most citedComparing extrapolations of the coronal magnetic field structure at 2.5 solar radii with multi-viewpoint coronagraphic observations

10 citations · 11 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2024

Electron Cyclotron Maser Emission and the Brightest Solar Radio Bursts

Stephen M. White, Masumi Shimojo, Kazumasa Iwai +5

This paper investigates the incidence of coherent emission in solar radio bursts, using a revised catalog of 3800 solar radio bursts observed by the Nobeyama Radio Polarimeters fro…

astro-ph.SR2020

Evolution of a Streamer-Blowout CME as Observed by Imagers on Parker Solar Probe and the Solar Terrestrial Relations Observatory

P. C. Liewer, J. Qiu, A. Vourlidas +2

Context: On 26-27 January 2020, the wide-field imager WISPR on Parker Solar Probe (PSP) observed a coronal mass ejection (CME) from a distance of approximately 30 solar radii as it…

astro-ph.SR2020

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

P. C. Liewer, J. Qiu, P. Penteado +3

The {\it Wide-field Imager for Solar Probe} (WISPR) on {\it Parker Solar Probe} (PSP), observing in white light, has a fixed angular field of view, extending from 13.5 to…

astro-ph.SR20201 cited

The Science Case for the Perspective: A Polar/Global View for Studying the Evolution & Propagation of the Solar Wind and Solar Transients

A. Vourlidas, S. Gibson, D. Hassler +4

To make progress on the open questions on CME/CIR propagation, their interactions and the role and nature of the ambient solar wind, we need spatially resolved coverage of the inne…

astro-ph.SR201910 cited

Comparing extrapolations of the coronal magnetic field structure at 2.5 solar radii with multi-viewpoint coronagraphic observations

C. Sasso, R. F. Pinto, V. Andretta +19

The magnetic field shapes the structure of the solar corona but we still know little about the interrelationships between the coronal magnetic field configurations and the resultin…