activity
20112023
most citedParker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum

158 citations · 355 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2023★ 158 cited

Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum

N. E. Raouafi, L. Matteini, J. Squire +54

Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to determine the…

physics.space-ph2019★ 45 cited

Plasma pressures in the heliosheath from Cassini ENA and Voyager 2 measurements: Validation by the Voyager 2 heliopause crossing

K. Dialynas, S. M. Krimigis, R. B. Decker +1

We report "ground truth", 28-3500 keV in-situ ion and 5.2-55 keV remotely sensed ENA measurements from Voyager 2/Low Energy Charged Particle (LECP) detector and Cassini/Ion and Neu…

math-ph2018

ϕ^4 Solitary Waves in a Parabolic Potential: Existence, Stability, and Collisional Dynamics

R. M. Ross, P. G. Kevrekidis, D. K. Campbell +2

We explore a ϕ^4 model with an added external parabolic potential term. This term dramatically alters the spectral properties of the system. We identify single and multiple kink so…

nlin.PS2017★ 50 cited

Kink Dynamics in a Parametric System: A Model With Controllably Many Internal Modes

A. Demirkaya, R. Decker, P. G. Kevrekidis +2

We explore a variant of the model originally proposed in Phys.\ Rev.\ D {\bf 12}, 1606 (1975) as a prototypical, so-called, "bag" model in which domain walls play the role of…

physics.space-ph2015★ 10 cited

Energetic Particle Pressure at Interplanetary Shocks: STEREO-A Observations

D. Lario, R. B. Decker, E. C. Roelof +1

We study periods of elevated energetic particle intensities observed by STEREO-A when the partial pressure exerted by energetic (83 keV) protons () is larger than the…

astro-ph.SR2011★ 92 cited

Is the magnetic field in the heliosheath laminar or a turbulent bath of bubbles?

M. Opher, J. F. Drake, M. Swisdak +4

All the current global models of the heliosphere are based on the assumption that the magnetic field in the heliosheath, in the region close to the heliopause is laminar. We argue…