149 results on '"Mascali David"'
Search Results
2. GEANT4 simulations for γ-ray detector array design for inplasma β-decays studies of nuclear astrophysics interest
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Naselli Eugenia, Santonocito Domenico, Amaducci Simone, Celona Luigi, Galatà Alessio, Mauro Giorgio, Mazzaglia Maria, Mishra Bharat, Pidatella Angelo, Torrisi Giuseppe, and Mascali David
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Physics ,QC1-999 - Abstract
The PANDORA project aims to investigate, by a new experimental approach, the β-decays lifetimes of isotopes of nuclear astrophysics interest as a function of thermodynamic conditions of a laboratory plasma able to mimic some stellar-like conditions. A γ-ray detection system was designed by GEANT4 simulations to tag the in-plasma β-decays via the γ-rays emitted from the excited states of the daughter nuclei. The feasibility of PANDORA, in terms of significance levels, was checked by a “virtual experiment run”, also investigating the sensitivity for discriminating among different theoretical predictions.
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- 2023
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3. Plasma Induced Variation of Electron Capture and Bound-State $\beta$ Decays
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Mishra, Bharat, Pidatella, Angelo, Taioli, Simone, Simonucci, Stefano, and Mascali, David
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Physics - Plasma Physics ,Nuclear Theory ,Physics - Atomic Physics - Abstract
The slow neutron capture ($s$-process) synthesises ~50% of all elements in the universe heavier than iron, whose abundances are determined by the competition between neutron capture and nuclear $\beta$-decay rates. The latter are expected to vary inside hot and dense plasmas such as those found in $s$-process nucleosynthesis sites. Here, we present a new and general theoretical study of the effect of local and non-local thermodynamic equilibrium ((N)LTE) plasmas on $\beta$-decays, using orbital electron capture (EC) decays in $^{7}$Be as a model case. We begin from the model of Takahashi and Yokoi to calculate the lepton phase volume of $^{7}$Be as a function of its ionisation state and excitation level, and consequently, the configuration-dependent EC decay rate. We then calculate the in-plasma ion charge state distribution (CSD) and level population distribution (LPD) for a grid of plasma density and temperatures, using the population kinetics code FLYCHK. By combining the configuration-dependent EC rate with the CSD and LPD, we calculate the in-plasma orbital EC rate in $^{7}$Be. The results show a strong correlation between the half-life and thermodynamic conditions of the plasma, underlining the importance of measuring decay rates in laboratory plasmas and the relevance of high precision atomic configuration models. The model discussed in this work is capable of calculating EC and bound state $\beta$ decay (BSBD) rates in both low-density NLTE and high-density LTE plasmas. We conclude by validating our model with state-of-the-art data in literature on isotopes of Pr and Dy, and by proposing future extension of the model to laboratory magnetoplasmas and stellar interiors aimed at improving nucleosynthesis models., Comment: 24 pages, 12 figures, 2 tables. Submitted to Nature Communications
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- 2024
4. Nuclear β-decays in plasmas: how to correlate plasma density and temperature to the activity
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Naselli Eugenia, Mascali David, Caliri Claudia, Castro Giuseppe, Celona Luigi, Galatá Alessio, Gammino Santo, Mazzaglia Maria, Romano Francesco Paolo, Giuseppe Torrisi, Santonocito Domenico, Cosentino Gianluigi, and Amaducci Simone
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Physics ,QC1-999 - Abstract
Magnetized plasmas in compact traps may become experimental en-vironments for the investigation of nuclear beta-decays of astrophysical inter-est. In the framework of the project PANDORA (Plasmas for Astrophysics, Nuclear Decays Observation and Radiation for Archaeometry) the research ac-tivities are devoted to demonstrate the feasibility of an experiment aiming atmeasuring lifetimes of radionuclides of astrophysical interest when changing the charge state distribution of the in-plasma ions and the other plasma param- eters such as density and temperature. This contribution describes the multidi-agnostics setup now available at INFN-LNS, which allows unprecedented in-vestigations of magnetoplasmas properties in terms of density, temperature and charge state distribution (CSD). The setup includes an interfero-polarimeter for total plasma density measurement, a multi-X-ray detectors system for X-ray spectroscopy (including time resolved spectroscopy), an X-ray pin-hole camera for high-resolution 2D space resolved spectroscopy, a two-pin plasma-chamber immersed antenna for the detection of plasma radio-self-emission, and differ- ent spectrometers for the plasma-emitted visible light characterization. The setup is also suitable for other studies of astrophysical interest, such as turbulent plasma regimes dominated by the so-called Cyclotron Maser Instability, which is a typical kinetic turbulence occurring in astrophysical objects like magnetized stars, brown dwarfs, etc. A description of recent results about plasma parame- ters characterization in quiescent and turbulent Electron Cyclotron Resonance-heated plasmas will be given.
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- 2020
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5. The PANDORA project: an experimental setup for measuring in-plasma β-decays of astrophysical interest
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Mascali David, Busso Maurizio, Mengoni Alberto, Amaducci Simone, Giuseppe Castro, Celona Luigi, Cosentino Gianluigi, Cristallo Sergio, Finocchiaro Paolo, Galata Alessio, Gammino Santo, Massimi Cristian, Maggiore Mario, Mauro Giorgio, Maria Mazzaglia, Naselli Eugenia, Odorici Fabrizio, Palmerini Sara, Santonocito Domenico, and Giuseppe Torrisi
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Physics ,QC1-999 - Abstract
Experiments performed on Storage Rings have shown that lifetimes of beta-radionuclides can change dramatically as a function of theionization state. PANDORA (Plasmas for Astrophysics, Nuclear Decay Observation and Radiation for Archaeometry) aims at measuring, for the first time, nuclear β-decay rates in stellar-like conditions, especially for radionuclides involved in nuclear-astrophysics processes (BBN, s- processing, CosmoChronometers, Early Solar System formation). Compact magnetic plasma traps, where plasmas reach density ne~10n-1014 cm-3, and temperature Te~0.1-30 keV, are suitable for such studies. The decay rates can be measured as a function of the charge state distribution of the inplasma ions. The collaboration is now designing the plasma trap able to reach the needed plasma densities, temperatures and charge states distributions. A first list of radioisotopes, including tens of physics cases of potential interest is now available. Possible physics cases include, among the others, 2°4Tl, 63Ni, 6°Co, 171Tm, 147Pm, 85Kr, 176Lu and the pairs 187Re-187Os and 87Sr-87Rb, which play a crucial role as cosmo-clock. Physics cases are now under evaluation in terms of lifetime measurements feasibility in a plasma trap.
