Marco Marinelli

Marco Marinelli

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Research Focus & Metrics

Academic Career Length

39Years (1988-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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15 June 2017 in Nuclear Fusion
Verified
Journal Article
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XLX. Litaudon
X. Litaudon
SAS. Abduallev
S. Abduallev
MAM. Abhangi
M. Abhangi
PAP. Abreu
P. Abreu
MAM. Afzal
M. Afzal
JCJet Contributors
Jet Contributors

6 May 2005 in Applied Physics Letters
Verified
Journal Article
Closed access
ABA. Balducci
A. Balducci
MMMarco Marinelli
Marco Marinelli
EME. Milani
E. Milani
MMM. E. Morgada
M. E. Morgada
ATA. Tucciarone
A. Tucciarone
MPMario Pillon
Mario Pillon
High-quality single-crystal diamond films, homoepitaxially grown by microwave chemical vapor deposition, have been used to produce diamond-based photodetectors. Such devices were tested over a very wide spectral range, from the extreme ultraviolet (UV) (20 nm) up to the near IR region (2400 nm). An optical parametric oscillator tunable laser was used to investigate the 210–2400 nm spectral range in pulse mode. In this region, the spectral response shows a UV to visible contrast of about 6 orders of magnitude. A time response shorter than 5 ns, i.e., the laser pulse duration, was observed. By integrating the pulse shape, a minor slow component was evidenced, which can be explained in terms of trapping–detrapping effects. Extreme UV gas sources and a toroidal grating vacuum monochromator were used to measure the device response down to 20 nm in continuous mode. In particular, the extreme UV He spectrum was measured and the He II m, 30.4 nmand He I 58.4 nm emission lines were clearly detected. The measured time response of 0.2 s is totally due to the instrumental readout time constants. In both experimental setups an extremely good stability and reproducibility of the device response were obtained, whereas no persistent photoconductivity nor undesirable pumping effects were observed.

30 August 2019 in Nuclear Fusion
Verified
Journal Article
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EJE. Joffrin
E. Joffrin
SAS. Abduallev
S. Abduallev
MAM. Abhangi
M. Abhangi
PAP. Abreu
P. Abreu
VAV. Afanasev
V. Afanasev
IZI. Zychor
I. Zychor
For the past several years, the JET scientific programme (Pamela et al 2007 Fusion Eng. Des. 82 590) has been engaged in a multi-campaign effort, including experiments in D, H and T, leading up to 2020 and the first experiments with 50%/50% D–T mixtures since 1997 and the first ever D–T plasmas with the ITER mix of plasma-facing component materials. For this purpose, a concerted physics and technology programme was launched with a view to prepare the D–T campaign (DTE2). This paper addresses the key elements developed by the JET programme directly contributing to the D–T preparation. This intense preparation includes the review of the physics basis for the D–T operational scenarios, including the fusion power predictions through first principle and integrated modelling, and the impact of isotopes in the operation and physics of D–T plasmas (thermal and particle transport, high confinement mode (H-mode) access, Be and W erosion, fuel recovery, etc). This effort also requires improving several aspects of plasma operation for DTE2, such as real time control schemes, heat load control, disruption avoidance and a mitigation system (including the installation of a new shattered pellet injector), novel ion cyclotron resonance heating schemes (such as the three-ions scheme), new diagnostics (neutron camera and spectrometer, active Alfvèn eigenmode antennas, neutral gauges, radiation hard imaging systems…) and the calibration of the JET neutron diagnostics at 14 MeV for accurate fusion power measurement. The active preparation of JET for the 2020 D–T campaign provides an incomparable source of information and a basis for the future D–T operation of ITER, and it is also foreseen that a large number of key physics issues will be addressed in support of burning plasmas.

2 July 2012 in Medical Physics
Verified
Journal Article
Closed access
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ICI. Ciancaglioni
I. Ciancaglioni
MMMarco Marinelli
Marco Marinelli
EME. Milani
E. Milani
Giuseppe PrestopinoGiuseppe Prestopino
Giuseppe Prestopino
Claudio VeronaClaudio Verona
Claudio Verona
FNF. De Notaristefani
F. De Notaristefani

1 June 1989 in Physical Review B
Verified
Journal Article
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GBG. Balestrino
G. Balestrino
ANA. Nigro
A. Nigro
RVR. Vaglio
R. Vaglio
MMMarco Marinelli
Marco Marinelli
Measurements of the excess conductivity above the superconducting transition for the 110-K phase of the Bi-Sr-Ca-Cu-O compound are reported. The data are very well described in terms of the classic theory of thermodynamic fluctuations in a two-dimensional superconductor. The results are discussed and compared with previous observations on the YBa2 Cu3 O7 compound, where three-dimensional superconductivity was found.

1 January 2010 in Journal of Applied Physics
Verified
Journal Article
Closed access
Salvatore AlmavivaSalvatore Almaviva
Salvatore Almaviva
MMMarco Marinelli
Marco Marinelli
EME. Milani
E. Milani
Giuseppe PrestopinoGiuseppe Prestopino
Giuseppe Prestopino
ATA. Tucciarone
A. Tucciarone
NTN. Tartoni
N. Tartoni
Recently, solid state photovoltaic Schottky diodes, able to detect ionizing radiation, in particular, x-ray and ultraviolet radiation, have been developed at the University of Rome “Tor Vergata.” We report on a physical and electrical properties analysis of the device and a detailed study of its detection capabilities as determined by its electrical properties. The design of the device is based on a metal/nominally intrinsic/p-type diamond layered structure obtained by microwave plasma chemical vapor deposition of homoepitaxial single crystal diamond followed by thermal evaporation of a metallic contact. The device can operate in an unbiased mode by using the built-in potential arising from the electrode-diamond junction. We compare the expected response of the device to photons of various energies calculated through Monte Carlo simulation with experimental data collected in a well controlled experimental setup i.e., monochromatic high flux x-ray beams from 6 to 20 keV, available at the Diamond Light Source synchrotron in Harwell (U.K.).