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[HTML][HTML] Review of solar energetic particle prediction models
Abstract Solar Energetic Particle (SEP) events are interesting from a scientific perspective as
they are the product of a broad set of physical processes from the corona out through the …
they are the product of a broad set of physical processes from the corona out through the …
Origins of the ambient solar wind: implications for space weather
The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …
Alfvén wave solar model (AWSoM): coronal heating
We present a new version of the Alfvén wave solar model, a global model from the upper
chromosphere to the corona and the heliosphere. The coronal heating and solar wind …
chromosphere to the corona and the heliosphere. The coronal heating and solar wind …
Magnetohydrodynamic waves and coronal heating: Unifying empirical and MHD turbulence models
We present a new global model of the solar corona, including the low corona, the transition
region, and the top of the chromosphere. The realistic three-dimensional magnetic field is …
region, and the top of the chromosphere. The realistic three-dimensional magnetic field is …
The open flux problem
The heliospheric magnetic field is of pivotal importance in solar and space physics. The field
is rooted in the Sun's photosphere, where it has been observed for many years. Global maps …
is rooted in the Sun's photosphere, where it has been observed for many years. Global maps …
Direct observations of a complex coronal web driving highly structured slow solar wind
The solar wind consists of continuous streams of charged particles that escape into the
heliosphere from the Sun, and is split into fast and slow components, with the fast wind …
heliosphere from the Sun, and is split into fast and slow components, with the fast wind …
Corotating interaction regions during the recent solar minimum: The power and limitations of global MHD modeling
The declining phase of solar activity cycle 23 has provided an unprecedented opportunity to
study the evolution and properties of corotating interaction regions (CIRs) during unique and …
study the evolution and properties of corotating interaction regions (CIRs) during unique and …
Predictability of the solar cycle over one cycle
The prediction of the strength of future solar cycles is of interest because of its practical
significance for space weather and as a test of our theoretical understanding of the solar …
significance for space weather and as a test of our theoretical understanding of the solar …
On polar magnetic field reversal and surface flux transport during solar cycle 24
As each solar cycle progresses, remnant magnetic flux from active regions (ARs) migrates
poleward to cancel the old-cycle polar field. We describe this polarity reversal process …
poleward to cancel the old-cycle polar field. We describe this polarity reversal process …
Solar magnetic field reversals and the role of dynamo families
The variable magnetic field of the solar photosphere exhibits periodic reversals as a result of
dynamo activity occurring within the solar interior. We decompose the surface field as …
dynamo activity occurring within the solar interior. We decompose the surface field as …