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- 2020
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6. Innovative launching schemes in ECR ion sources
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Torrisi Giuseppe, Mascali David, Sorbello Gino, Castro Giuseppe, Naselli Eugenia, Leonardi Ornella, Celona Luigi, and Gammino Santo
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Physics ,QC1-999 - Abstract
An optimised RF power delivery in magnetoplasmas of ECR ion sources is crucial in order to provide a cost effective upgrade (plasma density and temperature increase and multiply charged ions production) of these machines without recurring to higher and higher magnetic fields, power level and pumping wave frequency. This can be done by following two strategies: a) in a pure ECR-heating scenario, by multiplexing different frequencies; b) in a modal-conversion scenario, by multiple-launching at different frequencies, controllable angles and polarization. The paper will show two typical cases in both the aforementioned scenarios, as developed at INFN-LNS. Test-benches have been developed on purpose, such as the “Plasma Reactor” and “Flexible Plasma Trap”, and solutions have been proposed also for ion beams current boosting in the injectors of the Superconducting Cyclotron.
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- 2017
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7. Nanostructured surfaces for nuclear astrophysics studies in laser-plasmas
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Altana Carmen, Amarù Vincenzo, Castro Giuseppe, Frassetto Marco, Lanzalone Gaetano, Malferrari Luciana, Mascali David, Muoio Annamaria, Odorici Fabrizio, and Tudisco Salvo
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Physics ,QC1-999 - Abstract
The future availability of high-intensity laser facilities capable of delivering tens of petawatts of power (e.g. ELI-NP) into small volumes of matter at high repetition rates will give the unique opportunity to investigate nuclear reactions and fundamental interactions process under extreme plasma conditions [1]. In this context, use of targets with nanostructured surfaces is giving promising indications to reproduce plasma conditions suitable for measurements of thermonuclear reactions rates, in the domain of nanosecond laser pulses.
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- 2017
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8. Modelling RF-plasma interaction in ECR ion sources
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Mascali David, Torrisi Giuseppe, Galatà Alessio, Sorbello Gino, Castro Giuseppe, Celona Luigi, Lega Lorenzo, Leonardi Ornella, Mazzaglia Maria, Naselli Eugenia, Neri Lorenzo, and Gammino Santo
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Physics ,QC1-999 - Abstract
This paper describes three-dimensional self-consistent numerical simulations of wave propagation in magnetoplasmas of Electron cyclotron resonance ion sources (ECRIS). Numerical results can give useful information on the distribution of the absorbed RF power and/or efficiency of RF heating, especially in the case of alternative schemes such as mode-conversion based heating scenarios. Ray-tracing approximation is allowed only for small wavelength compared to the system scale lengths: as a consequence, full-wave solutions of Maxwell-Vlasov equation must be taken into account in compact and strongly inhomogeneous ECRIS plasmas. This contribution presents a multi-scale temporal domains approach for simultaneously including RF dynamics and plasma kinetics in a “cold-plasma”, and some perspectives for “hot-plasma” implementation. The presented results rely with the attempt to establish a modal-conversion scenario of OXB-type in double frequency heating inside an ECRIS testbench.
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- 2017
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9. Presolar grain isotopic ratios as constraints to nuclear and stellar parameters of AGB nucleosynthesis
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Palmerini, Sara, Busso, Maurizio, Vescovi, Diego, Naselli, Eugenia, Pidatella, Angelo, Mucciola, Riccardo, Cristallo, Sergio, Mascali, David, Mengoni, Alberto, Simonucci, Stefano, and Taioli, Simone
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Astrophysics - Solar and Stellar Astrophysics ,Nuclear Experiment ,Nuclear Theory - Abstract
Recent models for evolved Low Mass Stars (with $M \lesssim 3M_\odot$), undergoing the AGB phase assume that magnetic flux-tube buoyancy drives the formation of $^{13}$C reservoirs in He-rich layers. We illustrate their crucial properties, showing how the low abundance of $^{13}$C generated below the convective envelope hampers the formation of primary $^{14}$N and the ensuing synthesis of intermediate-mass nuclei, like $^{19}$F and $^{22}$Ne. In the mentioned models, their production is therefore of a purely secondary nature. Shortage of primary $^{22}$Ne has also important effects in reducing the neutron density. Another property concerns AGB winds, which are likely to preserve C-rich subcomponents, isolated by magnetic tension, even when the envelope composition is O-rich. Conditions for the formation of C-rich compounds are therefore found in stages earlier than previously envisaged. These issues, together with the uncertainties related to several nuclear physics quantities, are discussed in the light of the isotopic admixtures of s-process elements in presolar SiC grains of stellar origin, which provide important and precise constraints to the otherwise uncertain parameters. By comparing nucleosynthesis results with measured SiC data, it is argued that such a detailed series of constraints indicates the need for new measurements of weak interaction rates in ionized plasmas, as well as of neutron-capture cross sections, especially near the N = 50 and N = 82 neutron magic numbers. Nontheless, the peculiarity of our models allows us to achieve fits to the presolar grain data of a quality so far never obtained in previously published attempts., Comment: 33 pages, 38 figures, ApJ accepted
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- 2021
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10. In-plasma study of opacity relevant for compact binary ejecta
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Pidatella, Angelo, Cristallo, Sergio, Galatà, Alessio, La Cognata, Marco, Mazzaglia, Maria, Perego, Albino, Spartà, Roberta, Tumino, Aurora, Vescovi, Diego, and Mascali, David
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
In the context of the INFN project PANDORA_Gr3 (Plasma for Astrophysics, Nuclear Decays Observation and Radiation for Archaeometry) and of multi-messenger astronomy, we propose a feasibility study for in-laboratory plasma's opacity investigation, in an environment resembling thermodynamic conditions typical of the ejecta of compact binary mergers containing at least a neutron star. We aim to advance knowledge on the physics of kilonovae, the electromagnetic transients following a merger, which are relevant for the study of the origin of heavy nuclei in the Universe produced via r-process nucleosynthesis. In this paper, we present preliminary results of numerical simulations for some physics cases considered in the light of a possible experimental setup for future in-laboratory opacity spectroscopic measurements., Comment: 5 pages, 2 figures. Invited by S.I.F. to appear in Nuovo Cimento C
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- 2021
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11. Metal evaporation dynamics in electron cyclotron resonance ion sources: plasma role in the atom diffusion, ionisation, and transport
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Pidatella, Angelo, primary, Mascali, David, additional, Galatà, Alessio, additional, Mishra, Bharat, additional, Naselli, Eugenia, additional, Celona, Luigi, additional, Lang, Ralf, additional, Maimone, Fabio, additional, Mauro, Giorgio Sebastiano, additional, Santonocito, Domenico, additional, and Torrisi, Giuseppe, additional
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- 2024
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12. Design of Integrated Optics Accelerating Structures
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Torrisi, Giuseppe, primary, Mauro, Giorgio S., additional, Genre, Andres L., additional, Mascali, David, additional, Palmeri, Roberta, additional, Rocco, Davide, additional, Locatelli, Andrea, additional, Salerno, Nunzio, additional, and Sorbello, Gino, additional
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- 2023
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13. The tunable resonant IC antenna concept and its design for DTT experiment
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Milanesio, Daniele, primary, Galindo Huertas, David Leonardo, additional, Ceccuzzi, Silvio, additional, Vecchi, Giuseppe, additional, Baiocchi, Benedetta, additional, Cardinali, Alessandro, additional, Mascali, David, additional, Mauro, Giorgio Sebastiano, additional, Mirizzi, Francesco, additional, Pidatella, Angelo, additional, Ravera, Gian Luca, additional, Torrisi, Giuseppe, additional, and Tuccillo, Angelo A, additional
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- 2023
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14. The Multi-Detectors System of the PANDORA Facility: Focus on the Full-Field Pin-Hole CCD System for X-ray Imaging and Spectroscopy.
