whistler-Mode Hiss Waves at Saturn

E. E. Woodfield et al.

Summary: Plasmaspheric hiss waves at Saturn accelerate electrons instead of causing losses, due to the different plasma density environment. The interaction between electrons and hiss occurs at high latitudes, resulting in acceleration with mid to low pitch angles.

GEOPHYSICAL RESEARCH LETTERS (2022)

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Article Materials Science, Multidisciplinary

Dust-ion-acoustic waves in a x-nonthermal magnetized collisional dusty plasma with opposite polarity dust

M. R. Hassan et al.

Summary: A four-component magnetized collisional x-nonthermal plasma containing stationary dust grains of opposite charges, inertial ion fluid, and non-inertial x-distributed superthermal electrons has been studied to examine the properties of different modes of dust-ion-acoustic waves (DIAWs). The damped Zakharov-Kuznetsov-Burgers equation is derived using a reductive perturbation method and its solutions are used to analyze the characteristics of dust-ion-acoustic solitary and shock waves. The impact of relevant physical plasma parameters on the dust-ion-acoustic soliton and shock characteristics is examined, as well as the effect of the coexistence of oppositely charged dust grains.

RESULTS IN PHYSICS (2022)

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Article Astronomy & Astrophysics

Observations of Pole-to-Pole, Stratosphere-to-Ionosphere Connection

L. P. Goncharenko et al.

Summary: The behavior of the Earth's middle atmosphere and ionosphere is influenced by multiple processes, including energy transfer from the Sun and magnetosphere as well as from terrestrial weather. Recent developments in research infrastructure, particularly in Antarctica, have allowed for the observation of new ionospheric features. For the first time, it has been shown that disturbances occurring in the Arctic winter polar stratosphere can propagate across the globe and cause large disturbances in the summertime ionospheric plasma over Antarctica.

FRONTIERS IN ASTRONOMY AND SPACE SCIENCES (2022)

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Article Multidisciplinary Sciences

Tree-rings reveal two strong solar proton events in 7176 and 5259 BCE

Nicolas Brehm et al.

Summary: The Sun occasionally produces intense solar energetic particle (SEP) events that disrupt the near-Earth radiation environment. By analyzing C-14 concentrations in tree-rings, two spikes in atmospheric C-14 occurring in ancient times were discovered, providing critical information on the occurrence of extreme solar events in the past.

NATURE COMMUNICATIONS (2022)

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Review Astronomy & Astrophysics

Space Weather: From solar origins to risks and hazards evolving in time

Natalia Buzulukova et al.

Summary: Space Weather, a branch of space physics, has direct impacts on humankind and its effects have become more diverse with the advancement of human technologies. The risks and hazards of Space Weather originate from the variability of solar processes and could potentially have serious impacts on technological systems and human health.

FRONTIERS IN ASTRONOMY AND SPACE SCIENCES (2022)

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Article Astronomy & Astrophysics

Modeling Meteoroid Impacts on the Juno Spacecraft

Petr Pokorny et al.

Summary: This study analyzes star-tracker images from the Juno spacecraft and finds that the proposed events are unlikely to be caused by interplanetary dust particle impacts on its solar arrays. The predicted dust-impact rates from dynamical meteoroid models do not match the observed event rates and variations in dust flux. The hypothesis of dust leaving Mars or its moons also fails to reproduce the variations in star-tracker event rates observed by Juno.

PLANETARY SCIENCE JOURNAL (2022)

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Article Astronomy & Astrophysics

Student Dust Counter Status Report: The First 50 au

Edwin Bernardoni et al.

Summary: The Venetia Burney Student Dust Counter (SDC) is an in situ dust detector that provides near-continuous measurements of interplanetary dust particle (IDP) distribution. It has been used to study the outer solar system and the dominant source of IDP, the Edgeworth-Kuiper Belt (EKB). The updated dust density distribution to 50 au and the effects of IDP generation, transport, and loss on EKB objects are discussed. SDC measurements are critical for understanding the large-scale structure of the EKB and interpreting dust disks around other stars.

PLANETARY SCIENCE JOURNAL (2022)

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Article Engineering, Aerospace

WAAS and the Ionosphere - A Historical Perspective: Monitoring Storms

Lawrence Sparks et al.

