collaborators

8 papers

astro-ph.HE2026

Solar Cycle Variation of Sustained Gamma Ray Emission from the Sun

Nat Gopalswamy, Pertti Mäkelä, Seiji Yashiro +3

We investigated the occurrence rate of the sustained gamma ray emission (SGRE) events from the Sun using data obtained by Fermi Large Area Telescope (LAT) since its launch in 2008.…

astro-ph.SR2026

Unusual Circumstances of the 2024 June 8 GLE

Nat Gopalswamy, Pertti Makela, Hong Xie +3

Ground Level Enhancement (GLE) in large solar energetic particle (SEP) events is indicative of protons accelerated to GeV energies. Almost all GLE events are associated with sustai…

astro-ph.SR2025

Multispacecraft Observations of the 2024 September 9 Backside Solar Eruption that Resulted in a Sustained Gamma Ray Emission Event

Nat Gopalswamy, Pertti Mäkelä, Sachiko Akiyama +6

We report on the 2024 September 9 sustained gamma ray emission (SGRE) event observed by the Large Area Telescope (LAT) onboard the Fermi satellite. The event was associated with a…

astro-ph.SR2025

Third Harmonic Structure in an Interplanetary Type II Radio Burst and Other Energetic Phenomena During the 2024 September 14 Solar Eruption

Nat Gopalswamy, Pertti Makela, Hong Xie +2

We report on the observation of first, second, and third harmonic components during an interplanetary (IP) type II solar radio burst observed on 2024 September 14 by the radio inst…

astro-ph.SR2025

The Longest Duration SGRE Event in Solar Cycle 25

Nat Gopalswamy, Pertti Makela, Hong Xie +2

Solar Cycle (SC) 24 was the weakest in the space age, yet it produced many sustained gamma ray emission (SGRE) events from the Sun. Solar cycle (SC) 25, which is a bit stronger tha…

astro-ph.SR2025

Implications of the abundance of halo coronal mass ejections for the strength of solar cycle 25

Nat Gopalswamy, Grzegorz Michalek, Seiji Yashiro +3

We assess the relative strength of solar cycle (SC) 25 with respect to SCs 23 and 24 based on the abundance of halo coronal mass ejections (CMEs). We make use of the halo CME datab…