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Mascali, David, Naselli, Eugenia, Biri, Sandor, Finocchiaro, Giorgio, Galatà, Alessio, Mauro, Giorgio Sebastiano, Mazzaglia, Maria, Mishra, Bharat, Passarello, Santi, Pidatella, Angelo, Rácz, Richard, Santonocito, Domenico, and Torrisi, Giuseppe
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SPECTRAL imaging ,X-ray spectroscopy ,IMAGE converters ,X-ray imaging ,IMAGING systems ,RADIOACTIVE decay ,PLASMA turbulence - Abstract
PANDORA (Plasmas for Astrophysics Nuclear Decays Observation and Radiation for Archaeometry) is an INFN project aiming at measuring, for the first time, possible variations in in-plasma β -decay lifetimes in isotopes of astrophysical interest as a function of thermodynamical conditions of the in-laboratory controlled plasma environment. Theoretical predictions indicate that the ionization state can dramatically modify the β -decay lifetime (even of several orders of magnitude). The PANDORA experimental approach consists of confining a plasma able to mimic specific stellar-like conditions and measuring the nuclear decay lifetime as a function of plasma parameters. The β -decay events will be measured by detecting the γ -ray emitted by the daughter nuclei, using an array of 12 HPGe detectors placed around the magnetic trap. In this frame, plasma parameters have to be continuously monitored online. For this purpose, an innovative, non-invasive multi-diagnostic system, including high-resolution time- and space-resolved X-ray analysis, was developed, which will work synergically with the γ -rays detection system. In this contribution, we will describe this multi-diagnostics system with a focus on spatially resolved high-resolution X-ray spectroscopy. The latter is performed by a pin-hole X-ray camera setup operating in the 0.5–20 keV energy domain. The achieved spatial and energy resolutions are 450 µm and 230 eV at 8.1 keV, respectively. An analysis algorithm was specifically developed to obtain SPhC (Single Photon-Counted) images and local plasma emission spectrum in High-Dynamic-Range (HDR) mode. Thus, investigations of image regions where the emissivity can change by even orders of magnitude are now possible. Post-processing analysis is also able to remove readout noise, which is often observable and dominant at very low exposure times (ms). Several measurements have already been used in compact magnetic plasma traps, e.g., the ATOMKI ECRIS in Debrecen and the Flexible Plasma Trap at LNS. The main outcomes will be shortly presented. The collected data allowed for a quantitative and absolute evaluation of local emissivity, the elemental analysis, and the local evaluation of plasma density and temperature. This paper also discusses the new plasma emission models, implemented on PIC-ParticleInCell codes, which were developed to obtain powerful 3D maps of the X-rays emitted by the magnetically confined plasma. These data also support the evaluation procedure of spatially resolved plasma parameters from the experimental spectra as well as, in the near future, the development of appropriate algorithms for the tomographic reconstruction of plasma parameters in the X-ray domain. The described setups also include the most recent upgrade, consisting of the use of fast X-ray shutters with special triggering systems that will be routinely implemented to perform both space- and time-resolved spectroscopy during transient, stable, and turbulent plasma regimes (in the ms timescale). [ABSTRACT FROM AUTHOR]
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- 2024
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15. Analysis of the performance of low gain avalanche diodes for future particle detectors
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Vakili, Aref, primary, Pancheri, Lucio, additional, Farasat, Mahsa, additional, La Magna, Antonino, additional, Mascali, David, additional, and Bregoli, Matteo, additional
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- 2023
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16. Nuclear Reactions in a Laser-Driven Plasma Environment
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Denis-Petit, David, primary, Ledingham, Ken W.D., additional, McKenna, Paul, additional, Mascali, David, additional, Tudisco, Salvatore, additional, Spohr, Klaus M., additional, and Tarisien, Medhi, additional
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- 2018
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17. Nuclear physics midterm plan at LNS
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Universitat Politècnica de Catalunya. Departament de Física, Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica, Agodi, Clementina, Cappuzzello, Francesco, Cardella, Giuseppe, Cirrone, Pablo, De Filippo, Enrico, di Pietro, Alessia, Gargano, Angela, la Cognata, Marco, Mascali, David, Milluzzo, Giuliana, Nania, Rosario, José Pont, Jordi, Universitat Politècnica de Catalunya. Departament de Física, Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica, Agodi, Clementina, Cappuzzello, Francesco, Cardella, Giuseppe, Cirrone, Pablo, De Filippo, Enrico, di Pietro, Alessia, Gargano, Angela, la Cognata, Marco, Mascali, David, Milluzzo, Giuliana, Nania, Rosario, and José Pont, Jordi
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The next years will see the completion of several new facilities at Istituto Nazionale di Fisica Nucleare – Laboratori Nazionali del Sud (LNS) opening up new possibilities in the fields of nuclear structure, nuclear dynamics, nuclear astrophysics and applications. These include a new line for high-intensity cyclotron beams, a new facility for in-flight production of radioactive ion beams, the PANDORA plasma trap for multidisciplinary studies and a high-power laser for basic science and applied physics. The nuclear physics community has organized a workshop to discuss the new physics opportunities that will be possible in the middle term (5–7 years) by employing state-of-the-art detection systems. A detailed discussion of the outcome from the workshop is presented in this report., Postprint (published version)
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- 2023
18. Ku-Band Twisted Slotted Waveguide Antenna for Innovative "Plasma-Shaped" Cavity of Ion Sources
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Torrisi, Giuseppe, primary, Mauro, Giorgio S., additional, Pidatella, Angelo, additional, Sorbello, Gino, additional, Pavone, Santi C., additional, and Mascali, David, additional
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- 2023
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19. Editorial: Nuclear physics and astrophysics in plasma traps
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Mascali, David, primary, Santonocito, Domenico, additional, de Angelis, Giacomo, additional, Kratz, Karl-Ludwig, additional, Palmerini, Sara, additional, and Torrisi, Giuseppe, additional
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- 2022
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20. Experimental and numerical investigation of magneto-plasma optical properties toward measurements of opacity relevant for compact binary objects
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Pidatella, Angelo, primary, Mascali, David, additional, Bezmalinovich, Matteo, additional, Emma, Giulia, additional, Mazzaglia, Maria, additional, Mishra, Bharat, additional, Finocchiaro, Giorgio, additional, Galatà, Alessio, additional, Marletta, Salvo, additional, Mauro, Giorgio Sebastiano, additional, Naselli, Eugenia, additional, Santonocito, Domenico, additional, Torrisi, Giuseppe, additional, Cristallo, Sergio, additional, La Cognata, Marco, additional, Perego, Albino, additional, Spartà, Roberta, additional, Tumino, Aurora, additional, and Vescovi, Diego, additional
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- 2022
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21. Modeling space-resolved ion dynamics in ECR plasmas for predicting in-plasma β-decay rates
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Mishra, Bharat, primary, Galatà, Alessio, additional, Pidatella, Angelo, additional, Biri, Sándor, additional, Mauro, Giorgio Sebastiano, additional, Naselli, Eugenia, additional, Rácz, Richárd, additional, Torrisi, Giuseppe, additional, and Mascali, David, additional
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- 2022
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22. Status and Perspectives of the PANDORA Experiment: Investigating β-Decays in Magnetized Plasmas.
