Turbulence Heating ObserveR - satellite mission proposal
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F16%3A10334407" target="_blank" >RIV/00216208:11320/16:10334407 - isvavai.cz</a>
Alternative codes found
RIV/68378289:_____/16:00468397
Result on the web
<a href="http://dx.doi.org/10.1017/S0022377816000775" target="_blank" >http://dx.doi.org/10.1017/S0022377816000775</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S0022377816000775" target="_blank" >10.1017/S0022377816000775</a>
Alternative languages
Result language
angličtina
Original language name
Turbulence Heating ObserveR - satellite mission proposal
Original language description
The Universe is permeated by hot, turbulent, magnetized plasmas. Turbulent plasma is a major constituent of active galactic nuclei, supernova remnants, the intergalactic and interstellar medium, the solar corona, the solar wind and the Earth's magnetosphere, just to mention a few examples. Energy dissipation of turbulent fluctuations plays a key role in plasma heating and energization, yet we still do not understand the underlying physical mechanisms involved. THOR is a mission designed to answer the questions of how turbulent plasma is heated and particles accelerated, how the dissipated energy is partitioned and how dissipation operates in different regimes of turbulence. THOR is a single-spacecraft mission with an orbit tuned to maximize data return from regions in near-Earth space - magnetosheath, shock, foreshock and pristine solar wind - featuring different kinds of turbulence. Here we summarize the THOR proposal submitted on 15 January 2015 to the 'Call for a Medium-size mission opportunity in ESAs Science Programme for a launch in 2025 (M4)'. THOR has been selected by European Space Agency (ESA) for the study phase.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BL - Plasma physics and discharge through gases
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GA16-04956S" target="_blank" >GA16-04956S: Solar wind as a natural laboratory: structure, turbulence, and shocks.</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Journal of Plasma Physics
ISSN
0022-3778
e-ISSN
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Volume of the periodical
82
Issue of the periodical within the volume
5
Country of publishing house
GB - UNITED KINGDOM
Number of pages
16
Pages from-to
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UT code for WoS article
000390383400011
EID of the result in the Scopus database
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