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Recent Advances on Solar Global Magnetism and Variability
We discuss recent observational, theoretical and numerical progress made in understanding the solar global magnetism and its short and long term variability. We discuss the physical process thought to be at the origin of the solar magnetic field and its 22-yr cycle, namely dynamo action, and the nonlinear interplay between convection, …
NASA SVS | The Solar Polar Magnetic Field
The Solar Polar Magnetic Field. Released Tuesday, February 4, 2020. Visualizations by: Tom Bridgman. Written by: Joy Ng. View full credits. From our single vantage point of Earth, our view of the Sun is never complete. While the far-side of the Sun eventually rotates into view, coverage of the Sun''s polar regions is never satisfactory as ...
Measurements of Photospheric and Chromospheric Magnetic Fields …
The Sun is replete with magnetic fields, with sunspots, pores and plage regions being their most prominent representatives on the solar surface. But even far away from these active regions, magnetic fields are ubiquitous. To a large extent, their importance for the thermodynamics in the solar photosphere is determined by the total magnetic …
The best power banks 2024: top portable chargers for devices
You want a powerful magnetic charger: The Baseus Magnetic Foldable Power Bank is a high-capacity battery built onto a very strong magnet. It holds onto an …
Interplanetary magnetic field
The interplanetary magnetic field at the Earth''s orbit varies with waves and other disturbances in the solar wind, known as " space weather ." The field is a vector, with components in the radial and azimuthal directions as well as a component perpendicular to the ecliptic. The field varies in strength near the Earth from 1 to 37 nT, averaging ...
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Solar active region magnetogram image dataset for studies of …
Abstract. In this dataset we provide a comprehensive collection of line-of-sight (LOS) solar photospheric magnetograms (images quantifying the strength of the photospheric magnetic field) from the ...
The role and contribution of magnetic fields, characterized via their magnetic flux, to the statistical structuring of the solar …
The solar magnetic fields become more and more horizontal as their height increases from the photosphere to the upper atmosphere, forming the so-called canopies 43,44. Temperature and density ...
Switchbacks in the Solar Magnetic Field: Their Evolution, Their Content…
However, as the magnetic field rotates, more of the radial solar wind flow becomes perpendicular to the magnetic field, so it becomes an × /B 2 flow. Because the Poynting flux is × / μ 0, it must also increase along with …
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A model of solar magnetic flux rope eruption initiated primarily by magnetic …
Initial magnetic field (a) and bottom driving flow (b) of the MHD simulation. In panel (a), the field lines are shown by the thick lines, which are coloured by the value of the non-linear force-free factor defined as α = J · B/B 2.The green arrow points out …
Advancing Solar Magnetic Field Extrapolations through Multiheight Magnetic …
where B refers to the magnetic field vector and J to the electric current density. The force-free model builds on the assumption that the plasma density is low and therefore the ratio of plasma pressure and magnetic pressure is small (plasma beta β plasma ≪ 1), which is not satisfied in the solar photosphere but can be validly assumed …
A Large-Scale Dataset of Three-Dimensional Solar Magnetic …
It has been widely accepted that solar magnetic field manipulates all solar activities, especially violent solar bursts in solar corona. Thus, it is extremely important to reconstruct three ...
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A Model of Solar Magnetic Flux Rope Eruption Initiated Primarily by Magnetic …
The ideal MHD instability mechanisms are developed based on magnetic flux rope (MFR), which is a coherent group of magnetic field lines winding about a common axis by over one full turn (Cheng et al., 2017; Liu, 2020). In this framework, two primary models for initiation of eruption have been proposed, including the kink instability (Hood ...
Solar Polar Magnetic Fields: Comparing Full-disk and High-resolution Spectromagnet…
The solar polar magnetic fields dominate the global structure of the corona and heliosphere during most of the magnetic activity cycle (Petrie 2015).They also dominate the interplanetary magnetic field (IMF), defining its strength (Smith & Balogh 2008), and are believed to provide the seed field for subsequent activity cycles …
Solar dynamo
The solar dynamo is a physical process that generates the Sun''s magnetic field is explained with a variant of the dynamo theory.A naturally occurring electric generator in the Sun''s interior produces electric currents and a magnetic field, following the laws of Ampère, Faraday and Ohm, as well as the laws of fluid dynamics, which together form the laws of …
Sun''s magnetic field may originate closer to the solar surface
WASHINGTON, May 22 (Reuters) - The sun''s magnetic field, which causes solar storms like the one that hit Earth this month and produced beautiful auroras, may originate at shallower depths in the ...
