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Space weather: the solar perspective: An update to Schwenn (2006)
DOI: 10.1007/s41116-021-00030-3 Bibcode: 2021LRSP...18....4T

Temmer, Manuela

The Sun, as an active star, is the driver of energetic phenomena that structure interplanetary space and affect planetary atmospheres. The effects of Space Weather on Earth and the solar system is of increasing importance as human spaceflight is preparing for lunar and Mars missions. This review is focusing on the solar perspective of the Space We…

2021 Living Reviews in Solar Physics
PROBA-2 SOHO Ulysses 152
The evolution of the solar wind
DOI: 10.1007/s41116-021-00029-w Bibcode: 2021LRSP...18....3V

Vidotto, Aline A.

How has the solar wind evolved to reach what it is today? In this review, I discuss the long-term evolution of the solar wind, including the evolution of observed properties that are intimately linked to the solar wind: rotation, magnetism and activity. Given that we cannot access data from the solar wind 4 billion years ago, this review relies on…

2021 Living Reviews in Solar Physics
Ulysses 79
Solar structure and evolution
DOI: 10.1007/s41116-020-00028-3 Bibcode: 2021LRSP...18....2C

Christensen-Dalsgaard, Jørgen

The Sun provides a critical benchmark for the general study of stellar structure and evolution. Also, knowledge about the internal properties of the Sun is important for the understanding of solar atmospheric phenomena, including the solar magnetic cycle. Here I provide a brief overview of the theory of stellar structure and evolution, including t…

2021 Living Reviews in Solar Physics
SOHO Ulysses 62
Solar wind stream interaction regions throughout the heliosphere
DOI: 10.1007/s41116-017-0011-z Bibcode: 2018LRSP...15....1R

Richardson, Ian G.

This paper focuses on the interactions between the fast solar wind from coronal holes and the intervening slower solar wind, leading to the creation of stream interaction regions that corotate with the Sun and may persist for many solar rotations. Stream interaction regions have been observed near 1 AU, in the inner heliosphere (at

2018 Living Reviews in Solar Physics
Ulysses 242
The Solar Wind as a Turbulence Laboratory
DOI: 10.12942/lrsp-2013-2 Bibcode: 2013LRSP...10....2B

Bruno, Roberto; Carbone, Vincenzo

In this review we will focus on a topic of fundamental importance for both astrophysics and plasma physics, namely the occurrence of large-amplitude low-frequency fluctuations of the fields that describe the plasma state. This subject will be treated within the context of the expanding solar wind and the most meaningful advances in this research f…

2013 Living Reviews in Solar Physics
Cluster Ulysses 808
The Solar Wind as a Turbulence Laboratory
DOI: 10.12942/lrsp-2005-4 Bibcode: 2005LRSP....2....4B

Bruno, Roberto; Carbone, Vincenzo

In this review we will focus on a topic of fundamental importance for both plasma physics and astrophysics, namely the occurrence of large-amplitude low-frequency fluctuations of the fields that describe the plasma state. This subject will be treated within the context of the expanding solar wind and the most meaningful advances in this research f…

2005 Living Reviews in Solar Physics
Ulysses 476