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 …
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 …
Context. Switchbacks are discrete angular deflections in the solar wind magnetic field that have been observed throughout the heliosphere. Recent observations by Parker Solar …
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 …
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 …
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 …
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) …
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 …
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 …