Search

Your search keyword '"Nose M"' showing total 799 results
Start Over Author "Nose M"
799 results on '"Nose M"'

1. Effects Of Aluminum Sputtering On The Corrosion Resistance Of AZ91 Alloy

Author

Ishibashi Y., Nose M., Hatakeyama M., and Sunada S.

Subjects
Magnesium alloy, corrosion, Aluminum, sputtering, Mining engineering. Metallurgy, TN1-997, Materials of engineering and construction. Mechanics of materials, TA401-492
Abstract

The corrosion resistance of a Magnesium alloy is low and needs to be improved. This research aimed at corrosion-resistance improvement by supatterd deposition aluminium film, which is formed on the surface of AZ91 Magnesium-alloy. Corrosion resistance performed polarization curve measurement, was evaluated in quest of the corrosion rate using the Tafel extrapolation method, and conducted surface observation and EDS analysis by SEM. Although corrosion resistance is not improved only by film forming because of defects in film, corrosion resistance is improved by heat treatment for 3 hours by 553K after sputtering. In the case of heat treated at 623K and 673K for 3 hours, magnesium diffuses through the alminium film and reached the surface of the film. Thus, heat treatment at high temperature degrade the corrosion resistance of the film. The optimization of heat treatment after sputtering is important in this method.

Published
2015
Full Text
View/download PDF

2. Crystal Structure And Optical Properties Of TiO2 Thin Films Prepared By Reactive RF Magnetron Sputtering

Author

Goto S., Adachi Y., Matsuda K., and Nose M.

Subjects
TiO2, Rutile, Anatase, sputtering, XRD, Mining engineering. Metallurgy, TN1-997, Materials of engineering and construction. Mechanics of materials, TA401-492
Abstract

In sputtering deposition process of TiO2, metal Ti or sintered TiO2 target is used as deposition source. In this study, we have compared the characteristic of target materials. When TiO2 target was used, stoichiometric TiO2 films was deposited under the Ar atmosphere containing 1.0% of oxygen. The highest sputtering rate under this atmosphere was 3.9nm/min at 3.4W/cm2. But, sintered TiO2 target is fragile and cannot endure higher density of input power than 3.4W/cm2. On the other hand, Ti target needs higher oxygen concentration (8%) in sputtering gas atmosphere for obtaining rutile/anatase. Even though Ti target can be input twice power density of 7.9W/cm2, the highest deposition rate for Ti target was 1.4/nm, which was ~35% of the highest rate for TiO2 target. Then we have study out the composite target consisting of Ti plate and TiO2 chips. Using the composite target, stoichiometric TiO2 films were prepared in the rate of 9.6nm/min at 6.8 W/cm2 under the atmosphere of Ar/2.5%O2. Furthermore, we have found that the TiO2 films obtained from the composite target consisted of about 100% anatase, whereas TiO2 films obtained from other target have rutile dominant structure. The optical band gap energy of the film is determined by using the Tauc plot. The calculated band gap energies for the films deposited by Ti target and composite target were 2.95 and 3.24eV, which are equivalent to that of rutile and anatase structure, respectively.

Published
2015
Full Text
View/download PDF

3. Mechanical Properties And Microstructure Of AlN/SiCN Nanocomposite Coatings Prepared By R.F.-Reactive Sputtering Method

Author

Nakafushi Y., Matsuda K., and Nose M.

