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The Correspondence Between Sudden Commencements and Geomagnetically Induced Currents: Insights From New Zealand
DOI: 10.1029/2021SW002983 Bibcode: 2022SpWea..2002983S

Forsyth, C.; Rae, I. J.; Smith, A. W. +6 more

Variability of the geomagnetic field induces anomalous Geomagnetically Induced Currents (GICs) in grounded conducting infrastructure. GICs represent a serious space weather hazard but are not often measured directly and the rate of change of the magnetic field is often used as a proxy. We assess the correlation between the rate of change of the ma…

2022 Space Weather
SOHO 7
Time-of-Arrival of Coronal Mass Ejections: A Two-Phase Kinematics Approach Based on Heliospheric Imaging Observations
DOI: 10.1029/2022SW003070 Bibcode: 2022SpWea..2003070P

Vourlidas, Angelos; Paouris, Evangelos

The forecasting of the Time-of-Arrival (ToA) of coronal mass ejections (CMEs) to Earth does not yet meet most Space Weather users' requirements. The main physical reason is our incomplete understanding of CME propagation in the inner heliosphere. Therefore, many ToA forecasting algorithms rely on simple empirical relations to represent the interpl…

2022 Space Weather
SOHO 6
A Machine Learning Approach to Predicting SEP Events Using Properties of Coronal Mass Ejections
DOI: 10.1029/2021SW002797 Bibcode: 2022SpWea..2002797T

Zhang, Ming; Zhao, Lulu; Torres, Jesse +1 more

Solar energetic particles (SEPs) can cause severe damage to astronauts and their equipment, and can disrupt communications on Earth. A lack of thorough understanding the eruption processes of solar activities and the subsequent acceleration and transport processes of energetic particles makes it difficult to forecast the occurrence of an SEP event…

2022 Space Weather
SOHO 5
Automated Detection of coronaL MAss Ejecta origiNs for Space Weather AppliCations (ALMANAC)
DOI: 10.1029/2022SW003253 Bibcode: 2022SpWea..2003253W

Morgan, Huw; Williams, Thomas

Alerts of potentially hazardous coronal mass ejection (CME) are based on the detection of rapid changes in remote observations of the solar atmosphere. This paper presents a method that detects and estimates the central coordinates of CME eruptions in Extreme Ultraviolet data, with the dual aim of providing an early alert, and giving an initial es…

2022 Space Weather
SOHO 5
The Frequency-Domain Characterization of Cosmic Ray Intensity Variations Before Forbush Decreases Associated With Geomagnetic Storms
DOI: 10.1029/2021SW002863 Bibcode: 2022SpWea..2002863Y

He, Fei; Wang, Cong; Zhang, Xiaoxin +2 more

Nonrecurrent geomagnetic storms caused by Coronal Mass Ejection (CME) can induce serious impacts on space- and ground-based equipment. However, these nonrecurrent geomagnetic storms are hard to predict since CMEs are not periodic. Previous studies have shown that the variations of Cosmic Ray Intensity (CRI) before nonrecurrent storms may forebode …

2022 Space Weather
SOHO 3
Improving Multiday Solar Wind Speed Forecasts
DOI: 10.1029/2021SW002868 Bibcode: 2022SpWea..2002868E

Arge, C. N.; Henney, C. J.; Dayeh, M. A. +4 more

We analyze the residual errors for the Wang-Sheeley-Arge (WSA) solar wind speed forecasts as a function of the photospheric magnetic field expansion factor (fp) and the minimum separation angle (d) in the photosphere between the footpoints of open field lines and the nearest coronal hole boundary. We find the map of residual speed error…

2022 Space Weather
Ulysses 2
A Parametric Study of Performance of Two Solar Wind Velocity Forecasting Models During 2006-2011
DOI: 10.1029/2022SW003069 Bibcode: 2022SpWea..2003069K

Srivastava, Nandita; Kumar, Sandeep

There is an increasing need for the development of a robust space weather forecasting framework. State-of-the-art MHD space weather forecasting frameworks are based upon the Potential Field Source Surface (PFSS) and Schatten Current Sheet (SCS) extrapolation models for the magnetic field using synoptic magnetograms. These models create a solar win…

2022 Space Weather
SOHO 2
CME Magnetic Structure and IMF Preconditioning Affecting SEP Transport
DOI: 10.1029/2020SW002654 Bibcode: 2021SpWea..1902654P

Lowrance, Patrick J.; Möstl, Christian; Guo, Jingnan +15 more

Coronal mass ejections (CMEs) and solar energetic particles (SEPs) are two phenomena that can cause severe space weather effects throughout the heliosphere. The evolution of CMEs, especially in terms of their magnetic structure, and the configuration of the interplanetary magnetic field (IMF) that influences the transport of SEPs are currently are…

2021 Space Weather
MEx SOHO 33
A Multi-Purpose Heliophysics L4 Mission
DOI: 10.1029/2021SW002777 Bibcode: 2021SpWea..1902777P

Solanki, S. K.; Arge, C. N.; Henney, C. J. +13 more

The Earth-Sun Lagrangian point 4 is a meta-stable location at 1 AU from the Sun, 60° ahead of Earth's orbit. It has an uninterrupted view of the solar photosphere centered on W60, the Earth's nominal magnetic field connection to the Sun. Such a mission on its own would serve as a solar remote sensing observatory that would oversee the entire solar…

2021 Space Weather
Ulysses 26
Evaluation of CME Arrival Prediction Using Ensemble Modeling Based on Heliospheric Imaging Observations
DOI: 10.1029/2020SW002553 Bibcode: 2021SpWea..1902553A

Dumbović, Mateja; Möstl, Christian; Weiss, Andreas J. +8 more

In this study, we evaluate a coronal mass ejection (CME) arrival prediction tool that utilizes the wide-angle observations made by STEREO's heliospheric imagers (HI). The unsurpassable advantage of these imagers is the possibility to observe the evolution and propagation of a CME from close to the Sun out to 1 AU and beyond. We believe that by exp…

2021 Space Weather
SOHO 23