Summary: This paper discusses the protection of aircraft position estimates accuracy and integrity by WAAS, including ionospheric disturbance monitoring, storm detector implementation, algorithm evolution, and ranking of the largest ionospheric storms in the past two solar cycles.

NAVIGATION-JOURNAL OF THE INSTITUTE OF NAVIGATION (2022)

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Article Astronomy & Astrophysics

Switchbacks: statistical properties and deviations from Alfvenicity

A. Larosa et al.

Summary: The first solar encounter of the Parker Solar Probe has revealed the presence of sudden magnetic field deflections in the slow Alfvenic solar wind, known as switchbacks. These structures are often associated with proton velocity enhancements. Statistical analysis shows that switchbacks are Alfvenic in 73% of cases and compressible in 27%. The boundaries of these structures can be interpreted in terms of rotational or tangential discontinuities.

ASTRONOMY & ASTROPHYSICS (2021)

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Article Astronomy & Astrophysics

Relation of Microstreams in the Polar Solar Wind to Switchbacks and Coronal X-Ray Jets

Marcia Neugebauer et al.

Summary: The study found a high correlation between microstreams and switchbacks in the magnetic field during periods of minimum solar activity, suggesting that microstreams may be the result of the alternation of patches of switchbacks and quiet periods. This alternation could be caused by minifilament/flux rope eruptions that lead to coronal jets.

ASTROPHYSICAL JOURNAL LETTERS (2021)

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Article Astronomy & Astrophysics

The Interplanetary and Magnetospheric causes of Geomagnetically Induced Currents (GICs) > 10 A in the Mantsala Finland Pipeline: 1999 through 2019

Bruce T. Tsurutani et al.

Summary: Interplanetary and magnetospheric phenomena coinciding with intense geomagnetically induced current (GIC) events at the Mantsala, Finland gas pipeline from 1999 to 2019 have been studied. Although forward shocks and substorms are the main causes of intense GICs, new geoeffective interplanetary features such as solar wind plasma parcel (PP) impingements have been discovered. Analysis of >30 A GIC events revealed that supersubstorm and intense substorm auroral electrojet intensifications are the most common causes, with PPs and forward shocks also playing significant roles. The two Halloween superstorms in 2003 produced the greatest number of GIC events, with a shock-triggered supersubstorm causing the most intense event of the study.

JOURNAL OF SPACE WEATHER AND SPACE CLIMATE (2021)

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Article Astronomy & Astrophysics

Discontinuity analysis of the leading switchback transition regions

M. Akhavan-Tafti et al.

Summary: The study found that 78% of the leading switchback transition regions are rotational discontinuities, while 21% are categorized as either discontinuity. The ratio of RD-to-ED events decreases with increasing distance from the Sun. Significant jumps in proton temperature and prevalence of bad curvature are observed at leading RD-type switchback transition regions, indicating a possible evolution from RD-type to ED-type magnetic discontinuities.

ASTRONOMY & ASTROPHYSICS (2021)

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Review Astronomy & Astrophysics

Small-Scale Dynamic Aurora

Ryuho Kataoka et al.

Summary: This passage describes the characteristics of small-scale dynamic auroras and the development of related theories.

SPACE SCIENCE REVIEWS (2021)

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Editorial Material Astronomy & Astrophysics

Editorial: Topical Collection on Auroral Physics

David J. Knudsen et al.

SPACE SCIENCE REVIEWS (2021)

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Article Astronomy & Astrophysics

Geomagnetic Pulsations Driving Geomagnetically Induced Currents

M. J. Heyns et al.

Summary: GICs are driven by the geoelectric field induced by fluctuations of Earth's magnetic field, which are associated with large impulsive events and geomagnetic field oscillations. Low-frequency pulsations drive significant GICs, even at midlatitudes, due to the low-pass nature of GICs. Longer-period disturbances not typical of midlatitudes are observed with GIC amplitudes comparable to storm sudden commencement peak GICs.

SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS (2021)

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Article Astronomy & Astrophysics

Extreme-Event Magnetic Storm Probabilities Derived From Rank Statistics of Historical Dst Intensities for Solar Cycles 14-24

Jeffrey J. Love

Summary: This study compiled and fitted the maximum magnetic storm intensities from solar cycles 14-24, estimating storm intensity and the probability of future storms exceeding certain thresholds.

SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS (2021)

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Article Astronomy & Astrophysics

The Satellite Risk Prediction and Radiation Forecast System (SaRIF)

Richard B. Horne et al.

Summary: As new satellite technologies are being developed and the risk of space weather affecting satellites increases, there is a growing need to develop services to protect satellites. By discussing with satellite operators, designers, underwriters, and space agency staff, 10 user needs were identified and a satellite risk prediction system was proposed to meet these needs.

SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS (2021)

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Article Geochemistry & Geophysics

Distribution of Interplanetary Dust Detected by the Juno Spacecraft and Its Contribution to the Zodiacal Light

J. L. Jorgensen et al.

Summary: The Solar System contains a cloud of dust that scatters light and includes bands of dust orbiting near the ecliptic plane. Dust detectors on spacecraft have detected few particles due to limited aperture and sparsity. Interplanetary dust impacts on the Juno spacecraft have provided new insights into the distribution of dust particles and suggest a primary source near the Mars orbit plane. The measured dust distribution, influenced by orbital resonances with Jupiter, provides an alternative explanation for the observed variation of Zodiacal Light with ecliptic latitude.

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS (2021)

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Article Astronomy & Astrophysics

The Onset of a Substorm and the Mating Instability

Gerhard Haerendel et al.

Summary: The paper discusses the appearance and nonlinear growth of beading independently from the onset of reconnection, as well as the processes related to the onset arc breakup. The instability of the onset arc is traced back to a high-beta plasma layer, while the observation of auroral streamers provides valuable insights for analysis.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2021)

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Article Astronomy & Astrophysics

Periodicities and Colors of Pulsating Auroras: DSLR Camera Observations From the International Space Station

Sota Nanjo et al.

Summary: This study investigated the spatial characteristics of pulsating auroras using digital camera measurements from the International Space Station. The results suggest that the periodicity of the main pulsation of a PsA is not dependent on magnetic latitude and MLT, but rather on local conditions. The study also found that the B/G ratios in pulsating auroras can be used as proxies for the energies of PsA electrons, with higher ratios observed in the morning sector.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2021)

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Review Astronomy & Astrophysics

Carrington Events

Hugh S. Hudson

Summary: The Carrington event in 1859 serves as a prototype for studying extreme solar events and their potential threats to Earth and Earth-like exoplanets. Recent geophysical and photometry data have broadened our perspective on these events and their implications for solar-type stars. Comparing solar microphysics with related stellar phenomena can provide insights into potential superflare events in the future.

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 59 (2021)

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Article Astronomy & Astrophysics

PSP/WISPR observations of dust density depletion near the Sun I. Remote observations to 8 R⊙ from an observer between 0.13 and 0.35 AU

G. Stenborg et al.

Summary: This study used data from the PSP mission to investigate the dust environment near the Sun and found a dust density depletion zone, which is beyond the original theoretical expectations.

ASTRONOMY & ASTROPHYSICS (2021)

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Article Astronomy & Astrophysics

An M Dwarf's Chromosphere, Corona, and Wind Connection via Nonlinear Alfven Waves

Takahito Sakaue et al.

Summary: This study reveals that the atmosphere of M dwarfs is more magnetized, cooler, and denser compared to the Sun, with faster stellar winds and smaller mass-loss rates. The nonlinear propagation of Alfven waves plays a crucial role in heating the stellar atmosphere and driving stellar wind, as shown through simulations.

ASTROPHYSICAL JOURNAL (2021)

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Article Geosciences, Multidisciplinary

A Strong Correlation Between Relativistic Electron Microbursts and Patchy Aurora

M. Shumko et al.

Summary: The study demonstrates a high correlation between high-energy electron microbursts and patchy auroras, with a correlation coefficient of 0.8. This indicates a strong association between the dynamics of relativistic radiation belt electrons and keV electron precipitation, showing that they cannot be studied in isolation.