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Mascali, David and Santonocito, Domenico
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THERMODYNAMICS , *NUCLEOSYNTHESIS , *NUCLEAR physics , *NUCLEAR spectroscopy , *NEUTRON capture , *IMPACT ionization , *BETA decay - Abstract
It is based on the idea of exploiting the confinement properties of a plasma trap [[6]], to be built at the Laboratori Nazionali del Sud (INFN), Catania, in order to investigate, for the first time, the beta decay properties of selected radioisotopes in physical conditions resembling those of a nucleosynthesis environment. Plasma heating will be achieved through the interaction of the plasma electrons with electromagnetic waves in the range of 18 ÷ 21 GHz emitted by three microwave generators with about 6 kW of total power injected in the plasma [[7]]. Status and Perspectives of the PANDORA Experiment: Investigating -Decays in Magnetized Plasmas In most cases, for low neutron densities environments, the beta decay is significantly faster than neutron capture and therefore only neutron-rich nuclei close to the beta stability valley are populated via a complex sequence of neutron captures and beta decays. [Extracted from the article]
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- 2023
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23. Design study of a HPGe detector array for β-decay investigation in laboratory ECR plasmas
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Naselli, Eugenia, primary, Santonocito, Domenico, additional, Amaducci, Simone, additional, Celona, Luigi, additional, Galatà, Alessio, additional, Goasduff, Alain, additional, Mauro, Giorgio Sebastiano, additional, Mazzaglia, Maria, additional, Mishra, Bharat, additional, Napoli, Daniel R., additional, Pidatella, Angelo, additional, Torrisi, Giuseppe, additional, and Mascali, David, additional
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- 2022
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24. An Innovative Superconducting Magnetic Trap for Probing β-decay in Plasmas
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Mauro, Giorgio Sebastiano, primary, Celona, Luigi, additional, Torrisi, Giuseppe, additional, Pidatella, Angelo, additional, Naselli, Eugenia, additional, Russo, Filippo, additional, Mazzaglia, Maria, additional, Galatà, Alessio, additional, Maimone, Fabio, additional, Lang, Ralf, additional, Tinscher, Klaus, additional, Santonocito, Domenico, additional, and Mascali, David, additional
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- 2022
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25. Status of the AISHa Ion Source at INFN-LNS
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Celona, Luigi, Calabrese, Giuseppe, Castro, Giuseppe, Chines, Francesco, Costanzo, Giacomo, Gammino, Santo, Leonardi, Ornella, Manno, Giovanni, Mascali, David, Massara, Antonio, Maugeri, Claudio, Passarello, Santi, Russo, Filippo, Siliato, Davide, and Torrisi, Giuseppe
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Physics::Accelerator Physics ,02: Production of Highly Charged Ion Beams ,Accelerator Physics - Abstract
The AISHa ion source is an Electron Cyclotron Resonance Ion Source designed to generate high brightness multiply charged ion beams with high reliability, easy operations and maintenance for hadrontheraphy applications. The R performed by the INFN-LNS team during the 2019/2020 has allowed the improvement of the AISHa performances up to 20% for some of the extracted beams: both injection and extraction flanges has been improved and a movable electrode has been installed. The low energy beam transport has been equipped of an Emittance Measurement Unit (EMU), working through the beam wire scanners principle, for the measurement of the vertical and horizontal emittance of the beams of interest for hadrontherapy applications. Beam emittance has been characterized as a function of q/m and of the beam intensity to highlight space charge effects. If necessary, the beam wire scanners can be used for the characterization of the beam shape. The perspectives for further developments and plasma diagnostics will be also highlighted., Proceedings of the 24th International Workshop on ECR Ion Sources, ECRIS2020, East Lansing, MI, USA
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- 2022
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26. Electromagnetic Simulation of 'plasma-shaped' Plasma Chamber for Innovative ECRIS
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Mauro, Giorgio, Galatà, Alessio, Gallo, Carmelo Sebastiano, Leonardi, Ornella, Mascali, David, Pidatella, Angelo, Russo, Filippo, Sorbello, Gino, and Torrisi, Giuseppe
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06: Codes and Simulations ,Accelerator Physics - Abstract
The plasma chamber and injection system design play a fundamental role in ECRISs with the aim to obtain an optimized electromagnetic field configuration able to generate and sustain a plasma with a high energy content. In this work we present the numerical study and the design of an unconventionally-shaped cavity resonator* that possesses some key advantages with respect to the standard cylindrical cavities, usually adopted in ion sources setups. The cavity geometry, whose design has been completed on January 2020, has been inspired by the typical star-shaped ECR plasma, determined by the magnetic field structure. The chamber has been designed by using the commercial softwares CST and COMSOL, with the aim to maximize the on-axis electric field. Moreover, a radically innovative microwaves injection system, consisting in side-coupled slotted waveguides, has been implemented, allowing a better power coupling and a more symmetric power distribution inside the cavity with respect to the standard rectangular waveguides. This new ’plasma-shaped oriented’ design could relevantly improve the performances of the ECRISs while making more compact the overall setup., Proceedings of the 24th International Workshop on ECR Ion Sources, ECRIS2020, East Lansing, MI, USA
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- 2022
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27. High Resolution X-ray Imaging as a Powerful Diagnostics Tool to Investigate ECRIS Plasma Structure and Confinement Dynamics
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Naselli, Eugenia, Biri, Sandor, Castro, Giuseppe, Celona, Luigi, Galatà, Alessio, Gammino, Santo, Mascali, David, Mazzaglia, Maria, Pálinkás, Jozsef, Perduk, Zoltan, Rácz, Richárd, and Torrisi, Giuseppe
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Accelerator Physics ,01: Fundamental Processes - Abstract
