[HTML][HTML] Parker solar probe: Four years of discoveries at solar cycle minimum

NE Raouafi, L Matteini, J Squire, ST Badman… - Space Science …, 2023 - Springer
Abstract 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 …

Shear-driven transition to isotropically turbulent solar wind outside the Alfvén critical zone

D Ruffolo, WH Matthaeus, R Chhiber… - The Astrophysical …, 2020 - iopscience.iop.org
Shear-driven Transition to Isotropically Turbulent Solar Wind Outside the Alfvén Critical Zone -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of …

Characteristic scales of magnetic switchback patches near the sun and their possible association with solar supergranulation and granulation

N Fargette, B Lavraud, AP Rouillard… - The Astrophysical …, 2021 - iopscience.iop.org
Abstract Parker Solar Probe (PSP) data recorded within a heliocentric radial distance of 0.3
au have revealed a magnetic field dominated by Alfvénic structures that undergo large local …

[HTML][HTML] Enhanced proton parallel temperature inside patches of switchbacks in the inner heliosphere

LD Woodham, TS Horbury, L Matteini… - Astronomy & …, 2021 - aanda.org
Context. Switchbacks are discrete angular deflections in the solar wind magnetic field that
have been observed throughout the heliosphere. Recent observations by Parker Solar …

Coronal hole detection and open magnetic flux

JA Linker, SG Heinemann, M Temmer… - The Astrophysical …, 2021 - iopscience.iop.org
Many scientists use coronal hole (CH) detections to infer open magnetic flux. Detection
techniques differ in the areas that they assign as open, and may obtain different values for …

[HTML][HTML] Stirring the base of the solar wind: On heat transfer and vortex formation

AJ Finley, AS Brun, M Carlsson, M Szydlarski… - Astronomy & …, 2022 - aanda.org
Context. Current models of the solar wind must approximate (or ignore) the small-scale
dynamics within the solar atmosphere; however, these are likely important in shaping the …

[HTML][HTML] Measurement of the open magnetic flux in the inner heliosphere down to 0.13 AU

ST Badman, SD Bale, AP Rouillard, TA Bowen… - Astronomy & …, 2021 - aanda.org
Context. Robustly interpreting sets of in situ spacecraft data of the heliospheric magnetic
field (HMF) for the purpose of probing the total unsigned magnetic flux in the heliosphere is …

Hydrogen isotopic composition of hydrous minerals in asteroid Ryugu

L Piani, K Nagashima, N Kawasaki… - The Astrophysical …, 2023 - iopscience.iop.org
Rock fragments of the Cb-type asteroid Ryugu returned to Earth by the JAXA Hayabusa2
mission share mineralogical, chemical, and isotopic properties with the Ivuna-type (CI) …

Multiscale solar wind turbulence properties inside and near switchbacks measured by the parker solar probe

MM Martinović, KG Klein, J Huang… - The Astrophysical …, 2021 - iopscience.iop.org
Abstract The Parker Solar Probe (PSP) routinely observes magnetic field deflections in the
solar wind at distances less than 0.3 au from the Sun. These deflections are related to …

[HTML][HTML] Estimating the Open Solar Flux from In-Situ Measurements

AM Frost, M Owens, A Macneil, M Lockwood - Solar Physics, 2022 - Springer
A fraction of the magnetic flux threading the solar photosphere extends to sufficient
heliocentric distances that it is dragged out by the solar wind. Understanding this open solar …