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Physical models for solar cycle predictions
The dynamic activity of stars such as the Sun influences (exo) planetary space environments
through modulation of stellar radiation, plasma wind, particle and magnetic fluxes. Energetic …
through modulation of stellar radiation, plasma wind, particle and magnetic fluxes. Energetic …
Mean field models of flux transport dynamo and meridional circulation in the Sun and stars
The most widely accepted model of the solar cycle is the flux transport dynamo model. This
model evolved out of the traditional α Ω dynamo model which was first developed at a time …
model evolved out of the traditional α Ω dynamo model which was first developed at a time …
Predicting the corona for the 21 August 2017 total solar eclipse
The total solar eclipse that occurred on 21 August 2017 across the United States provided
an opportunity to test a magnetohydrodynamic model of the solar corona driven by …
an opportunity to test a magnetohydrodynamic model of the solar corona driven by …
Causality in heliophysics: Magnetic fields as a bridge between the Sun's interior and the Earth's space environment
Our host star, the Sun, is a middle-aged main sequence G type star whose activity varies.
These variations are primarily governed by solar magnetic fields which are produced in the …
These variations are primarily governed by solar magnetic fields which are produced in the …
Impact of anomalous active regions on the large-scale magnetic field of the sun
One of the major sources of perturbation in the solar cycle amplitude is believed to be the
emergence of anomalous active regions that do not obey Hale's polarity law and Joy's law of …
emergence of anomalous active regions that do not obey Hale's polarity law and Joy's law of …
Solar coronal magnetic field extrapolation from synchronic data with AI-generated farside
Solar magnetic fields play a key role in understanding the nature of the coronal phenomena.
Global coronal magnetic fields are usually extrapolated from photospheric fields, for which …
Global coronal magnetic fields are usually extrapolated from photospheric fields, for which …
A 3D kinematic Babcock Leighton solar dynamo model sustained by dynamic magnetic buoyancy and flux transport processes
Context. Magnetohydrodynamic interactions between plasma flows and magnetic fields is
fundamental to the origin and sustenance of the 11-year sunspot cycle. These processes are …
fundamental to the origin and sustenance of the 11-year sunspot cycle. These processes are …
Long-term forcing of the Sun's coronal field, open flux, and cosmic ray modulation potential during grand minima, maxima, and regular activity phases by the solar …
Magnetic fields generated in the Sun's interior by the dynamo mechanism drive solar activity
over a range of time-scales. Direct sunspot observations exist for a few centuries; …
over a range of time-scales. Direct sunspot observations exist for a few centuries; …
Images and spectra of the 2017 total solar eclipse corona from our Oregon site
JM Pasachoff, C Lockwood, E Meadors… - Frontiers in Astronomy …, 2018 - frontiersin.org
We report on early results from a suite of instruments for imaging and spectra we deployed
to Salem, Oregon, for 2 min of totality at the August 21, 2017, total solar eclipse. Our …
to Salem, Oregon, for 2 min of totality at the August 21, 2017, total solar eclipse. Our …
Polar flux imbalance at the sunspot cycle minimum governs hemispheric asymmetry in the following cycle
Aims. Hemispheric irregularities of solar magnetic activity is a well-observed phenomenon,
the origin of which has been studied through numerical simulations and data analysis …
the origin of which has been studied through numerical simulations and data analysis …