(PDF) Switchbacks in the Solar Magnetic Field: Their Evolution, …
Switchbacks in the Solar Magnetic Field: Their Evolution, Their Content, and Their Effects on the Plasma February 2020 The Astrophysical Journal Supplement Series 246(2):68 DOI:10.3847/1538-4365 ...
Generating Photospheric Vector Magnetograms of Solar Active Regions for SOHO/MDI Using SDO/HMI and BBSO Data with Deep Learning
Solar activity is often caused by the evolution of solar magnetic fields. Magnetic field parameters derived from photospheric vector magnetograms of solar active regions (ARs) have been used to analyze and forecast eruptive events, such as solar flares and coronal mass ejections. Unfortunately, the most recent Solar Cycle 24 was relatively …
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Mapping solar magnetic fields from the photosphere to the base …
Moreover, from the visible photospheric surface to the chromosphere-corona transition region (TR), the plasma density decreases exponentially by several orders of magnitude, more rapidly than the magnetic field strength. As a result, the β = 1 corrugated surface, where the ratio of gas to magnetic pressure is unity, lies inside the ...
BLAVOR [Upgraded Magnetic Solar Power Bank, PD 18W QC3.0 …
[Magnetic Wireless Solar Power Bank]: Just attach your phone to the magnetic solar charger and press the power button for efficient wireless charging. The …
Large scale coherent magnetohydrodynamic oscillations in a …
Since magnetic fields dynamically couple different layers of the solar atmosphere, MHD waves are thought to play a major role in heating the outer regions of the atmosphere to million-degree ...
Solar Magnetic Fields: Polarized Radiation Diagnostics
History of Solar Magnetic Fields Since George Ellery Hale Article 07 September 2015 Quiet Sun magnetic fields: an observational view Article Open access 18 February 2019 Radiative Diagnostics in the Article Open access collision ...
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(PDF) Small-Scale Solar Magnetic Fields
Small-Scale Solar Magnetic Fields.pdf Available via license: CC BY-NC 2.0 Content may be subject to copyright. arXiv:0812.4465v1 [astro-ph] 24 Dec 2008 Space Sci Rev DOI 10.1007/s11214-008-9 473-6
The magnetic field in the solar atmosphere | The …
This publication provides an overview of magnetic fields in the solar atmosphere with the focus lying on the corona. The solar magnetic field couples the solar interior with the visible surface of the …
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Magnetics Applications for Solar Power Conversion
Solar energy has been widely deployed to realize carbon-neutralizing benefits. Along with the demand for efficiency of power conversion systems, magnetic component selection for photovoltaic solutions becomes more challenging for design engineers. This article features key principles of power conversion and magnetics …
History of Solar Magnetic Fields Since George Ellery Hale
2 The Enigmatic General Magnetic Field of the Sun. Soon after his discovery of magnetic fields in sunspots Hale wanted to explore the non-spot "background field", the so-called "general" magnetic field of the Sun, which he believed to be a global dipole based on the appearance of the solar corona at eclipses.
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Solar magnetogram
In solar observation, a magnetogram is a pictorial representation of the spatial variations in strength of the solar magnetic field . Solar magnetograms are produced by solar magnetographs. Some magnetographs only measure the absolute value of the magnetic field strength while others are capable of measuring the 3-dimensional magnetic field.
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SOLAR MAGNETIC FIELDS
This solar magnetic sector structure can be described as a rotating dipole whose magnetic axis makes an angle of approximately 90 with the axis of rotation. Possible similarities between this solar-sector magnetism and the models derived from observations of stellar magnetism are discussed. Key words: solar magnetic fields - interplanetary ...
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