most citedFirst year of energetic particle measurements in the inner heliosphere with Solar Orbiter's Energetic Particle Detector

69 citations · 473 across the 16 of their papers we have counts for

collaborators

16 papers

physics.space-ph2021★ 30 cited

Multi-spacecraft observations of the structure of the sheath of an interplanetary coronal mass ejection and related energetic ion enhancement

E. K. J. Kilpua, S. W. Good, N. Dresing +18

Sheaths ahead of coronal mass ejections (CMEs) are large heliospheric structures that form with CME expansion and propagation. Turbulent and compressed sheaths contribute to the ac…

astro-ph.SR2021★ 35 cited

Whistler waves observed by Solar Orbiter / RPW between 0.5 AU and 1 AU

M. Kretzschmar, T. Chust, V. Krasnoselskikh +29

The goal of our study is to detect and characterize the electromagnetic waves that can modify the electron distribution functions, with a special attention to whistler waves. We an…

astro-ph.SR2021★ 19 cited

Magnetic reconnection as a mechanism to produce multiple protonpopulations and beams locally in the solar wind

B. Lavraud, R. Kieokaew, N. Fargette +37

Context. Spacecraft observations early revealed frequent multiple proton populations in the solar wind. Decades of research on their origin have focused on processes such as magnet…

astro-ph.SR2021★ 69 cited

First year of energetic particle measurements in the inner heliosphere with Solar Orbiter's Energetic Particle Detector

R. F. Wimmer-Schweingruber, N. Janitzek, D. Pacheco +45

Solar Orbiter strives to unveil how the Sun controls and shapes the heliosphere and fills it with energetic particle radiation. To this end, its Energetic Particle Detector (EPD) h…

physics.space-ph2021★ 4 cited

The solar-wind angular-momentum flux observed during Solar Orbiter's first orbit

Daniel Verscharen, David Stansby, Adam J. Finley +19

Aims: We present the first measurements of the solar-wind angular-momentum (AM) flux recorded by the Solar Orbiter spacecraft. Our aim is the validation of these measurements to su…

physics.space-ph2021

Statistical study of electron density turbulence and ion-cyclotron waves in the inner heliosphere: Solar Orbiter observations

F. Carbone, L. Sorriso-Valvo, Yu. V. Khotyaintsev +27

The recently released spacecraft potential measured by the RPW instrument on-board Solar Orbiter has been used to estimate the solar wind electron density in the inner heliosphere.…

astro-ph.SR2021

Signatures of coronal hole substructure in the solar wind: combined Solar Orbiter remote sensing and in situ measurements

T. S. Horbury, R. Laker, L. Rodriguez +21

Context. The Sun's complex corona is the source of the solar wind and interplanetary magnetic field. While the large scale morphology is well understood, the impact of variations i…

physics.space-ph2021★ 20 cited

Solar wind current sheets and deHoffmann-Teller analysis: First results of DC electric field measurements by Solar Orbiter

K. Steinvall, Yu. V. Khotyaintsev, G. Cozzani +25

Solar Orbiter was launched on February 10, 2020 with the purpose of investigating solar and heliospheric physics using a payload of instruments designed for both remote and in-situ…

physics.space-ph2021★ 28 cited

Kinetic Electrostatic Waves and their Association with Current Structures in the Solar Wind

D. B. Graham, Yu. V. Khotyaintsev, A. Vaivads +21

A variety of kinetic waves develop in the solar wind. The relationship between these waves and larger-scale structures, such as current sheets and ongoing turbulence remain a topic…

physics.space-ph2021★ 29 cited

First-year ion-acoustic wave observations in the solar wind by the RPW/TDS instrument onboard Solar Orbiter

D. Píša, J. Souček, O. Santolík +21

Electric field measurements of the Time Domain Sampler (TDS) receiver, part of the Radio and Plasma Waves (RPW) instrument on board Solar Orbiter, often exhibit very intense broadb…

astro-ph.SR2021★ 27 cited

Solar Orbiter Observations of the Kelvin-Helmholtz Instability in the Solar Wind

R. Kieokaew, B. Lavraud, Y. Yang +17

The Kelvin-Helmholtz instability (KHI) is a nonlinear shear-driven instability that develops at the interface between shear flows in plasmas. KHI has been inferred in various astro…

physics.space-ph2021★ 45 cited

Density Fluctuations Associated with Turbulence and Waves: First Observations by Solar Orbiter

Yu. V. Khotyaintsev, D. B. Graham, A. Vaivads +21

We use the plasma density based on measurements of the probe-to-spacecraft potential in combination with magnetic field measurements by MAG to study fields and density fluctuations…

astro-ph.SR2021★ 41 cited

Multi point analysis of coronal mass ejection flux ropes using combined data from Solar Orbiter, BepiColombo and Wind

A. J. Weiss, C. Moestl, E. E. Davies +15

The recent launch of Solar Orbiter and BepiColombo opened a brief window in which these two spacecraft were positioned in a constellation that allows for the detailed sampling of a…

physics.space-ph2021★ 12 cited

Multi-spacecraft Study of the Solar Wind at Solar Minimum: Dependence on Latitude and Transient Outflows

R. Laker, T. S. Horbury, S. D. Bale +15

The recent launches of Parker Solar Probe (PSP), Solar Orbiter (SO) and BepiColombo, along with several older spacecraft, have provided the opportunity to study the solar wind at m…

physics.space-ph2021★ 52 cited

Turbulence/wave transmission at an ICME-driven shock observed by Solar Orbiter and Wind

L. L. Zhao, G. P. Zank, J. S. He +10

Solar Orbiter observed an interplanetary coronal mass ejection (ICME) event at 0.8 AU on 2020 April 19. The ICME was also observed by Wind at 1 AU on 2020 April 20. An interplaneta…

physics.space-ph2020★ 62 cited

In situ multi-spacecraft and remote imaging observations of the first CME detected by Solar Orbiter and BepiColombo

E. E. Davies, C. Möstl, M. J. Owens +20

On 2020 April 19 a coronal mass ejection (CME) was detected in situ by Solar Orbiter at a heliocentric distance of about 0.8 AU. The CME was later observed in situ on April 20th by…