Subjects
AlN, SiCN, XRD, sputtering, TEM, Mining engineering. Metallurgy, TN1-997, Materials of engineering and construction. Mechanics of materials, TA401-492
Abstract

FIn this work, AlN/SiCN composite coatings were deposited by r.f.-reactive sputtering method using a facing target-type sputtering (FTS) apparatus with composite targets consisting of Al plate and SiC chips in a gaseous mixture of Ar and N2, and investigated their mechanical properties and microstructure. The indentation hardness (HIT) of AlN/SiCN coatings prepared from composite targets consisting of 8 ~32 chips of SiC and Al plate showed the maximum value of about 29~32 GPa at a proper nitrogen gas flow rate. X-ray diffraction (XRD) patterns for the AlN/SiCN composite coatings indicated the presence of the only peeks of hexagonal (B4) structured AlN phase. AlN coatings clarified the columnar structure of the cross sectional view TEM observation. On the other hand, microstructure of AlN/SiCN composite coatings changed from columnar to equiaxed structure with increasing SiCN content. HR-TEM observation clarified that the composite coatings consisted of very fine equiaxial grains of B4 structured AlN phase and amorphous phase.

Published
2015
Full Text
View/download PDF

4. The Analysis Of Structure For The Multi-Layered Of Ge/TiO2 Films Prepared By The Differential Prressure Co-Sputtering

Author

Adachi Y., Abe S., Matsuda K., and Nose M.

Subjects
TiO2, Ge, solar cells, sputtering, Mining engineering. Metallurgy, TN1-997, Materials of engineering and construction. Mechanics of materials, TA401-492
Abstract

We tried to fabricate the Ge/TiO2 composite films with the differential pressure (pumping) co-sputtering (DPCS) apparatus in order to improve the optical properties. In the study, the micro structure of these thin films has been evaluated. TEM image revealed that the thin film was alternately layered with TiO2 and Ge, lattice fringes were observed both of Ge layer and TiO2 layer. There were portions that lattice fringe of Ge was disturbed near the interface of Ge and TiO2. X-ray photoelectron spectroscopy elucidated that there were few germanium oxides and a part with the thin film after annealed.

Published
2015
Full Text
View/download PDF

7. The Space Physics Environment Data Analysis System (SPEDAS).

Author

Angelopoulos, V, Cruce, P, Drozdov, A, Grimes, EW, Hatzigeorgiu, N, King, DA, Larson, D, Lewis, JW, McTiernan, JM, Roberts, DA, Russell, CL, Hori, T, Kasahara, Y, Kumamoto, A, Matsuoka, A, Miyashita, Y, Miyoshi, Y, Shinohara, I, Teramoto, M, Faden, JB, Halford, AJ, McCarthy, M, Millan, RM, Sample, JG, Smith, DM, Woodger, LA, Masson, A, Narock, AA, Asamura, K, Chang, TF, Chiang, C-Y, Kazama, Y, Keika, K, Matsuda, S, Segawa, T, Seki, K, Shoji, M, Tam, SWY, Umemura, N, Wang, B-J, Wang, S-Y, Redmon, R, Rodriguez, JV, Singer, HJ, Vandegriff, J, Abe, S, Nose, M, Shinbori, A, Tanaka, Y-M, UeNo, S, Andersson, L, Dunn, P, Fowler, C, Halekas, JS, Hara, T, Harada, Y, Lee, CO, Lillis, R, Mitchell, DL, Argall, MR, Bromund, K, Burch, JL, Cohen, IJ, Galloy, M, Giles, B, Jaynes, AN, Le Contel, O, Oka, M, Phan, TD, Walsh, BM, Westlake, J, Wilder, FD, Bale, SD, Livi, R, Pulupa, M, Whittlesey, P, DeWolfe, A, Harter, B, Lucas, E, Auster, U, Bonnell, JW, Cully, CM, Donovan, E, Ergun, RE, Frey, HU, Jackel, B, Keiling, A, Korth, H, McFadden, JP, Nishimura, Y, Plaschke, F, Robert, P, Turner, DL, Weygand, JM, Candey, RM, Johnson, RC, Kovalick, T, Liu, MH, McGuire, RE, and Breneman, A

Subjects
Geospace science, Ionospheric physics, Magnetospheric physics, Planetary magnetospheres, Solar wind, Space plasmas, Solarwind, Astronomical and Space Sciences, Astronomy & Astrophysics
Abstract

