Astrospheres and Solar-like Stellar Winds
Stellar analogs for the solar wind have proven to be frustratingly difficult to detect directly. However, these stellar winds can be studied indirectly by observing the interaction regions carved out by the collisions between these winds and the interstellar medium (ISM). These interaction regions a...
Main Author: | Wood Brian E. |
---|---|
Format: | Article |
Language: | English |
Published: |
Springer
2004-07-01
|
Series: | Living Reviews in Solar Physics |
Subjects: | |
Online Access: | http://www.livingreviews.org/lrsp-2004-2 |
Similar Items
-
The Direction of the Flow of Interstellar Neutral H Based on Photometric Observations from SOHO/SWAN
by: M. Bzowski, et al.
Published: (2023-01-01) -
Evidence of a Thick Heliopause Boundary Layer Resulting from Active Magnetic Reconnection with the Interstellar Medium
by: Drew L. Turner, et al.
Published: (2024-01-01) -
Kinetic Features of Alpha Particles in a Pestchek-like Magnetic Reconnection Event in the Solar Wind Observed by Solar Orbiter
by: Die Duan, et al.
Published: (2023-01-01) -
Observation of the Hall Magnetic Reconnection As Close As 56 Solar Radii from the Sun
by: Rongsheng Wang, et al.
Published: (2023-01-01) -
Modulation of Solar Wind Impact on the Earth’s Magnetosphere during the Solar Cycle
by: Francesco Carbone, et al.
Published: (2022-06-01)