PSP Bibliography


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Found 4 entries in the Bibliography.

Showing entries from 1 through 4


Identification of Active Magnetic Reconnection Using Magnetic Flux Transport in Plasma Turbulence

Magnetic reconnection has been suggested to play an important role in the dynamics and energetics of plasma turbulence by spacecraft observations, simulations, and theory over the past two decades, and recently, by magnetosheath observations of MMS. A new method based on magnetic flux transport (MFT) has been developed to identify reconnection activity in turbulent plasmas. This method is applied to a gyrokinetic simulation of two-dimensional (2D) plasma turbulence. Results on the identification of three active reconnection ...

Li, Tak; Liu, Yi-Hsin; Qi, Yi;

Published by: The Astrophysical Journal      Published on: 03/2021

YEAR: 2021     DOI: 10.3847/2041-8213/abea0b

Solar magnetic reconnection; Space plasmas; interplanetary turbulence; 1504; 1544; 830


Evolution of a steamer-blowout CME as observed by imagers on Parker Solar Probe and the Solar Terrestrial Relations Observatory

Context. On 26-27 January 2020, the Wide-field Imager for Solar Probe on Parker Solar Probe (PSP) observed a coronal mass ejection (CME) from a distance of approximately 30 R$_\ensuremath\odot$ as it passed through the instrument s 95\textdegree field-of- view, providing an unprecedented view of the flux rope morphology of the CME s internal structure. The same CME was seen by Solar Terrestrial Relations Observatory-Ahead (STEREO-A), beginning on 25 January. \ Aims: Our goal is to understand the origin and determine the traj ...

Liewer, P.; Qiu, J.; Vourlidas, A.; Hall, J.; Penteado, P.;

Published by: Astronomy and Astrophysics      Published on: jun

YEAR: 2020     DOI: "10.1051/0004-6361/202039641"

Parker Data Used; parker solar probe; Solar Probe Plus

Trajectory Determination for Coronal Ejecta Observed by WISPR/Parker Solar Probe

TheWide-field Imager for Solar Probe(WISPR) onboard theParker Solar Probe(PSP), observing in white light, has a fixed angular field of view, extending from 13.5(circle)to 108(circle)from the Sun and approximately 50(circle)in the transverse direction. Because of the highly elliptical orbit of PSP, the physical extent of the imaged coronal region varies directly as the distance from the Sun, requiring new techniques for analysis of the motions of observed density features. Here, we present a technique for determining the 3D t ...

Liewer, P.; Qiu, J.; Penteado, P.; Hall, J.; Vourlidas, A.; Howard, R.;

Published by: SOLAR PHYSICS      Published on: 10/2020

YEAR: 2020     DOI: 10.1007/s11207-020-01715-y

Parker Data Used


Simulating White Light Images of Coronal Structures for WISPR/Parker Solar Probe: Effects of the Near-Sun Elliptical Orbit

The three-to-five-month elliptical orbit of Parker Solar Probe (PSP), approaching within 10 solar radii of the Sun, will allow the Wide-field Imager for Solar Probe (WISPR) to view the corona with unprecedented spatial resolution from multiple viewpoints. WISPR has a wide fixed angular field of view, extending from 13.5 degrees to 108 degrees from the Sun and approximately 50 degrees in the transverse direction, but the physical extent of the imaged coronal region varies directly with the distance of the spacecraft from the ...

Liewer, P.; Vourlidas, A.; Thernisien, A.; Qiu, J.; Penteado, P.; Nistico, G.; Howard, R.; Bothmer, V.;

Published by: SOLAR PHYSICS      Published on: 07/2019

YEAR: 2019     DOI: 10.1007/s11207-019-1489-4

Parker Data Used