Energy Spectra, Composition, and Other Properties of Ground-Level Events During Solar Cycle 23

By R. Mewaldt, M. Looper, C. Cohen, D. Haggerty, A. Labrador, R. Leske, G. Mason, J. Mazur, T. T. Rosenvinge. 2012

172 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

GLOBAL ENERGETICS OF THIRTY-EIGHT LARGE SOLAR ERUPTIVE EVENTS (2012, background): “Examples of energy spectra and both functional forms are given in Mewaldt et al. (2005, 2012) and Cohen et al. (2005).”
Integrated Science Investigation of the Sun (ISIS): Design of the Energetic Particle Investigation (2016, background): “What factors determine the maximum energies in SEP events and why are only a small fraction of CMEs associated with the so-called Ground Level Events (GLEs) (Mewaldt et al. 2012a)?”
The Solar Probe Plus Mission: Humanity’s First Visit to Our Star (2016, background): “SPP will measure CME shocks where particle acceleration to high energies (protons to 10 GeV, electrons to a few tens of MeV) is thought to maximize (R < 20 RS ; Kahler 1994; Mewaldt et al. 2012).”
The Two Sources of Solar Energetic Particles (2012, background): “(6) Shock spectra have a high-energy break downward or knee (Ellison and Ramaty 1985; Lee 2005); spectral breaks have been measured recently in 16 GLEs by Mewaldt et al. (2012).”