The Properties of the Solar Corona and Its Connection to the Solar Wind.

Cranmer, S. R., & Winebarger, A. R. (2019). The Properties of the Solar Corona and Its Connection to the Solar Wind. Annual Review of Astronomy and Astrophysics, 157-187.

Type

Journal article

Intellectual base

Review or monograph

Year

2019

DOI

10.1146/annurev-astro-091918-104416

Link

https://doi.org/10.1146/annurev-astro-091918-104416

Cited by

1 citation across 1 artifact.

Domain-specific

• Stellar Wind
  • The solar wind is the supersonic expansion of the Sun's hot, magnetized corona; winds of hot massive stars are accelerated mainly by radiation interacting with spectral lines; winds of cool asymptotic-giant-branch stars depend on pulsation, dust formation, and radiation pressure on grains coupled to gas.

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Registry ID ref:651f311fffbb · see in the full table