With the advent of the Heliophysics/Geospace System Observatory (H/GSO), a complement of multi-spacecraft missions and ground-based observatories to study the space environment, data retrieval, analysis, and visualization of space physics data can be daunting. The Space Physics Environment Data Analysis System (SPEDAS), a grass-roots software development platform (www.spedas.org), is now officially supported by NASA Heliophysics as part of its data environment infrastructure. It serves more than a dozen space missions and ground observatories and can integrate the full complement of past and upcoming space physics missions with minimal resources, following clear, simple, and well-proven guidelines. Free, modular and configurable to the needs of individual missions, it works in both command-line (ideal for experienced users) and Graphical User Interface (GUI) mode (reducing the learning curve for first-time users). Both options have "crib-sheets," user-command sequences in ASCII format that can facilitate record-and-repeat actions, especially for complex operations and plotting. Crib-sheets enhance scientific interactions, as users can move rapidly and accurately from exchanges of technical information on data processing to efficient discussions regarding data interpretation and science. SPEDAS can readily query and ingest all International Solar Terrestrial Physics (ISTP)-compatible products from the Space Physics Data Facility (SPDF), enabling access to a vast collection of historic and current mission data. The planned incorporation of Heliophysics Application Programmer's Interface (HAPI) standards will facilitate data ingestion from distributed datasets that adhere to these standards. Although SPEDAS is currently Interactive Data Language (IDL)-based (and interfaces to Java-based tools such as Autoplot), efforts are under-way to expand it further to work with python (first as an interface tool and potentially even receiving an under-the-hood replacement). We review the SPEDAS development history, goals, and current implementation. We explain its "modes of use" with examples geared for users and outline its technical implementation and requirements with software developers in mind. We also describe SPEDAS personnel and software management, interfaces with other organizations, resources and support structure available to the community, and future development plans.Electronic supplementary materialThe online version of this article (10.1007/s11214-018-0576-4) contains supplementary material, which is available to authorized users.

Published
2019

8. Spatial structure and temporal evolution of energetic particle injections in the inner magnetosphere during the 14 July 2013 substorm event

Author

Gkioulidou, Matina, Ohtani, S., Mitchell, D. G., Ukhorskiy, A. Y., Reeves, G. D., Turner, D. L., Gjerloev, J. W., Nosé, M., Koga, K., Rodriguez, J. V., and Lanzerotti, L. J.

Subjects
Physics - Space Physics
Abstract

Recent results by the Van Allen Probes mission showed that the occurrence of energetic ion injections inside geosynchronous orbit could be very frequent throughout the main phase of a geomagnetic storm. Understanding, therefore, the formation and evolution of energetic particle injections is critical in order to quantify their effect in the inner magnetosphere. We present a case study of a substorm event that occurred during a weak storm $\textit{ Dst }$ $\sim$ -40nT on 14 July 2013. Van Allen Probe B, inside geosynchronous orbit, observed two energetic proton injections within 10min, with different dipolarization signatures and duration. The first one is a dispersionless, short-timescale injection pulse accompanied by a sharp dipolarization signature, while the second one is a dispersed, longer-timescale injection pulse accompanied by a gradual dipolarization signature. We combined ground magnetometer data from various stations and in situ particle and magnetic field data from multiple satellites in the inner magnetosphere and near-Earth plasma sheet to determine the spatial extent of these injections, their temporal evolution, and their effects in the inner magnetosphere. Our results indicate that there are different spatial and temporal scales at which injections can occur in the inner magnetosphere and depict the necessity of multipoint observations of both particle and magnetic field data in order to determine these scales.

