Turbulence Heating ObserveR – satellite mission proposal

Vaivads, A.; Retinò, A.; Souček, Jan; Khotyaintsev, Y. V.; Valentini, F.; Escoubet, C. P.; Alexandrova, O.; André, M.; Bale, S. D.; Balikhin, M.; Burgess, D.; Camporeale, E.; Caprioli, D.; Chen, C. H. K.; Clacey, E.; Cully, C. M.; Keyser de, J.; Eastwood, J. P.; Fazakerley, A. N.; Eriksson, S.; Goldstein, M. L.; Graham, D. B.; Haaland, S.; Hoshino, M.; Ji, H.; Karimabadi, H.; Kucharek, H.; Lavraud, B.; Marcucci, F.; Matthaeus, W. H.; Moore, T. E.; Nakamura, R.; Narita, Y.; Němeček, Z.; Norgren, C.; Opgenoorth, H.; Palmroth, M.; Perrone, D.; Pinçon, J.-L.; Rathsman, P.; Rothkaehl, H.; Sahraoui, F.; Servidio, S.; Sorriso-Valvo, L.; Vainio, L.; Vörös, Z.; Wimmer-Schweingruber, R. F.

doi:https://dx.doi.org/10.1017/S0022377816000775

Počet záznamů: 1

Turbulence Heating ObserveR – satellite mission proposal

1.

SYSNO ASEP	0468397
Druh ASEP	J - Článek v odborném periodiku
Zařazení RIV	J - Článek v odborném periodiku
Poddruh J	Článek ve WOS
Název	Turbulence Heating ObserveR – satellite mission proposal
Tvůrce(i)	Vaivads, A. (SE) Retinò, A. (FR) Souček, Jan (UFA-U)_{RID, ORCID} Khotyaintsev, Y. V. (SE) Valentini, F. (IT) Escoubet, C. P. (NL) Alexandrova, O. (FR) André, M. (SE) Bale, S. D. (US) Balikhin, M. (GB) Burgess, D. (GB) Camporeale, E. (NL) Caprioli, D. (US) Chen, C. H. K. (GB) Clacey, E. (SE) Cully, C. M. (CN) Keyser de, J. (BE) Eastwood, J. P. (GB) Fazakerley, A. N. (GB) Eriksson, S. (US) Goldstein, M. L. (US) Graham, D. B. (SE) Haaland, S. (DE) Hoshino, M. (JP) Ji, H. (US) Karimabadi, H. (US) Kucharek, H. (US) Lavraud, B. (FR) Marcucci, F. (IT) Matthaeus, W. H. (US) Moore, T. E. (US) Nakamura, R. (AT) Narita, Y. (AT) Němeček, Z. (CZ) Norgren, C. (SE) Opgenoorth, H. (SE) Palmroth, M. (FI) Perrone, D. (ES) Pinçon, J.-L. (FR) Rathsman, P. (SE) Rothkaehl, H. (PL) Sahraoui, F. (FR) Servidio, S. (IT) Sorriso-Valvo, L. (IT) Vainio, L. (FI) Vörös, Z. (AT) Wimmer-Schweingruber, R. F. (DE)
Celkový počet autorů	47
Zdroj.dok.	Journal of Plasma Physics. - : Cambridge University Press - ISSN 0022-3778 Roč. 82, č. 5 (2016), 905820501/1-905820501/16
Poč.str.	16 s.
Jazyk dok.	eng - angličtina
Země vyd.	US - Spojené státy americké
Klíč. slova	plasma heating ; plasma properties ; space plasma physics
Vědní obor RIV	BL - Fyzika plazmatu a výboje v plynech
Obor OECD	Fluids and plasma physics (including surface physics)
Institucionální podpora	UFA-U - RVO:68378289
UT WOS	000390383400011
EID SCOPUS	85011657185
DOI	10.1017/S0022377816000775
Anotace	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.
Pracoviště	Ústav fyziky atmosféry
Kontakt	Kateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
Rok sběru	2017

Počet záznamů: 1