We present the finalized catalog of solar energetic proton events detected by the
Wind/EPACT instrument over the period 1996–2016. Onset times, peak times, peak proton …

We present a new catalogue of solar energetic particle events near the Earth, covering solar
cycle 23 and the majority of solar cycle 24 (1996–2016), based on the 55–80 MeV proton …

To evaluate the solar energetic proton (SEP) forecast model of Laurenza et al., here termed
ESPERTA, we computed the input parameters (soft X-ray (SXR) fluence and∼ 1 MHz radio …

Solar type II radio bursts are the signature of particle acceleration by shock waves in the
solar corona and interplanetary medium. The shocks originate in solar eruptions involving …

We analyze periods with elevated> 40 MeV proton intensities observed near Earth over a
time span of 43 yr (1973–2016) that coincide with the passage of interplanetary (IP) shocks …

Solar cycle (SC) 24 has come to an end by the end of 2019, providing the opportunity to
compare two full cycles to understand the manifestations of SC 24-the smallest cycle in the …

After providing an overview of solar activity as measured by the sunspot number (SSN) and
space weather events during solar cycles (SCs) 21-24, we focus on the weak solar activity in …

We present the first comprehensive catalogue of in situ observed solar energetic electron
(SEE) events that covers solar cycles [SCs] 23 and 24 in the energy range 103–315 keV …

Statistical studies have found a close association between large solar energetic particle
(SEP) events and fast and wide coronal mass ejections (CMEs). However, not all fast and …

The number of coronal mass ejections (CMEs) and their parameters and cycle variations
were investigated and compared to the photospheric magnetic field evolution in cycles 23 …