High resolution spatially-resolved X-ray spectroscopy, by means of a X-ray pin-hole camera setup* ** operating in the 0.5-20 keV energy domain, is a very powerful method for ECRIS plasma structure evaluation. We present the setup installed at a 14 GHz ECRIS (ATOMKI, Debrecen), including a multi-layered collimator enabling measurements up to several hundreds of watts of RF pumping power and the achieved spatial and energy resolution (0.5 mm and 300 eV). Results coming by a new algorithm for analyzing Integrated (multi-events detection) and Photon-Counted images (single-event detection) to perform energy-resolved investigation will be described. The analysis permits to investigate High-Dynamic-Range (HDR) and spectrally resolved images, to study the effect of the axial and radial confinement (even separately), the plasma radius, the fluxes of deconfined electrons distinguishing fluorescence lines of the materials of the plasma chamber (Ti, Ta) from plasma (Ar) fluorescence lines. This method allows a detailed characterization of warm electrons, important for ionization, and to quantitatively estimate local plasma density and spectral temperature pixel-by-pixel., Proceedings of the 24th International Workshop on ECR Ion Sources, ECRIS2020, East Lansing, MI, USA
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- 2022
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28. Advancements in Self-Consistent Modeling of Time- and Space-Dependent Phenomena in ECRIS Plasma
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Pidatella, Angelo, Galatà, Alessio, Mascali, David, Mishra, Bharat, Naselli, Eugenia, and Torrisi, Giuseppe
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06: Codes and Simulations ,Physics::Plasma Physics ,Accelerator Physics - Abstract
Resonant interaction with microwave radiation in ECRIS plasma leads to a strongly anisotropic electron energy distribution function (EEDF), given as a combination of two to three electron populations, with anisotropy that might trigger kinetic instabilities. At the INFN, further efforts have been paid to improve and update self-consistent 3D numerical codes for plasma electrons kinetics. Progresses have opened several perspectives. It is now possible to derive a space-resolved EEDF, providing local information on electron properties. Also, the code has been updated to provide reaction rates of electromagnetic emissions, including X-ray fluorescence. Estimates of the local ion charge state distribution is potentially possible, and first evaluations are ongoing. Dealing with fast-transient mechanisms, such as electromagnetic emission via the electron-cyclotron MASER instability, the code is now updated for locally evaluating the EEDF anisotropy. We will present the collected results, which we believe to have a relevant impact both on the ECRIS plasma physics and on the INFN’s PANDORA project that plans to use ECR plasmas for fundamental studies in Nuclear and AstroNuclear Physics., Proceedings of the 24th International Workshop on ECR Ion Sources, ECRIS2020, East Lansing, MI, USA
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- 2022
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29. Imaging in X-ray Ranges to Locally Investigate the Effect of the Two-Close-Frequency Heating in ECRIS Plasmas
- Author
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Rácz, Richárd, Biri, Sandor, Castro, Giuseppe, Celona, Luigi, Galatà, Alessio, Gammino, Santo, Mascali, David, Mazzaglia, Maria, Naselli, Eugenia, Pálinkás, Jozsef, Perduk, Zoltan, and Torrisi, Giuseppe
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Physics::Plasma Physics ,Astrophysics::High Energy Astrophysical Phenomena ,Accelerator Physics ,01: Fundamental Processes - Abstract
Plasma instabilities limit the ECR Ion Sources performances in terms of flux of the extracted highly charged ions by causing beam ripple and unstable operation conditions. In a 14 GHz ECRIS (Atomki, Debrecen), the effect on the plasma instabilities in an Argon plasma at Two Close Frequencies heating scheme (the frequency gap is smaller than 1 GHz) has been explored. A special multi-diagnostic setup [1, 2] has been designed and implemented consisting of detectors for the simultaneous collection of plasma radio-self-emission and of high spatial resolution X-ray images in the 500 eV - 20 keV energy domain (using an X-ray pin-hole camera setup). We present the comparison of plasma structural changes as observed from X-ray images in single and double-frequency operations. The latter has been particularly correlated to the confinement and velocity anisotropy, also by considering results coming from numerical simulations., Proceedings of the 24th International Workshop on ECR Ion Sources, ECRIS2020, East Lansing, MI, USA
- Published
- 2022
- Full Text
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30. Numerical Simulation of a Hollow-Core Woodpile-Based Mode Launcher for Dielectric Laser Accelerators
- Author
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Mauro, Giorgio Sebastiano, primary, Torrisi, Giuseppe, additional, Locatelli, Andrea, additional, Bacci, Alberto, additional, De Angelis, Costantino, additional, Mascali, David, additional, and Sorbello, Gino, additional
- Published
- 2022
- Full Text
- View/download PDF
31. Microwave techniques for electron cyclotron resonance plasma diagnostics
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Mascali, David, primary, Naselli, Eugenia, additional, and Torrisi, Giuseppe, additional
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- 2022
- Full Text
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32. A Novel Approach to β-Decay: PANDORA, a New Experimental Setup for Future In-Plasma Measurements
- Author
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Mascali, David, primary, Santonocito, Domenico, additional, Amaducci, Simone, additional, Andò, Lucio, additional, Antonuccio, Vincenzo, additional, Biri, Sándor, additional, Bonanno, Alfio, additional, Bonanno, Vincenza Piera, additional, Briefi, Stefan, additional, Busso, Maurizio, additional, Celona, Luigi, additional, Cosentino, Luigi, additional, Cristallo, Sergio, additional, Cuffiani, Marco, additional, De Angelis, Costantino, additional, De Angelis, Giacomo, additional, De Salvador, Davide, additional, Di Donato, Loreto, additional, Ducret, Jean-Eric, additional, Eshkevar Vakili, Aref, additional, Fantz, Ursel, additional, Galatà, Alessio, additional, Gallo, Carmelo Sebastiano, additional, Gammino, Santo, additional, Isernia, Tommaso, additional, Koivisto, Hannu, additional, Kratz, Karl-Ludwig, additional, Kronholm, Risto, additional, La Cognata, Marco, additional, Leoni, Silvia, additional, Locatelli, Andrea, additional, Maggiore, Mario, additional, Maimone, Fabio, additional, Malferrari, Luciana, additional, Mancini, Giorgio, additional, Maunoury, Laurent, additional, Mauro, Giorgio Sebastiano, additional, Mazzaglia, Maria, additional, Mengoni, Alberto, additional, Miraglia, Andrea, additional, Mishra, Bharat, additional, Musumeci, Mario, additional, Napoli, Daniel Ricardo, additional, Naselli, Eugenia, additional, Odorici, Fabrizio, additional, Palladino, Libero, additional, Palmisano, Giuseppe, additional, Pavone, Santi, additional, Pennisi, Salvatore, additional, Perego, Albino, additional, Pidatella, Angelo, additional, Rácz, Richard, additional, Reitano, Riccardo, additional, Rifuggiato, Danilo, additional, Rinaldi, Matteo, additional, Russo, Antonio Domenico, additional, Russo, Filippo, additional, Schillaci, Gaetano, additional, Selleri, Stefano, additional, Simonucci, Stefano, additional, Sorbello, Gino, additional, Spartà, Roberta, additional, Taioli, Simone, additional, Tinschert, Klaus, additional, Torrisi, Giuseppe, additional, Trifirò, Antonio, additional, Tsikata, Sedina, additional, Tumino, Aurora, additional, Vescovi, Diego, additional, and Vincetti, Luca, additional