GEOPHYSICAL RESEARCH LETTERS (2021)

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Article Astronomy & Astrophysics

Detecting the surface composition of geological features on Europa and Ganymede using a surface dust analyzer

William Goode et al.

Summary: Europa and Ganymede are likely to have subsurface oceans and young surface features provide an opportunity to sample material for understanding evolution and habitability. A model was developed to detect the composition of ejecta from surface features accurately for close flybys, such as those planned for NASA's Europa Clipper mission.

PLANETARY AND SPACE SCIENCE (2021)

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Review Instruments & Instrumentation

Laboratory plasma devices for space physics investigation

Yu Liu et al.

Summary: Laboratory experiments have significantly contributed to the exploration of fundamental physics of space plasmas over the past decades. Researchers reviewed the initiation, development, and current status of laboratory plasma devices, categorized and discussed them according to central scientific research topics, and provided challenges and suggestions for future research. The objective is to enhance knowledge of experimental apparatuses and techniques, promoting the development of space physics through a combination of spacecraft observation, numerical simulation, and laboratory experiments.

REVIEW OF SCIENTIFIC INSTRUMENTS (2021)

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Review Astronomy & Astrophysics

The Relativistic Electron-Proton Telescope (REPT) Investigation: Design, Operational Properties, and Science Highlights

Daniel N. Baker et al.

Summary: This paper briefly reviews the design, operational performance, mode changes and trends of the REPT instruments, as well as corrections for relevant background effects. It highlights significant discoveries and advancements in understanding physical processes obtained using REPT data, particularly for energetic electrons in the outer Van Allen belt and energetic protons in the inner Van Allen zone. The paper also discusses the importance of continuing REPT-like measurements for both science and space situational awareness.

SPACE SCIENCE REVIEWS (2021)

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Article Astronomy & Astrophysics

Birth of a Magnetosphere

Hans Nilsson et al.

Summary: A magnetosphere can form around an object in a stellar wind either due to the intrinsic magnetic field of the object or stellar wind interaction with the ionosphere of the object. Through the study of the birth and evolution of a comet magnetosphere as the comet nucleus approached the Sun, we gain insights into the characteristics of comet magnetospheres and the changes in solar wind-atmosphere interaction.

MAGNETOSPHERES IN THE SOLAR SYSTEM (2021)

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Article Astronomy & Astrophysics

Overview of Moon-Magnetosphere Interactions

Joachim Saur

Summary: Moon-magnetosphere interaction refers to the interaction between a moon orbiting within a host planet's magnetosphere with the planet's magnetospheric plasma. This interaction helps in understanding the basic physics of plasma flows in the universe and provides geophysical information about the moons' interiors. The interaction is influenced by various factors both locally near the moon and further away in the magnetospheric plasma.

MAGNETOSPHERES IN THE SOLAR SYSTEM (2021)

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Article Astronomy & Astrophysics

Collisional Evolution of the Inner Zodiacal Cloud

J. R. Szalay et al.

Summary: The zodiacal cloud, influenced by meteoroid collisions, contains three distinct populations of dust grains: alpha-meteoroids on elliptic orbits, beta-meteoroids on hyperbolic orbits, and impactors that may be from discrete meteoroid streams or their collisional by-products. The Geminids meteoroid stream's beta-stream is a likely candidate for the third population of impactors. Collisional erosion in the zodiacal cloud primarily occurs within 10-20 solar radii, with a zodiacal erosion rate of approximately 100 kg s(-1) and a flux of beta-meteoroids at 1 au of (0.4-0.8) x 10(-4) m(-2) s(-1) consistent with observed impact rates.

PLANETARY SCIENCE JOURNAL (2021)

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Article Astronomy & Astrophysics

Dust Directionality and an Anomalous Interplanetary Dust Population Detected by the Parker Solar Probe

A. Pusack et al.

Summary: Theory and previous space missions suggest the existence of multiple populations of zodiacal dust, with alpha- and beta-meteoroids being the most prominent. The Parker Solar Probe (PSP) has observed dust populations that do not align with current models, potentially indicating the presence of additional dust populations. An anomaly in dust impact directionality post-perihelion during Orbit 4 suggests the existence of another dust population related to the Geminids meteoroid stream associated with asteroid 3200 Phaethon.

