Journal ArticleDOI
The Angular Momentum of the Solar Wind
Edmund J. Weber,Leverett Davis +1 more
Reads0
Chats0
TLDR
Steady state model of solar wind flow in equatorial plane solved for radial and azimuthal motions, taking into account pressure gradient, magnetic field and gravitational effects as discussed by the authors.Abstract:
Steady state model of solar wind flow in equatorial plane solved for radial and azimuthal motions, taking into account pressure gradient, magnetic field and gravitational effectsread more
Citations
More filters
Journal ArticleDOI
Current Sheets, Plasmoids and Flux Ropes in the Heliosphere. Part I. 2-D or not 2-D? General and Observational Aspects
Olga Khabarova,Olga Malandraki,Helmi Malova,Roman Kislov,A. Greco,Roberto Bruno,Oreste Pezzi,Sergio Servidio,Gang Li,William H. Matthaeus,J. A. le Roux,N. E. Engelbrecht,F. Pecora,Lev Zelenyi,V. N. Obridko,V. D. Kuznetsov +15 more
TL;DR: A review of the evolution of views on processes related to current sheets, plasmoids, blobs and flux ropes of various scales and origins in the heliosphere can be found in this article.
Journal ArticleDOI
Observational studies of stellar rotation
TL;DR: In this article, rotational properties of non-degenerate stars as observed from the protostellar stage to the end of the main sequence are reviewed, including various observational techniques used to measure stellar rotation.
Journal ArticleDOI
Cosmic rays and the magnetic field in the nearby starburst galaxy NGC253 III. Helical magnetic fields in the nuclear outflow
TL;DR: In this paper, the magnetic field structure in the central part of the nuclear starburst galaxy NGC 253 with spatial resolutions between 40 and 150 pc was studied to detect any filamentary emission associated with the nuclear outflow.
Journal ArticleDOI
The Role of Alfvén Wave Dynamics on the Large-scale Properties of the Solar Wind: Comparing an MHD Simulation with Parker Solar Probe E1 Data
Victor Réville,Victor Réville,Marco Velli,Olga Panasenco,Anna Tenerani,Chen Shi,Samuel T. Badman,Stuart D. Bale,Justin C. Kasper,Justin C. Kasper,Michael L. Stevens,Kelly E. Korreck,John W. Bonnell,Anthony W. Case,Thierry Dudok de Wit,Keith Goetz,Peter Harvey,Davin Larson,Roberto Livi,David M. Malaspina,Robert J. MacDowall,Marc Pulupa,Phyllis Whittlesey +22 more
TL;DR: In this article, the authors numerically model the solar corona during this first encounter, solving the MHD equations and accounting for Alfven wave transport and dissipation, finding that the large scale plasma parameters are well reproduced, allowing the computation of the solar wind sources at Probe with confidence.
Journal ArticleDOI
Stellar Winds on the Main-Sequence I: Wind Model
TL;DR: In this paper, the authors developed a method for estimating the properties of stellar winds for low-mass main-sequence stars between masses of 0.4 and 1.1 solar masses at a range of distances from the star.