activity
20122026
most citedA comparison of Alpha Particle and Proton Beam Differential flow in Collisionally Young Solar Wind

94 citations · 488 across the 9 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

Energy Evolution from the Chromosphere to the Heliosphere in the 2021 October 28 Solar Eruption

Katharine K. Reeves, Daniel B. Seaton, Cynthia Cattell +20

We perform a detailed study of the energetics for a well-observed solar eruption and flare that occurred on 28 October 2021. This event included a GOES class X1.0 flare, a global E…

astro-ph.IM2020★ 58 cited

A Merged Search-Coil and Fluxgate Magnetometer Data Product for Parker Solar Probe FIELDS

Trevor A. Bowen, Stuart D. Bale, John W. Bonnell +12

NASA's Parker Solar Probe (PSP) mission is currently investigating the local plasma environment of the inner-heliosphere (0.25) using both {\em{in-situ}} and remote se…

hep-ex2019★ 9 cited

Contribution of exclusive diffractive processes to the measured azimuthal asymmetries in SIDIS

J. Agarwala, M. G. Alexeev, G. D. Alexeev +203

Hadron leptoproduction in Semi-Inclusive measurements of Deep-Inelastic Scattering (SIDIS) on unpolarised nucleons allows one to get information on the intrinsic transverse momentu…

astro-ph.SR2018★ 94 cited

A comparison of Alpha Particle and Proton Beam Differential flow in Collisionally Young Solar Wind

B. L. Alterman, Justin C. Kasper, Michael L. Stevens +1

In fast wind or when the local Coulomb collision frequency is low, observations show that solar wind minor ions and ion sub-populations flow with different bulk velocities. Measure…

hep-ex2018★ 42 cited

Letter of Intent: A New QCD facility at the M2 beam line of the CERN SPS (COMPASS++/AMBER)

B. Adams, C. A. Aidala, R. Akhunzyanov +263

A New QCD facility at the M2 beam line of the CERN SPS COMPASS++/AMBER

astro-ph.SR2013★ 53 cited

Inner Heliospheric Evolution of a "Stealth" CME Derived From Multi-view Imaging and Multipoint In--situ observations: I. Propagation to 1 AU

T. Nieves-Chinchilla, A. Vourlidas, G. Stenborg +4

Coronal mass ejections (CMEs) are the main driver of Space Weather. Therefore, a precise forecasting of their likely geo-effectiveness relies on an accurate tracking of their morph…