A new data product from the Helioseismic and Magnetic Imager (HMI) onboard the Solar
Dynamics Observatory (SDO) called Space-weather HMI Active Region Patches (SHARPs) is …

We attempt to forecast M-and X-class solar flares using a machine-learning algorithm,
called support vector machine (SVM), and four years of data from the Solar Dynamics …

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 also …

We present a new data product, called Space-Weather MDI Active Region Patches (SMARPs),
derived from maps of the solar surface magnetic field taken by the Michelson Doppler …

Solar active region (AR) 12192 of 2014 October hosts the largest sunspot group in 24 years.
It is the most prolific flaring site of Cycle 24 so far, but surprisingly produced no coronal …

The goal of the SunPy project is to facilitate and promote the use and development of
community-led, free, and open source data analysis software for solar physics based on the …

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 …

We consider the flare prediction problem that distinguishes flare-imminent active regions that
produce an M-or X-class flare in the succeeding 24 hr, from quiet active regions that do not …

The Atmospheric Imaging Assembly (AIA; Lemen et al., 2012) instrument onboard the NASA
Solar Dynamics Observatory (SDO; Pesnell et al., 2012) spacecraft has observed the …

One of the main science motivations for the ESA PLAnetary Transit and Oscillations (PLATO)
mission is to measure exoplanet transit radii with 3 per cent precision. In addition to flares …