Electron Kappa Distributions in the Solar Wind: Cause of the Acceleration or Consequence of the Expansion?

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00561919" target="_blank" >RIV/67985815:_____/21:00561919 - isvavai.cz</a>
Alternative codes found
RIV/68378289:_____/21:00561932
Result on the web
<a href="http://dx.doi.org/10.1007/978-3-030-82623-9_3" target="_blank" >http://dx.doi.org/10.1007/978-3-030-82623-9_3</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/978-3-030-82623-9_3" target="_blank" >10.1007/978-3-030-82623-9_3</a>

Result language
angličtina
Original language name
Electron Kappa Distributions in the Solar Wind: Cause of the Acceleration or Consequence of the Expansion?
Original language description
The electron velocity distribution functions in the solar wind, far from the Sun, clearly exhibit a Kappa-like suprathermal tail. Is this characteristic also present in the corona or is it simply the consequence of the solar wind expansion? We elaborate around this question in this short chapter by relying, among others, on the recent electron measurements, as close as 29 solar radii (RSun) from the Sun, by the Parker Solar Probe.
Czech name
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Czech description
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Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2021
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Book/collection name
Kappa Distributions : From Observational Evidences via Controversial Predictions to a Consistent Theory of Nonequilibrium Plasmas
ISBN
978-3-030-82623-9
Number of pages of the result
13
Pages from-to
39-51
Number of pages of the book
330
Publisher name
Springer
Place of publication
Cham
UT code for WoS chapter
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