- Published
- 2022
- Full Text
- View/download PDF
33. Innovative Analytical Method for X-ray Imaging and Space-Resolved Spectroscopy of ECR Plasmas
- Author
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Naselli, Eugenia, primary, Rácz, Richard, additional, Biri, Sandor, additional, Mazzaglia, Maria, additional, Celona, Luigi, additional, Gammino, Santo, additional, Torrisi, Giuseppe, additional, Perduk, Zoltan, additional, Galatà, Alessio, additional, and Mascali, David, additional
- Published
- 2021
- Full Text
- View/download PDF
34. Experimental study of single vs. two-close-frequency heating impact on confinement and losses dynamics in ECR Ion Sources plasmas by means of X-ray spectroscopy and imaging
- Author
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Mascali, David, primary, Naselli, Eugenia, additional, Racz, Richard, additional, Biri, Sándor, additional, Celona, Luigi, additional, Galatá, Alessio, additional, Gammino, Santo, additional, Mazzaglia, Maria, additional, and Torrisi, Giuseppe, additional
- Published
- 2021
- Full Text
- View/download PDF
35. Probing Electron Properties in ECR Plasmas Using X-ray Bremsstrahlung and Fluorescence Emission
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Mishra, Bharat, primary, Pidatella, Angelo, additional, Galatà, Alessio, additional, Biri, Sandor, additional, Rácz, Richard, additional, Naselli, Eugenia, additional, Mazzaglia, Maria, additional, Torrisi, Giuseppe, additional, and Mascali, David, additional
- Published
- 2021
- Full Text
- View/download PDF
36. Presolar Grain Isotopic Ratios as Constraints to Nuclear and Stellar Parameters of Asymptotic Giant Branch Star Nucleosynthesis
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Palmerini, Sara, primary, Busso, Maurizio, additional, Vescovi, Diego, additional, Naselli, Eugenia, additional, Pidatella, Angelo, additional, Mucciola, Riccardo, additional, Cristallo, Sergio, additional, Mascali, David, additional, Mengoni, Alberto, additional, Simonucci, Stefano, additional, and Taioli, Simone, additional
- Published
- 2021
- Full Text
- View/download PDF
37. Numerical Simulation and Beam-Dynamics Study of a Hollow-Core Woodpile Coupler for Dielectric Laser Accelerators
- Author
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Mauro, Giorgio, Bacci, Alberto, De Angelis, Costantino, Locatelli, Andrea, Mascali, David, Rossi, Andrea, Sorbello, Gino, and Torrisi, Giuseppe
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MC5: Beam Dynamics and EM Fields ,Physics::Accelerator Physics ,Physics::Optics ,Accelerator Physics - Abstract
Hollow core dielectric microstructures powered by lasers represent a new and promising area of accelerator research thanks to the higher damage threshold and accelerating gradients with respect to metals at optical wavelengths. In this paper we present the design of a dielectric Electromagnetic Band Gap (EBG) mode converter for high-power coupling of the accelerating mode in Dielectric Laser Accelerators (DLAs). The design is wavelength-independent, and here we propose an implementation operating at 90.505 GHz (wavelength 3.3 mm) based on a silicon woodpile structure. The coupler is composed by two perpendicularly coupled hollow-core waveguides: a TE-like mode waveguide (excited from RF/laser power) and a TM-like mode accelerating waveguide. The structure has been numerically designed and optimized, presenting Insertion Losses (IL) 0.3 dB and an efficient mode conversion in the operating bandwidth. The properties and effectiveness of the confined accelerating mode have been optimized in order to derive the needed accelerating gradient. The simulated electric field has been used as input for Astra beam-dynamics simulations in order to compute the beam properties., Proceedings of the 12th International Particle Accelerator Conference, IPAC2021, Campinas, SP, Brazil
- Published
- 2021
- Full Text
- View/download PDF
38. Light Emitting Diodes selection for space applications based on the analysis of proton-induced damage
- Author
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Vakili, Aref Eshkevar, primary, Bassetti, Daniel, additional, Bregoli, Matteo, additional, LaMagna, Antonino, additional, Mascali, David, additional, Bellini, Vincenzo, additional, Ficorella, Francesco, additional, Ali, Omar Hammad, additional, Buffardo, Mario, additional, Finocchi, Daniele, additional, Francola, Stefano, additional, and Cianci, Corrado, additional
- Published
- 2021
- Full Text
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39. Numerical simulations of the ECR heating with waves of different frequency in electron cyclotron resonance ion sources
- Author
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Gammino, Santo, Ciavola, Giovanni, Celona, Luigi G., Mascali, David, and Maimone, Fabio
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Ion sources -- Usage ,Numerical analysis -- Methods ,Cyclotron resonance -- Evaluation ,Ion bombardment -- Methods ,Ion bombardment -- Equipment and supplies ,Plasma engineering -- Research ,Business ,Chemistry ,Electronics ,Electronics and electrical industries - Abstract
The improvement of highly charged ion production with the use of two-frequency heating (TFH) in electron cyclotron resonance ion sources (ECRISs) was observed for the first time already in 1994, but the process has not been explained in details yet. The increase of the ionization rate because of the presence of two resonance surfaces instead of one is clear but not the relation between the two frequencies and the relative weight in terms of power. A series of numerical simulations about the heating process in ECR plasmas has been carried out at INFN-LNS, based on a single particle approach. They allow one to give a reasonable explanation of the TFH of the plasma electrons in terms of the microwave field distribution over the resonance surface, which changes with the excited mode, i.e., with the frequency. By analyzing the results, some considerations about the phase relationship between the electron's gyromotion and the electromagnetic wave can be done, taking into account the stochastic heating theory of ECR plasmas. The phase difference between the two waves in this case is shown to play a role. Finally, the analysis of the simulations' output will give the possibility to explain a great deal of experimental results concerning the multifrequency heating of plasmas in ECRIS. Index Terms--Ion beams, ion sources, plasma heating, simulations.