PLANETARY SCIENCE JOURNAL (2021)

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Article Astronomy & Astrophysics

The Formation of Electron Outflow Jets with Power-law Energy Distribution in Guide-field Magnetic Reconnection

H. Che et al.

Summary: Observationally, electron beams with power-law energy spectra are commonly associated with solar flares. Previous studies have found that electron beams are unable to develop during magnetic reconnection with a guide field B-g larger than 0.1 times the asymptotic field B-0 due to the strong deflection caused by the guide field. Using particle-in-cell simulations, it is shown that in force-free reconnection, the development of an electron Kelvin-Helmholtz instability can suppress the Hall effect and produce a flute-like outflow exhaust, resulting in collimated jets with a power-law energy spectrum.

ASTROPHYSICAL JOURNAL (2021)

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Article Astronomy & Astrophysics

Statistical Properties of Superflares on Solar-type Stars: Results Using All of the Kepler Primary Mission Data

Soshi Okamoto et al.

Summary: A study was conducted on solar-type and Sun-like stars to analyze superflares using Kepler and Gaia data, finding that the frequency of superflares decreases as the stellar rotation period increases. The maximum energy of superflares on Sun-like stars was found to be 4 x 10^34 erg, with the Sun potentially causing similar X700-class and X1000-class flares every approximately 3000 and 6000 years, respectively.

ASTROPHYSICAL JOURNAL (2021)

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Article Astronomy & Astrophysics

Full compressible 3D MHD simulation of solar wind

Takuma Matsumoto

Summary: This study utilized a three-dimensional simulation to differentiate between heating mechanisms in the fast solar wind, confirming Alfven turbulence as the dominant heating mechanism in the acceleration region. Shock formation and phase mixing were also found to be important in the lower transition region.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

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Review Astronomy & Astrophysics

Quiet, Discrete Auroral Arcs-Observations

T. Karlsson et al.

SPACE SCIENCE REVIEWS (2020)

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Review Astronomy & Astrophysics

Aurora in the Polar Cap: A Review

Keisuke Hosokawa et al.

SPACE SCIENCE REVIEWS (2020)

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Review Astronomy & Astrophysics

Diffuse and Pulsating Aurora

Yukitoshi Nishimura et al.

SPACE SCIENCE REVIEWS (2020)

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Article Multidisciplinary Sciences

Multiple time-scale beats in aurora: precise orchestration via magnetospheric chorus waves

K. Hosokawa et al.

SCIENTIFIC REPORTS (2020)

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Article Geochemistry & Geophysics

Juno Waves Detection of Dust Impacts Near Jupiter

S. -Y. Ye et al.

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS (2020)

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Review Astronomy & Astrophysics

Quiet, Discrete Auroral Arcs: Acceleration Mechanisms

R. Lysak et al.

SPACE SCIENCE REVIEWS (2020)

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Article Astronomy & Astrophysics

Zodiacal light observations and its link with cosmic dust: A review

Jeremie Lasue et al.

PLANETARY AND SPACE SCIENCE (2020)

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Article Astronomy & Astrophysics

The Impenetrable Barrier: Suppression of Chorus Wave Growth by VLF Transmitters

John C. Foster et al.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2020)

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Article Astronomy & Astrophysics

Lower-Band Monochromatic Chorus Riser Subelement/Wave Packet Observations

Bruce T. Tsurutani et al.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2020)

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Article Astronomy & Astrophysics

The Near-Sun Dust Environment: Initial Observations from Parker Solar Probe

J. R. Szalay et al.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2020)

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Article Astronomy & Astrophysics

Turbulence Spectra of Electron Density and Magnetic Field Fluctuations in the Local Interstellar Medium

K. H. Lee et al.

ASTROPHYSICAL JOURNAL (2020)

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Article Astronomy & Astrophysics

Switchbacks in the Solar Magnetic Field: Their Evolution, Their Content, and Their Effects on the Plasma

F. S. Mozer et al.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2020)

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Article Astronomy & Astrophysics

Examining Dust Directionality with the Parker Solar Probe FIELDS Instrument

Brent Page et al.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2020)

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Article Astronomy & Astrophysics

In Situ Observations of Interplanetary Dust Variability in the Inner Heliosphere

David M. Malaspina et al.

