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Map** the Sun's coronal magnetic field using the Zeeman effect
Regular remote sensing of the magnetic field embedded within the million-degree solar
corona is severely lacking. This reality impedes fundamental investigations of the nature of …
corona is severely lacking. This reality impedes fundamental investigations of the nature of …
Observations of cross scale energy transfer in the inner heliosphere by Parker Solar Probe
The solar wind, a continuous flow of plasma from the sun, not only shapes the near Earth
space environment but also serves as a natural laboratory to study plasma turbulence in …
space environment but also serves as a natural laboratory to study plasma turbulence in …
Solar wind driven from gong magnetograms in the last solar cycle
In a previous study, Huang et al. used the Alfvén Wave Solar atmosphere Model, one of the
widely used solar wind models in the community, driven by ADAPT-GONG magnetograms to …
widely used solar wind models in the community, driven by ADAPT-GONG magnetograms to …
Global sensitivity analysis and uncertainty quantification for background solar wind using the Alfvén wave solar atmosphere model
Modeling the impact of space weather events such as coronal mass ejections (CMEs) is
crucial to protecting critical infrastructure. The Space Weather Modeling Framework is a …
crucial to protecting critical infrastructure. The Space Weather Modeling Framework is a …
The solar minimum eclipse of 2019 july 2. II. The first absolute brightness measurements and MHD model predictions of Fe x, xi, and xiv out to 3.4 R⊙
B Boe, S Habbal, C Downs… - The Astrophysical …, 2022 - iopscience.iop.org
We present the spatially resolved absolute brightness of the Fe x, Fe xi, and Fe xiv visible
coronal emission lines from 1.08 to 3.4 R⊙, observed during the 2019 July 2 total solar …
coronal emission lines from 1.08 to 3.4 R⊙, observed during the 2019 July 2 total solar …
Assessing the performance of the ADAPT and AFT flux transport models using in situ measurements from multiple satellites
Abstract The launches of Parker Solar Probe (Parker) and Solar Orbiter (SolO) are enabling
a new era of solar wind studies that track the solar wind from its origin at the photosphere …
a new era of solar wind studies that track the solar wind from its origin at the photosphere …
Evolution of magnetic field fluctuations and their spectral properties within the heliosphere: Statistical approach
We present the first comprehensive statistical study of the evolution of compressive and
noncompressive magnetic field fluctuations in the inner heliosphere. Based on Parker Solar …
noncompressive magnetic field fluctuations in the inner heliosphere. Based on Parker Solar …
Simulating Compressive Stream Interaction Regions during Parker Solar Probe's First Perihelion Using Stream-aligned Magnetohydrodynamics
We used the stream-aligned magnetohydrodynamics (SA-MHD) model to simulate
Carrington rotation 2210, which contains Parker Solar Probe's (PSP) first perihelion at 36.5 …
Carrington rotation 2210, which contains Parker Solar Probe's (PSP) first perihelion at 36.5 …
An extended and fragmented Alfvén zone in the young solar wind
Motivated by theoretical, numerical, and observational evidence, we explore the possibility
that the critical transition between sub-Alfvénic flow and super-Alfvénic flow in the solar …
that the critical transition between sub-Alfvénic flow and super-Alfvénic flow in the solar …
Charge state calculation for global solar wind modeling
The charge state composition of the solar wind carries information about the electron
temperature, density, and velocity of plasma in the solar corona that cannot always be …
temperature, density, and velocity of plasma in the solar corona that cannot always be …