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Mavromichalaki, H.; Vassilaki, A.; Tsagouri, I.

doi:10.1023/a:1005294103370

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Solar Wind Modeling1

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2001

2023

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Cited by 6 publications

(1 citation statement)

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“…The topology of magnetic clouds was modeled by Hidalgo et al (2000). The sector structures of the interplanetary magnetic field associated with fast plasma streams were modeled by Mavromichalaki, Vassilaki, & Tsagouri (1999). The shock compression at corotating interaction regions was simulated by Lee (2000).…”

Section: Solar Wind Modelingmentioning

confidence: 99%

Astrophysics in 2000

Trimble

Aschwanden

2001

PUBL ASTRON SOC PAC

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It was a year in which some topics selected themselves as important through the sheer numbers of papers published. These include the connection(s) between galaxies with active central engines and galaxies with starbursts, the transition from asymptotic giant branch stars to white dwarfs, gamma-ray bursters, solar data from three major satellite missions, and the cosmological parameters, including dark matter and very large scale structure. Several sections are oriented around processes-accretion, collimation, mergers, and disruptions-shared by a number of kinds of stars and galaxies. And, of course, there are the usual frivolities of errors, omissions, exceptions, and inventories.

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Section: Solar Wind Modelingmentioning

confidence: 99%