2022
DOI: 10.48550/arxiv.2211.04887
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Solar wind interaction with a comet: evolution, variability, and implication

Abstract: Once a cometary plasma cloud has been created through ionisation of the cometary neutrals, it presents an obstacle to the solar wind and the magnetic field within it. The acceleration and incorporation of the cometary plasma by the solar wind is a complex process that shapes the cometary plasma environment and is responsible for the creation of boundaries such as a bow shock and diamagnetic cavity boundary. It also gives rise to waves and electric fields which in turn contribute to the acceleration of the plas… Show more

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“…A comprehensive review of previous case studies and the potential use of comet-tail observations as proxy solar wind data are discussed in Jones et al (2018, and references therein). As comets approach the Sun, the increased thermal energy causes their icy composition to sublimate into gas, forming the coma, dust and plasma tails (Götz et al 2022). A comet has two types of tail: a dust tail, which follows the orbit of the comet (appearing curved), and a plasma tail, which points almost radially away from the Sun and is shaped by the solar wind (Voelzke 2005).…”
Section: Introductionmentioning
confidence: 99%
“…A comprehensive review of previous case studies and the potential use of comet-tail observations as proxy solar wind data are discussed in Jones et al (2018, and references therein). As comets approach the Sun, the increased thermal energy causes their icy composition to sublimate into gas, forming the coma, dust and plasma tails (Götz et al 2022). A comet has two types of tail: a dust tail, which follows the orbit of the comet (appearing curved), and a plasma tail, which points almost radially away from the Sun and is shaped by the solar wind (Voelzke 2005).…”
Section: Introductionmentioning
confidence: 99%