Published
2016
Full Text
View/download PDF

9. Simultaneous Precipitation of Sub‐Relativistic Electron Microburst and Pulsating Aurora Electrons

Author

Namekawa, T., primary, Mitani, T., additional, Asamura, K., additional, Miyoshi, Y., additional, Hosokawa, K., additional, Lessard, M., additional, Moser, C., additional, Halford, A. J., additional, Sakanoi, T., additional, Kawamura, M., additional, Nose, M., additional, Nomura, R., additional, Teramoto, M., additional, Shumko, M., additional, Lynch, K. A., additional, Jaynes, A. N., additional, and McHarg, M. G., additional

Published
2023
Full Text
View/download PDF

11. Excitation of drift-compressional mode waves by drift resonance with ring current ions: Arase observation

Author

Yamamoto, K., Rubtsov, A., Kostarev, D., Mager, P., Klimushkin, D., Nose, M., Matsuoka, A., Asamura, K., Miyoshi, Y., Yokota, S., Kasahara, S., Kasahara, Y., and Shinohara, I.

Abstract

Compressional Pc 5 waves are important for the energy dynamics in the terrestrial inner magnetosphere because they can accelerate the relativistic electrons (Ukhorskiy et al., 2009). One of the origins of compressional Pc 5 waves is local plasma instability, but the generation mechanism of the compressional Pc 5 waves is still controversial. Recently, drift compressional instability has been focused on because it can generate compressional waves even if plasma beta is less than unity (Rubtsov et al., 2018; Mager et al., 2019; Takahashi et al., 2022). However, the wave property and excitation mechanism of the drift compressional mode are not fully understood due to the lack of observation.This study reports the role of drift resonance in the excitation of drift compressional waves observed by the Arase satellite on 19th November 2018. From the theoretical calculations of the wave frequency (Mager et al., 2013) and pressure perturbation (Takahashi et al., 2022), we concluded that the observed wave is the drift compressional mode. We estimated the azimuthal wave number (m number) from the finite Larmor radius effect and obtained m ~ -140. This is consistent with the drift resonance with protons at 20-30 keV, whose fluxes showed the most coherent oscillations. In addition to a positive radial gradient of ion temperature, we found that an inward phase space density gradient and positive df/dW sometimes appeared, which indicates that the drift resonance gives free energy to the wave, where f and W are phase space density and energy, respectively., The 28th IUGG General Assembly (IUGG2023) (Berlin 2023)

Published
2023
Full Text
View/download PDF

14. Comparing Long-Acting Antipsychotic Discontinuation Rates Under Ordinary Clinical Circumstances: A Survival Analysis from an Observational, Pragmatic Study