ASTROPHYSICAL JOURNAL (2020)

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Article Geosciences, Multidisciplinary

The physics of space weather/solar-terrestrial physics (STP): what we know now and what the current and future challenges are

Bruce T. Tsurutani et al.

NONLINEAR PROCESSES IN GEOPHYSICS (2020)

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Article Astronomy & Astrophysics

Energy Transfer by Nonlinear Alfven Waves in the Solar Chromosphere and Its Effect on Spicule Dynamics, Coronal Heating, and Solar Wind Acceleration

Takahito Sakaue et al.

ASTROPHYSICAL JOURNAL (2020)

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Review Astronomy & Astrophysics

Circumplanetary Dust Populations

Frank Spahn et al.

SPACE SCIENCE REVIEWS (2019)

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Article Multidisciplinary Sciences

Direct observations of a surface eigenmode of the dayside magnetopause

M. O. Archer et al.

NATURE COMMUNICATIONS (2019)

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Article Geochemistry & Geophysics

Meteoroids at the Moon: Orbital Properties, Surface Vaporization, and Impact Ejecta Production

Petr Pokorny et al.

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS (2019)

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Review Astronomy & Astrophysics

Interplanetary Dust, Meteoroids, Meteors and Meteorites

Detlef Koschny et al.

SPACE SCIENCE REVIEWS (2019)

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Article Astronomy & Astrophysics

The Solar and Interplanetary Causes of Superstorms (Minimum Dst ≤-250 nT) During the Space Age

Xing Meng et al.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2019)

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Article Astronomy & Astrophysics

Magnetospheric Multiscale Observations of ULF Waves and Correlated Low-Energy Ion Monoenergetic Acceleration

B. Li et al.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2019)

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Article Geosciences, Multidisciplinary

Rapid Electron Acceleration in Low-Density Regions of Saturn's Radiation Belt by Whistler Mode Chorus Waves

E. E. Woodfield et al.

GEOPHYSICAL RESEARCH LETTERS (2019)

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Review Astronomy & Astrophysics

Coronal Mass Ejections over Solar Cycles 23 and 24

P. L. Lamy et al.

SPACE SCIENCE REVIEWS (2019)

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Article Astronomy & Astrophysics

Effects of VLF Transmitter Waves on the Inner Belt and Slot Region

J. P. J. Ross et al.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2019)

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Article Geochemistry & Geophysics

On the seasonal and solar cycle variation of the ULF fluctuations at low latitudes: A comparison with the ionospheric parameters

U. Villante et al.

JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS (2019)

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Article Astronomy & Astrophysics

Satellite Orbital Drag During Magnetic Storms

D. M. Oliveira et al.

SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS (2019)

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Review Astronomy & Astrophysics

The Dawn of Dust Astronomy

Eberhard Gruen et al.

SPACE SCIENCE REVIEWS (2019)

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Review Astronomy & Astrophysics

Interstellar Dust in the Solar System

Veerle J. Sterken et al.

SPACE SCIENCE REVIEWS (2019)

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Review Astronomy & Astrophysics

Dayside Aurora

Harald U. Frey et al.

SPACE SCIENCE REVIEWS (2019)

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Article Astronomy & Astrophysics

Drifting of the line-tied footpoints of CME flux-ropes

Guillaume Aulanier et al.

ASTRONOMY & ASTROPHYSICS (2019)

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Article Astronomy & Astrophysics

Diagnosing solar wind origins using in situ measurements in the inner heliosphere

D. Stansby et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

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Article Multidisciplinary Sciences

Near-Sun observations of an F-corona decrease and K-corona fine structure

R. A. Howard et al.

NATURE (2019)

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Article Multidisciplinary Sciences

Visualization of rapid electron precipitation via chorus element wave-particle interactions

Mitsunori Ozaki et al.

