Computational analysis has become ubiquitous within the heliophysics community.
However, community standards for peer review of codes and analysis have lagged behind …

We compare magnetic field measurements taken by the FIELDS instrument on board Parker
Solar Probe (PSP) during its first solar encounter to predictions obtained by potential field …

Coronal mass ejections (CMEs) are the primary sources of intense disturbances at Earth,
where their geoeffectiveness is largely determined by their dynamic pressure and internal …

We introduce and make openly accessible a comprehensive, multivariate time series
(MVTS) dataset extracted from solar photospheric vector magnetograms in Spaceweather …

We present a long short-term memory (LSTM) network for predicting whether an active
region (AR) would produce a ϒ-class flare within the next 24 hr. We consider three ϒ …

In this paper, we present a curated data set from the NASA Solar Dynamics Observatory
(SDO) mission in a format suitable for machine-learning research. Beginning from level 1 …

Of all the activity observed on the Sun, two of the most energetic events are flares and
coronal mass ejections (CMEs). Usually, solar active regions that produce large flares will …

The precise physical process that triggers solar flares is not currently understood. Here we
attempt to capture the signature of this mechanism in solar-image data of various …

One of the grand challenges in heliophysics is the characterization of coronal mass ejection
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …

Context. Solar observatories are providing the world-wide community with a wealth of data,
covering wide time ranges (eg Solar and Heliospheric Observatory, SOHO), multiple …