Author

Bertolini, F., Ostuzzi, G., Pievani, M., Aguglia, A., Bartoli, F., Bortolaso, P., Callegari, C., Caroleo, M., Carra, G., Corbo, M., D'Agostino, A., De Fazio, P., Magliocco, F., Martinotti, G., Ostinelli, E. G., Piccinelli, M. P., Tedeschi, F., Barbui, C., Boschello, F., Gastaldon, C., Mazzi, M. A., Nose, M., Papola, D., Perini, G., Piccoli, A., Purgato, M., Ruggeri, M., Terlizzi, S., Turrini, G., Raffaele, G., Cavallotti, S., Chirico, M., Ferrato, F., Limosani, I., Mastromo, D., Monzani, E., Porcellana, M., Restaino, F., Annese, P. M., Bolognesi, S., Cerretini, M., De Capua, A., Debolini, S., Del Zanna, M., Fargnoli, F., Giannini, A., Luccarelli, L., Lucii, C., Pierantozzi, E., Tozzi, F., Bardicchia, F., Cardamone, G., Facchi, E., Magnani, N., Soscia, F., Biancosino, B., Zotos, S., Giacomin, M., Pompei, F., Spano, M., Zonta, F., Buzzi, A., Callegred, C., Calzolari, R., Caselli, I., Diurni, M., Giana, E., Ielmini, M., Milano, A., Poloni, N., Sani, E., Zizolfi, D., Alberini, G., Cazzamalli, S., Costantini, C., Di Caro, A., Paronelli, C., Piantanida, S., Piccinelli, M., Alessandro, P., Barbanti, S. V., D'Ippolito, C., Gozzi, M., Moretti, V., Campese, O., Di Capro, L., di Giannantonio, M., Fiori, F., Lorusso, M., Mancini, V., Viceconte, D., Calandra, C., Luca, M., Signorelli, M. S., Suraniti, F., Balzarro, B., Boncompagni, G., Caretto, V., Emiliani, R., Lupoli, P., Menchetti, M., Rossi, E., Storbini, V., Tarricone, I., Terzi, L., Boso, M., Catania, C., De Paoli, G., Risaro, P., Aspesi, F., Bava, M., Bono, A., Brambilla, G., Castagna, G., Lucchi, S., Nava, R., Provenzi, M., Tabacchi, T., Tremolada, M., Verrengia, E., Barchiesi, M., Oriani, M. G., Pacetti, M., Ferro, M., Ghio, L., Beneduce, R., Laffranchini, L., Magni, L. R., Rossi, G., Tura, G. B., Addeo, L., Balletta, G., De Vivo, E., Di Benedetto, R., Parise, V. F., Carpiniello, B., Pinna, F., Pecile, D., Mattei, C., Bonavigo, T., Fabrici, E. P., Panarello, S., Peresson, G., Vitucci, C., Gardellin, F., Strizzolo, S., Cossetta, E., Fizzotti, C., Moretti, D., Di Gregorio, L., Sozzi, F., Colli, G., La Barbera, D., Laurenzi, S., Bertolini, F, Ostuzzi, G, Pievani, M, Aguglia, A, Bartoli, F, Bortolaso, P, Callegari, C, Caroleo, M, Carra, G, Corbo, M, D'Agostino, A, De Fazio, P, Magliocco, F, Martinotti, G, Ostinelli, E, Piccinelli, M, Tedeschi, F, Barbui, C, Boschello, F, Gastaldon, C, Mazzi, M, Nose, M, Papola, D, Perini, G, Piccoli, A, Purgato, M, Ruggeri, M, Terlizzi, S, Turrini, G, Raffaele, G, Cavallotti, S, Chirico, M, Ferrato, F, Limosani, I, Mastromo, D, Monzani, E, Porcellana, M, Restaino, F, Annese, P, Bolognesi, S, Cerretini, M, De Capua, A, Debolini, S, Del Zanna, M, Fargnoli, F, Giannini, A, Luccarelli, L, Lucii, C, Pierantozzi, E, Tozzi, F, Bardicchia, F, Cardamone, G, Facchi, E, Magnani, N, Soscia, F, Biancosino, B, Zotos, S, Giacomin, M, Pompei, F, Spano, M, Zonta, F, Buzzi, A, Calzolari, R, Caselli, I, Diurni, M, Giana, E, Ielmini, M, Milano, A, Poloni, N, Sani, E, Zizolfi, D, Alberini, G, Cazzamalli, S, Costantini, C, Di Caro, A, Paronelli, C, Piantanida, S, Alessandro, P, Barbanti, S, D'Ippolito, C, Gozzi, M, Moretti, V, Campese, O, Di Capro, L, di Giannantonio, M, Fiori, F, Lorusso, M, Mancini, V, Viceconte, D, Calandra, C, Luca, M, Signorelli, M, Suraniti, F, Balzarro, B, Boncompagni, G, Caretto, V, Emiliani, R, Lupoli, P, Menchetti, M, Rossi, E, Storbini, V, Tarricone, I, Terzi, L, Boso, M, Catania, C, De