NATURE COMMUNICATIONS (2019)

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Article Astronomy & Astrophysics

Low Frequency (f < 200 Hz) Polar Plasmaspheric Hiss: Coherent and Intense

Bruce T. Tsurutani et al.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2019)

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Article Astronomy & Astrophysics

A New MHD Model with a Rotated-hybrid Scheme and Solenoidality-preserving Approach

Xueshang Feng et al.

ASTROPHYSICAL JOURNAL (2019)

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Article Astronomy & Astrophysics

The detectability of radio emission from exoplanets

C. R. Lynch et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2018)

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Article Physics, Fluids & Plasmas

Laboratory space physics: Investigating the physics of space plasmas in the laboratory

Gregory G. Howes

PHYSICS OF PLASMAS (2018)

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Article Astronomy & Astrophysics

Quasi-electrostatic twisted waves in Lorentzian dusty plasmas

Kashif Arshad et al.

PLANETARY AND SPACE SCIENCE (2018)

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Article Astronomy & Astrophysics

Lunar dust and dusty plasmas: Recent developments, advances, and unsolved problems

S. I. Popel et al.

PLANETARY AND SPACE SCIENCE (2018)

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Article Astronomy & Astrophysics

Effects of interplanetary coronal mass ejections on the transport of nano-dust generated in the inner solar system

Leela O'Brien et al.

PLANETARY AND SPACE SCIENCE (2018)

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Article Astronomy & Astrophysics

Determining the Mode, Frequency, and Azimuthal Wave Number of ULF Waves During a HSS and Moderate Geomagnetic Storm

Kyle R. Murphy et al.

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2018)

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Energetic outer zone electron loss timescales during low geomagnetic activity

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JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2006)

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lAn explanation of the Voyager paradox: Particle acceleration at a blunt termination shock

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GEOPHYSICAL RESEARCH LETTERS (2006)

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Arbitrary amplitude dust-acoustic double layers in a non-thermal plasma

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The process of electron acceleration during collisionless magnetic reconnection

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PHYSICS OF PLASMAS (2006)

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Charged dust and shock phenomena in the Solar System

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NONLINEAR PROCESSES IN GEOPHYSICS (2006)

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Dispersion analysis of low-frequency waves through the terrestrial bow shock

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Complex (dusty) plasmas: Current status, open issues, perspectives

VE Fortov et al.

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS (2005)

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Simulation of the outer radiation belt electrons near geosynchronous orbit including both radial diffusion and resonant interaction with Whistler-mode chorus waves

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GEOPHYSICAL RESEARCH LETTERS (2005)

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Visibility of coronal mass ejections as a function of flare location and intensity

S Yashiro et al.

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Crossing the termination shock into the hetiosheath:: Magnetic fields

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Voyager 1 in the foreshock, termination shock, and heliosheath

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Electron plasma oscillations upstream of the solar wind termination shock

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Voyager 1 explores the termination shock region and the heliosheath beyond

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Wave acceleration of electrons in the Van Allen radiation belts

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Magnetic pulsations: Their sources and relation to solar wind and geomagnetic activity

R McPherron

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Geomagnetic storm of 29-31 October 2003: Geomagnetically induced currents and their relation to problems in the Swedish high-voltage power transmission system

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A parametric study of the influence of non-thermal ions on linear dust-acoustic waves in an unmagnetized dusty plasma

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Dayside global ionospheric response to the major interplanetary events of October 29-30, 2003 Halloween storms

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GEOPHYSICAL RESEARCH LETTERS (2005)

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Low-latitude auroras observed in Japan: 1999-2004

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Timescale for radiation belt electron acceleration by whistler mode chorus waves

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Direct evidence for magnetic reconnection in the solar wind near 1 AU

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Mixed particle acceleration at CME-driven shocks and flares

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GEOPHYSICAL RESEARCH LETTERS (2005)

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Statistical distributions of speeds of coronal mass ejections

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The October 28, 2003 extreme EUV solar flare and resultant extreme ionospheric effects: Comparison to other Halloween events and the Bastille Day event

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Nonlinear Alfven waves, discontinuities, proton perpendicular acceleration, and magnetic holes/decreases in interplanetary space and the magnetosphere: intermediate shocks?

