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The Radial Variation of the Solar Wind Turbulence Spectra near the Kinetic Break Scale from Parker Solar Probe Measurements
DOI: 10.3847/1538-4357/aca903 Bibcode: 2023ApJ...942...93L

Bale, S. D.; Kontar, E. P.; Engelbrecht, N. E. +7 more

In this study we examine the radial dependence of the inertial and dissipation range indices, as well as the spectral break separating the inertial and dissipation range in power density spectra of interplanetary magnetic field fluctuations using Parker Solar Probe data from the fifth solar encounter between ~0.1 and ~0.7 au. The derived break wav…

2023 The Astrophysical Journal
Ulysses 19
Modeling a Coronal Mass Ejection from an Extended Filament Channel. II. Interplanetary Propagation to 1 au
DOI: 10.3847/1538-4357/ad0229 Bibcode: 2023ApJ...958...91P

Scolini, Camilla; Lynch, Benjamin J.; Palmerio, Erika +5 more

We present observations and modeling results of the propagation and impact at Earth of a high-latitude, extended filament channel eruption that commenced on 2015 July 9. The coronal mass ejection (CME) that resulted from the filament eruption was associated with a moderate disturbance at Earth. This event could be classified as a so-called "proble…

2023 The Astrophysical Journal
SOHO Ulysses 13
Estimates of Proton and Electron Heating Rates Extended to the Near-Sun Environment
DOI: 10.3847/2041-8213/acf85e Bibcode: 2023ApJ...955L..28B

McComas, D. J.; Bale, S. D.; Cranmer, S. R. +11 more

A central problem of space plasma physics is how protons and electrons are heated in a turbulent, magnetized plasma. The differential heating of charged species due to dissipation of turbulent fluctuations plays a key role in solar wind evolution. Measurements from previous heliophysics missions have provided estimates of proton and electron heati…

2023 The Astrophysical Journal
Ulysses 11
Unfolding Drift Effects for Cosmic Rays over the Period of the Sun's Magnetic Field Reversal
DOI: 10.3847/1538-4357/acc24a Bibcode: 2023ApJ...947...72A

Luo, Xi; Potgieter, M. S.; Aslam, O. P. M. +2 more

A well-established, comprehensive 3D numerical modulation model is applied to simulate galactic protons, electrons, and positrons from 2011 May to 2015 May, including the solar magnetic polarity reversal of Solar Cycle 24. The objective is to evaluate how simulations compare with corresponding Alpha Magnetic Spectrometer observations for 1.0-3.0 G…

2023 The Astrophysical Journal
Ulysses 11
The Polytropic Behavior of Solar Wind Protons as Observed by the Ulysses Spacecraft during Solar Minimum
DOI: 10.3847/1538-4357/acbf33 Bibcode: 2023ApJ...948...22N

Livadiotis, George; Nicolaou, Georgios; McComas, David J.

We analyze proton bulk parameters derived from Ulysses observations and investigate the polytropic behavior of solar wind protons over a wide range of heliocentric distances and latitudes. The large-scale variations of the proton density and temperature over heliocentric distance indicate that plasma protons are governed by subadiabatic processes …

2023 The Astrophysical Journal
Ulysses 9
Formulating Mass-loss Rates for Sun-like Stars: A Hybrid Model Approach
DOI: 10.3847/1538-4357/acfa72 Bibcode: 2023ApJ...957...71S

Toriumi, Shin; Cranmer, Steven R.; Shoda, Munehito

We observe an enhanced stellar wind mass-loss rate from low-mass stars exhibiting higher X-ray flux. This trend, however, does not align with the Sun, where no evident correlation between X-ray flux and mass-loss rate is present. To reconcile these observations, we propose a hybrid model for the stellar wind from solar-type stars, incorporating bo…

2023 The Astrophysical Journal
Ulysses 6
A Three-dimensional Model for the Evolution of Magnetohydrodynamic Turbulence in the Outer Heliosphere
DOI: 10.3847/1538-4357/acd84e Bibcode: 2023ApJ...953..133K

Oughton, Sean; Fichtner, Horst; Kleimann, Jens +1 more

We present a time-dependent, three-dimensional single-fluid model for the transport of magnetohydrodynamic (MHD) turbulence that is self-consistently evolving with a dynamic large-scale solar wind in the outer heliosphere. The emphasis is on the region beyond the termination shock, where the solar wind expands subsonically, as well as sub-Alfvénic…

2023 The Astrophysical Journal
Ulysses 6
Modulation of Cosmic-Ray Antiprotons in the Heliosphere: Simulations for a Solar Cycle
DOI: 10.3847/1538-4357/ace31e Bibcode: 2023ApJ...953..101A

Luo, Xi; Potgieter, M. S.; Aslam, O. P. M. +1 more

The precision measurements of galactic cosmic-ray protons from the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics and the Alpha Magnetic Spectrometer are reproduced using a well-established three-dimensional numerical model for the period 2006 July-2019 November. The resulting modulation parameters are applied to simulate …

2023 The Astrophysical Journal
Ulysses 5
Connection between Polytropic Index and Heating
DOI: 10.3847/1538-4357/acf45d Bibcode: 2023ApJ...956...88L

McComas, D. J.; Livadiotis, G.

The paper derives the one-to-one connecting relationships between plasma heating and its polytropic index, and addresses the consequences through the transport equation of temperature. Thermodynamic polytropic processes are classified in accordance to their polytropic index, the exponent of the power-law relationship of thermal pressure expressed …

2023 The Astrophysical Journal
Ulysses 5
Influence of Intermittency on the Energy Transfer Rate of Solar Wind Turbulence
DOI: 10.3847/2041-8213/ad0a68 Bibcode: 2023ApJ...958L..28W

Wang, Xin; Yuan, Zhigang; Huang, Shiyong +2 more

The intermittency in the solar wind turbulence manifests itself in the anisotropic scaling due to the anisotropic spectral index and the intermittent level based on the extended P model. However, the influence of intermittency on the energy transfer rate remains unclear. Here we apply the partial variance of increments method to identify the inter…

2023 The Astrophysical Journal
Ulysses 3