- Published
- 2008
40. Design and Analysis of Slotted Waveguide Antenna Radiating in a “Plasma-Shaped” Cavity of an ECR Ion Source
- Author
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Mauro, Giorgio Sebastiano, primary, Torrisi, Giuseppe, additional, Leonardi, Ornella, additional, Pidatella, Angelo, additional, Sorbello, Gino, additional, and Mascali, David, additional
- Published
- 2021
- Full Text
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41. Physics and Technology of Compact Plasma Traps
- Author
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Mascali, David, Castro, Giuseppe, Celona, Luigi, Gammino, Santo, Leonardi, Ornella, Mazzaglia, Maria, Naselli, Eugenia, and Torrisi, Giuseppe
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Physics::Plasma Physics ,06 Cyclotron and FFAG Concepts, New Projects ,Accelerator Physics - Abstract
ECR Ion Sources are deemed to be among the most performing ion sources feeding particle accelerators, cyclotrons in particular. Improvements of their performances strictly depend on the knowledge of plasma physics in compact magnetic traps. The paper will comment on the results obtained by the INFN-LNS team and international collaborators by means of a multi-diagnostics setup able to monitor the evolution in space and time of several plasma parameters, simultaneously with beam extraction and analysis in the LEBT, in single vs. double frequency operations, including the RF power and magnetic field scalings, and exploring regimes dominated by plasma turbulence. The results are relevant for the operations of existing ion sources and for the design of new ones. Compact magnetic traps fashioned in a similar way of ECRISs can be considered as an experimental environment by itself: we are exploring this opportunity relying to the in-plasma measurements of radionuclides lifetimes (in particular, beta-decaying elements): CosmoChronometers or nuclei involved in the s-process nucleosynthesis are among the case studies, opening new perspectives in the nuclear astrophysics field., Proceedings of the 22nd International Conference on Cyclotrons and their Applications, Cyclotrons2019, Cape Town, South Africa
- Published
- 2020
- Full Text
- View/download PDF
42. Innovative Analytical Method for X-ray Imaging and Space-Resolved Spectroscopy of ECR Plasmas.
- Author
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Naselli, Eugenia, Rácz, Richard, Biri, Sandor, Mazzaglia, Maria, Celona, Luigi, Gammino, Santo, Torrisi, Giuseppe, Perduk, Zoltan, Galatà, Alessio, and Mascali, David
- Subjects
POLARIMETRY ,X-ray imaging ,PLASMA spectroscopy ,SPECTRAL imaging ,CYCLOTRON resonance ,EMISSION spectroscopy - Abstract
At the Italian National Institute for Nuclear Physics-Southern National Laboratory (INFN-LNS), and in collaboration with the ATOMKI laboratories, an innovative multi-diagnostic system with advanced analytical methods has been designed and implemented. This is based on several detectors and techniques (Optical Emission Spectroscopy, RF systems, interfero-polarimetry, X-ray detectors), and here we focus on high-resolution, spatially resolved X-ray spectroscopy, performed by means of a X-ray pin-hole camera setup operating in the 0.5–20 keV energy domain. The diagnostic system was installed at a 14 GHz Electron Cyclotron Resonance (ECR) ion source (ATOMKI, Debrecen), enabling high-precision, X-ray, spectrally resolved imaging of ECR plasmas heated by hundreds of Watts. The achieved spatial and energy resolutions were 0.5 mm and 300 eV at 8 keV, respectively. Here, we present the innovative analysis algorithm that we properly developed to obtain Single Photon-Counted (SPhC) images providing the local plasma-emitted spectrum in a High-Dynamic-Range (HDR) mode, by distinguishing fluorescence lines of the materials of the plasma chamber (Ti, Ta) from plasma (Ar). This method allows for a quantitative characterization of warm electrons population in the plasma (and its 2D distribution), which are the most important for ionization, and to estimate local plasma density and spectral temperatures. The developed post-processing analysis is also able to remove the readout noise that is often observable at very low exposure times (msec). The setup is now being updated, including fast shutters and trigger systems to allow simultaneous space and time-resolved plasma spectroscopy during transients, stable and turbulent regimes. [ABSTRACT FROM AUTHOR]
- Published
- 2022
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43. Impact of the Two Close Frequency Heating on ECRIS Plasmas Stability
- Author
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Naselli, Eugenia, Biri, Sandor, Caliri, Claudia, Castro, Giuseppe, Celona, Luigi, GalatÃ, Alessio, Gammino, Santo, Mascali, David, Mazzaglia, Maria, Pálinkás, Jozsef, Perduk, Zoltan, Romano, Francesco, RáCz, RicháRd, and Torrisi, Giuseppe
- Subjects
Physics::Plasma Physics ,Plasma physics and techniques ,Accelerator Physics - Abstract
Several experiments have recently demonstrated that plasma instabilities are powerful limiting factors to the flux of highly charged ion beam extracted from ECRIS. One of the methods for damping the instabilities is to feed the plasma in two frequency heating mode. Since the fundamental physical mechanism is still unclear (diffusion in velocity space? additional confinement?), a deeper experimental investigation is necessary, using multi-diagnostics setups. At ATOMKI-Debrecen the effect on the plasma instabilities of an argon plasma in a 'Two Close Frequencies' scheme has been explored. Spectra of radio-emission from the plasma have been collected for different frequency gaps and relative power balances. The measurements show the plasma self-emitted radiation comes out from the internal plasma (i.e. around the lower frequency) but the instability damping can be effective for some specific combinations of frequency-gap and power balance. Radiofrequency spectra have been collected simultaneously to time-resolved X-ray measurements, triggered by RF bursts produced by the instabilities and detected via a microwave diode connected to a plasma-chamber-immersed multi-pin RF probe., Proceedings of the 23th Int. Workshop on ECR Ion Sources, ECRIS2018, Catania, Italy
- Published
- 2019
- Full Text
- View/download PDF
44. Time Resolved X-Ray Measurements in a Simple Mirror Trap
- Author
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Salvatore, Tudisco, Altana, Carmen, Castro, Giuseppe, Celona, Luigi, Gammino, Santo, Lanzalone, Gaetano, Litrico, Frazia, Mascali, David, Mazzaglia, Maria, Miracoli, Rosalba, Muoio, Annamaria, Naselli, Eugenia, and Torrisi, Giuseppe
