It is argued here that the inner heliosphere is filled with a network of entangled magnetic flux
tubes and that the flux tubes are fossil structures that originate at the solar surface. 65,860 …

In this paper we present an assessment of the status of models of the global solar wind in
the inner heliosphere. We limit our discussion to the class of models designed to provide …

A three‐parameter algebraic scheme is developed to categorize the solar wind at 1 AU into
four plasma types: coronal‐hole‐origin plasma, streamer‐belt‐origin plasma, sector …

Multiple coronal and heliospheric models have been recently upgraded at the Community
Coordinated Modeling Center (CCMC), including the Wang‐Sheeley‐Arge (WSA)‐Enlil …

Space weather effects on technological systems originate with energy carried from the Sun
to the terrestrial environment by the solar wind. In this study, we present results of modeling …

High‐speed solar wind streams emanating from coronal holes are frequently im**ing on
the Earth's magnetosphere causing recurrent, medium‐level geomagnetic storm activity …

Emanating from the base of the Sun's corona, the solar wind fills the interplanetary medium
with a magnetized stream of charged particles whose interaction with the Earth's …

We present here a time‐dependent three‐dimensional magnetohydrodynamic (MHD) solar
wind simulation from the solar surface to the Earth's orbit driven by time‐varying line‐of …

Context. Parker Solar Probe (PSP) is providing an unprecedented view of the Sun's corona
as it progressively dips closer into the solar atmosphere with each solar encounter. Each set …

Geomagnetic activity has long been known to exhibit approximately 27 day periodicity,
resulting from solar wind structures repeating each solar rotation. Thus a very simple near …