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Helio-latitude Dependence of the Solar Wind Parameters and the Magneto-Gravitational Dragging of the Solar Wind
A theoretical model of the magnetic-field coupling to the background gravitational field of a rotating Sun-like star is used here to calculate the...
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Solar Wind and Space Weather
Hot coronal plasma cannot be confined by the gravitational field of the Sun and gradually flows out into interplanetary space, forming the solar...
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Annual Variations in the Near-Earth Solar Wind
Earth’s orbit and rotation produces systematic variations in geomagnetic activity, most notably via the changing orientation of the dayside...
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Solar Wind or Solar Breeze?
Long before the advent of research enabled by rockets, scientists speculated about the physical processes external to stars. That is, in addition to...
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Multi-source connectivity as the driver of solar wind variability in the heliosphere
The ambient solar wind that fills the heliosphere originates from multiple sources in the solar corona and is highly structured. It is often...
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Causal Analysis of Influence of the Solar Cycle and Latitudinal Solar-Wind Structure on Co-Rotation Forecasts
Studying solar-wind conditions is central to forecasting the impact of space weather on Earth. Under the assumption that the structure of this wind...
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Quantum-enhanced multi-objective collaboration for wind and solar hydrogen storage optimization
In pursuit of the “Dual Carbon Goals” and to mitigate the adverse effects of “power supply restrictions,” a microgrid scheme integrating wind and...
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Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind
The tendency for low-speed solar wind to show greater spatiotemporal variability and different compositional properties from high-speed wind has led...
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Comparative Analysis of Various Machine-Learning Models for Solar-Wind Propagation-Delay Estimation
Geomagnetic storms resulting from solar disturbances impact telecommunication and satellite systems. Satellites are positioned at Lagrange point L1...
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Solar wind plasma variations with interplanetary magnetic field during solar cycles 22–24
In this paper, we have studied the relationship between the monthly variations of solar wind plasma velocity, interplanetary magnetic field (IMF) and...
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Cross-Scale Phase Relationship of the Ca II K Index with Solar Wind Parameters: A Space Climate Focus
The solar wind, representing one of the most impacting phenomena in the circum-terrestrial space, constitutes one of the several manifestations of...
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Improvements to the Empirical Solar Wind Forecast (ESWF) model
The empirical solar wind forecast (ESWF) model in its current version 2.0 runs as a space-safety service in the frame of ESA’s Heliospheric Weather...
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Distributions of Mesoscale Periodic Structures in the Elemental and Ionic Composition of the Solar Wind
Multiple statistical and event studies based on in situ observations have shown that the solar wind contains mesoscale (∼ 100 – 10,000 Mm) periodic...
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Spectra of Fluctuations of Solar Wind Plasma Parameters near a Shock Wave
AbstractThe paper investigates the characteristics of the power spectra of fluctuations in the density of protons and α particles near the front of...
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Interplanetary Scintillation Observations of Solar-Wind Disturbances During Cycles 23 and 24
Interplanetary scintillation (IPS) analysis is an effective technique for remotely sensing solar-wind disturbances, such as stream-interaction...
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Direct observation of turbulent magnetic reconnection in the solar wind
Magnetic reconnection in a current sheet is commonly found in astrophysical plasma environments. If it is often bursty, releasing magnetic free...
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On Correlation of the Interplanetary Scintillation Level and Solar Wind Speed
AbstractThe paper reports the results of observations of the interplanetary scintillation of a compact radio source 3С 48 at the descending phase 24...
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On the Differences in the Ambient Solar Wind Speed Forecasting Caused by Using Synoptic Maps from Different Observatories
We consider the problem of forecasting the solar wind speed using not only well-known magnetic field data sets, such as the Wilcox Solar Observatory ...
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Dynamics and solar wind control of the recovery of strong geomagnetic storms
In this work we have studied about the characteristics and dynamical changes during the recovery time of moderate and strong geomagnetic storms of (
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Identifying kinetic scale magnetic discontinuity structures in turbulent solar wind
The turbulent solar wind magnetic field shows structures that are characterized by sudden, strong changes in the field magnitude and/or direction....