- Subjects
Astrophysics::High Energy Astrophysical Phenomena ,Plasma physics and techniques ,Accelerator Physics - Abstract
The time-resolved characterization of the X-ray emission represents an innovative technique to investigate the heating mechanism of the worm/hot electron component in ECRIS devices. In this paper, the technique has been described and the results of an experimental campaign of measurements in order to characterize the X-rays emission of an axis-symmetric simple mirror trap has been showed. Particular attention has been paid to the ignition and turning off phase. This approach has permitted to estimate confinement time of the warm/hot electron population and put in evidence eventual instability effects during the critical phases. Further developments and perspectives of the technique will be highlighted., Proceedings of the 23th Int. Workshop on ECR Ion Sources, ECRIS2018, Catania, Italy
- Published
- 2019
- Full Text
- View/download PDF
45. Results of the Optical Emission Spectroscopy diagnostics of the ESS proton source
- Author
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Castro, Giuseppe, Celona, Luigi, Gammino, Santo, Leonardi, Ornella, Mascali, David, Mazzaglia, Maria, Miraglia, Andrea, Naselli, Eugenia, Neri, Lorenzo, Reitano, Riccardo, and Torrisi, Giuseppe
- Subjects
Plasma physics and techniques ,Accelerator Physics - Abstract
The high intensity proton source for the European Spallation Source, designed and commissioned at INFN-LNS, is able to produce a stable total current between 40 and 125 mA through an 8 mm extraction aperture, with a proton fraction up to 87%. The best source condition for PS-ESS requirements has been investigated by means of the Optical Emission Spectroscopy (OES). OES has permitted to evaluate simultaneously the H/H2 relative abundances together with electron density and temperature. Results demonstrated that high intensity proton beams are generated in overdense plasma conditions (around 10¹⁸ m⁻³ electron density measured by OES), while electron temperature shows a decreasing trend with power. The results will be discussed and compared with Faraday-cup and Doppler shift measurements. Further upgrades of OES diagnostics will be highlighted., Proceedings of the 23th Int. Workshop on ECR Ion Sources, ECRIS2018, Catania, Italy
- Published
- 2019
- Full Text
- View/download PDF
46. An Irradiation Test Facility at INFN-LNS: Status and Perspectives
- Author
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Rapisarda, Giuseppe, Bonanno, Vincenza, Catalano, Roberto, Cirrone, Giuseppe, Cosentino, Luigi, Cuttone, Giacomo, Mascali, David, Musumeci, Mario, Petringa, Giada, Puglia, Sebastiana, Rifuggiato, Danilo, and Salvatore, Tudisco
- Subjects
Applications ,Accelerator Physics - Abstract
In the framework of ASIF "ASI Supported Irradiation Facilities" project some beamlines available at Laboratori Nazionali del Sud-INFN (LNS) Catania have been dedicated to irradiation test. These beamlines have been recently upgraded in order to meet the ESA specifications about radiation hardness testing of devices suitable for space applications. The Superconducting Cyclotron K800 installed at LNS can provide protons up to 80 MeV for integrated dose tests and a number of heavy ion beams for Single Event Effect (SEE) studies. The beamlines are equipped with detectors that allow beam diagnostic in term of spatial uniformity, purity and energy measurement, including on-line monitoring of flux and fluence received by the device under test. Upgrades activities are now ongoing, especially to broaden up the number of available beams, both in terms of ion species and energy, to optimize the switching times from one beam to another. The paper will present an overview of the developed facility, which will take benefit of the ongoing SERSE (the superconducting ECR ion source) revamping: the new gas-box system, plasma chamber and controls system are ready to be installed within autumn 2018., Proceedings of the 23th Int. Workshop on ECR Ion Sources, ECRIS2018, Catania, Italy
- Published
- 2019
- Full Text
- View/download PDF
47. Commissioning of the AISHA Ion Source at INFN-LNS
- Author
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Celona, Luigi, Castro, Giuseppe, Chines, Francesco, Gammino, Santo, Leonardi, Ornella, Mascali, David, Mazzaglia, Maria, Neri, Lorenzo, and Torrisi, Giuseppe
- Subjects
Status reports and new development ,Accelerator Physics - Abstract
The AISHa ion source has been designed to generate high brightness multiply charged ion beams with high reliability, easy operations and maintenance for hadrontheraphy applications. Aisha is a compact ECRIS whose hybrid magnetic system consists of a permanent Halbach-type hexapole magnet and a set of independently energized superconducting He-free coils. The present work shows the results of the ion source commissioning in SFH operational mode (18 GHz) for different ion species. Current status and further improvements will be highlighted., Proceedings of the 23th Int. Workshop on ECR Ion Sources, ECRIS2018, Catania, Italy
- Published
- 2019
- Full Text
- View/download PDF
48. A Finite-Difference Approach for Plasma Microwave Imaging Profilometry
- Author
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Di Donato, Loreto, primary, Mascali, David, additional, Morabito, Andrea F., additional, and Sorbello, Gino, additional
- Published
- 2019
- Full Text
- View/download PDF
49. A Fluxgate-Based Approach for Ion Beam Current Measurement in ECRIS Beamline: Design and Preliminary Investigations
- Author
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Ando, Bruno, primary, Baglio, Salvatore, additional, Crispino, Ruben, additional, Graziani, Salvatore, additional, Marletta, Vincenzo, additional, Mazzaglia, Alfio, additional, Sinatra, Valentina, additional, Mascali, David, additional, and Torrisi, Giuseppe, additional
- Published
- 2019
- Full Text
- View/download PDF
50. Numerical and Experimental Characterization of RF Waves Propagation in Ion Sources Magnetoplasmas
- Author
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Torrisi, Giuseppe, primary, Mascali, David, additional, Sorbello, Gino, additional, Castro, Giuseppe, additional, Celona, Luigi, additional, and Gammino, Santo, additional
- Published
- 2019
- Full Text
- View/download PDF
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