activity
20172026
most citedMagnetic connectivity of the ecliptic plane within 0.5 AU : PFSS modeling of the first PSP encounter

161 citations · 1.4k across the 37 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

physics.space-ph2020★ 50 cited

Statistical analysis of orientation, shape, and size of solar wind switchbacks

Ronan Laker, Timothy S. Horbury, Stuart D. Bale +9

One of the main discoveries from the first two orbits of Parker Solar Probe (PSP) was the presence of magnetic switchbacks, whose deflections dominated the magnetic field measureme…

astro-ph.SR2020★ 127 cited

Switchbacks as signatures of magnetic flux ropes generated by interchange reconnection in the corona

J. F. Drake, O. Agapitov, M. Swisdak +10

The structure of magnetic flux ropes injected into the solar wind during reconnection in the coronal atmosphere is explored with particle-in-cell simulations and compared with in s…

astro-ph.SR2020★ 17 cited

Periodicities in an active region correlated with Type III radio bursts observed by Parker Solar Probe

Cynthia Cattell, Lindsay Glesener, Benjamin Leiran +5

Context. Periodicities have frequently been reported across many wavelengths in the solar corona. Correlated periods of ~5 minutes, comparable to solar p-modes, are suggestive of c…

astro-ph.SR2020★ 11 cited

Sensitivity of solar wind mass flux to coronal temperature

D. Stansby, L. Berčič, L. Matteini +4

Solar wind models predict that the mass flux carried away from the Sun in the solar wind should be extremely sensitive to the temperature in the corona, where the solar wind is acc…

astro-ph.SR2020★ 41 cited

Measurement of the Open Magnetic Flux in the Inner Heliosphere down to 0.13AU

Samuel T. Badman, Stuart D. Bale, Alexis P. Rouillard +7

(Abridged) Aim: We attempt to determine robust estimates of the heliospheric magnetic flux () using Parker Solar Probe (PSP) data, analyze how susceptible this is to overestim…

astro-ph.SR2020★ 58 cited

Coronal Electron Temperature inferred from the Strahl Electrons in the Inner Heliosphere: Parker Solar Probe and Helios observations

Laura Bercic, Davin Larson, Phyllis Whittlesey +17

The shape of the electron velocity distribution function plays an important role in the dynamics of the solar wind acceleration. Electrons are normally modelled with three componen…