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Initial results of a survey of equatorial noise emissions observed by the Cluster spacecraft

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Differential velocity between solar wind protons and alpha particles in pressure balance structures

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Global dayside ionospheric uplift and enhancement associated with interplanetary electric fields

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A catalog of white light coronal mass ejections observed by the SOHO spacecraft

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Plasma clouds associated with Comet P Borrelly dust impacts

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Systematic analysis of equatorial noise below the lower hybrid frequency

O Santolik et al.

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Dust near the Sun

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Solar cycle variations of the electron radiation belts: Observations and radial diffusion simulation

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Acceleration of coronal mass ejections

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A kinetic approach to the Ponderomotive Force

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GEOPHYSICAL RESEARCH LETTERS (2003)

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Particle acceleration and coronal mass ejection driven shocks: Shocks of arbitrary strength

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Diffuse auroral electron scattering by electron cyclotron harmonic and whistler mode waves during an isolated substorm

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Spatio-temporal structure of storm-time chorus -: art. no. 1278

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The extreme magnetic storm of 1-2 September 1859

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Statistical analysis of relativistic electron energies for cyclotron resonance with EMIC waves observed on CRRES

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Evaluation of quasi-linear diffusion coefficients for EMIC waves in a multispecies plasma

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Two components in major solar particle events

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GEOPHYSICAL RESEARCH LETTERS (2003)

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Relativistic electron acceleration and precipitation during resonant interactions with whistler-mode chorus

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GEOPHYSICAL RESEARCH LETTERS (2003)

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Resonant diffusion of radiation belt electrons by whistler-mode chorus

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Controlled precipitation of radiation belt electrons

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Shock aurora: FAST and DMSP observations

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Relativistic electron pitch-angle scattering by electromagnetic ion cyclotron waves during geomagnetic storms

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Prominence eruptions and coronal mass ejection: A statistical study using microwave observations

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Energetic particle acceleration and transport at coronal mass ejection-driven shocks

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Penetration of the solar wind electric field into the magnetosphere/ionosphere system

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Properties of small-scale Alfve'n waves and accelerated electrons from FAST

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Evolution of energetic electron pitch angle distributions during storm time electron acceleration to megaelectronvolt energies

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Coronal Mass Ejection (CME)-induced shock formation, propagation and some temporally and spatially developing shock parameters relevant to particle energization

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NONLINEAR PROCESSES IN GEOPHYSICS (2003)

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SPACE SCIENCE REVIEWS (2003)

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Phase-steepened Alfven waves, proton perpendicular energization and the creation of magnetic holes and magnetic decreases: The ponderomotive force

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GIC observations and studies in the Hydro-Quebec power system

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A first approach to model the low-frequency wave activity in the plasmasphere

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Oblique 1-Hz whistler mode waves in an electron foreshock: The Cassini near-Earth encounter

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Recordings and occurrence of geomagnetically induced currents in the Finnish natural gas pipeline network

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On the temporal relationship between coronal mass ejections and flares

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Interplanetary shock triggering of nightside geomagnetic activity: Substorms, pseudobreakups, and quiescent events

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Substorm dependence of chorus amplitudes: Implications for the acceleration of electrons to relativistic energies

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JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS (2001)

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Parametric decay of oblique arc-polarized Alfven waves

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GEOPHYSICAL RESEARCH LETTERS (2001)

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Ion distributions in large magnetic holes in the fast solar wind

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Observations of relativistic electron microbursts in association with VLF chorus

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The electron and ion plasma experiment for FAST

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Magnetically-driven planetary radio emissions and application to extrasolar planets

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An emerging flux trigger mechanism for coronal mass ejections

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Composition of quasi-stationary solar wind flows from ulysses/solar wind ion composition spectrometer

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Proton and electron heating by radially propagating fast magnetosonic waves

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Particle acceleration and coronal mass ejection driven shocks: A theoretical model

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A review on the genesis of coronal mass ejections

TG Forbes

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Magnetic field depressions in the solar wind

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Relationship of halo coronal mass ejections, magnetic clouds, and magnetic storms

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On the processing and transport of inner source hydrogen

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Surface waves in strongly irradiated dusty plasmas

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Identification of the coronal sources of the fast solar wind

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