http://www.cnr.it/ontology/cnr/individuo/prodotto/ID26167
Ultraviolet imaging of a magneto-plasmadynamic thruster (Articolo in rivista)
- Type
- Label
- Ultraviolet imaging of a magneto-plasmadynamic thruster (Articolo in rivista) (literal)
- Anno
- 2004-01-01T00:00:00+01:00 (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
- 10.1063/1.1789588 (literal)
- Alternative label
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- Spizzo G.; P.Franz; G.Gadani; L.Marrelli; P.Martin; F.Paganucci; P.Rossetti (literal)
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- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#altreInformazioni
- PROCEEDINGS OF THE 15TH TOPICAL CONFERENCE ON HIGH-TEMPERATURE PLASMA DIAGNOSTICS / OPTICAL SYSTEMS, IR TO X-RAY (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
- http://rsi.aip.org/resource/1/rsinak/v75/i10/p4149_s1?isAuthorized=no (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
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- ISI Web of Science (WOS) (literal)
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- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- Spizzo; Franz; GadaniConsorzio RFX, Euratom-ENEA Association, Corso Stati Uniti, 4-35127 Padova, Italy and Dipartimento di Fisica, Universitá di Padova, Via Marzolo, 8-35131 Padova, Italy
2Consorzio RFX, Euratom-ENEA Association, Corso Stati Uniti, 4-35127 Padova, Italy
3Centrospazio-ALTA, Via A. Gherardesca, 5-56121 Ospedaletto, Pisa, Italy (literal)
- Titolo
- Ultraviolet imaging of a magneto-plasmadynamic thruster (literal)
- Abstract
- In this paper the results of a project concerning the ultraviolet (UV) imaging of a plasma for space applications, produced in a magneto-plasmadynamic (MPD) thruster, are presented. MPD are a class of high-power electric space propulsion devices that accelerate a plasma to high velocities (>10 km/s), by exploiting the Lorentz force. This force arises from the interaction between the discharge electrical current and a self induced and externally applied magnetic field. The imaging system has been realized by inserting three arrays of UV-enhanced photodiodes directly into the plastic structure of the anode. The amplifiers are miniaturized and built into the detector. This advanced diagnostic design allows for a detailed tomographic reconstruction of the emissivity spatial structure, both in the axial direction z (corresponding to a wave number n) and azimuthal direction (wave number m) with high time resolution. A magneto-hydrodynamic instability, with mode numbers m=1 and n=1 has been observed, which might affect the performances of the thruster. (literal)
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