Paoli, G, Risaro, P, Aspesi, F, Bava, M, Bono, A, Brambilla, G, Castagna, G, Lucchi, S, Nava, R, Provenzi, M, Tabacchi, T, Tremolada, M, Verrengia, E, Barchiesi, M, Oriani, M, Pacetti, M, Ferro, M, Ghio, L, Beneduce, R, Laffranchini, L, Magni, L, Rossi, G, Tura, G, Addeo, L, Balletta, G, De Vivo, E, Di Benedetto, R, Parise, V, Carpiniello, B, Pinna, F, Pecile, D, Mattei, C, Bonavigo, T, Fabrici, E, Panarello, S, Peresson, G, Vitucci, C, Gardellin, F, Strizzolo, S, Cossetta, E, Fizzotti, C, Moretti, D, Di Gregorio, L, Sozzi, F, Colli, G, La Barbera, D, Laurenzi, S, Bertolini F., Ostuzzi G., Pievani M., Aguglia A., Bartoli F., Bortolaso P., Callegari C., Caroleo M., Carra G., Corbo M., D'Agostino A., De Fazio P., Magliocco F., Martinotti G., Ostinelli E.G., Piccinelli M.P., Tedeschi F., Barbui C., Boschello F., Gastaldon C., Mazzi M.A., Nose M., Papola D., Perini G., Piccoli A., Purgato M., Ruggeri M., Terlizzi S., Turrini G., Raffaele G., Cavallotti S., Chirico M., Ferrato F., Limosani I., Mastromo D., Monzani E., Porcellana M., Restaino F., Annese P.M., Bolognesi S., Cerretini M., De Capua A., Debolini S., Del Zanna M., Fargnoli F., Giannini A., Luccarelli L., Lucii C., Pierantozzi E., Tozzi F., Bardicchia F., Cardamone G., Facchi E., Magnani N., Soscia F., Biancosino B., Zotos S., Giacomin M., Pompei F., Spano M., Zonta F., Buzzi A., Callegred C., Calzolari R., Caselli I., Diurni M., Giana E., Ielmini M., Milano A., Poloni N., Sani E., Zizolfi D., Alberini G., Cazzamalli S., Costantini C., Di Caro A., Paronelli C., Piantanida S., Piccinelli M., Alessandro P., Barbanti S.V., D'Ippolito C., Gozzi M., Moretti V., Campese O., Di Capro L., di Giannantonio M., Fiori F., Lorusso M., Mancini V., Viceconte D., Calandra C., Luca M., Signorelli M.S., Suraniti F., Balzarro B., Boncompagni G., Caretto V., Emiliani R., Lupoli P., Menchetti M., Rossi E., Storbini V., Tarricone I., Terzi L., Boso M., Catania C., De Paoli G., Risaro P., Aspesi F., Bava M., Bono A., Brambilla G., Castagna G., Lucchi S., Nava R., Provenzi M., Tabacchi T., Tremolada M., Verrengia E., Barchiesi M., Oriani M.G., Pacetti M., Ferro M., Ghio L., Beneduce R., Laffranchini L., Magni L.R., Rossi G., Tura G.B., Addeo L., Balletta G., De Vivo E., Di Benedetto R., Parise V.F., Carpiniello B., Pinna F., Pecile D., Mattei C., Bonavigo T., Fabrici E.P., Panarello S., Peresson G., Vitucci C., Gardellin F., Strizzolo S., Cossetta E., Fizzotti C., Moretti D., Di Gregorio L., Sozzi F., Colli G., La Barbera D., and Laurenzi S.

Subjects
Male, Pediatrics, respectively), 0302 clinical medicine, Delayed-Action Preparation, Brief Psychiatric Rating Scale, Pharmacology (medical), he STAR Network ‘Depot Study’ prospectively followed 394 subjects initiating treatment with long-acting injections (LAIs) of antipsychotics under naturalistic conditions for 12 months. LAI discontinuation was frequent in everyday clinical practice in Italy, Original Research Article, Prospective Studies, Prospective cohort study, treatment, Mental Disorders, Hazard ratio, whereas more than half of participants initiating risperidone LAI and olanzapine LAI discontinued during the 12 months of follow-up (51.4 and 62.5%, Psychiatric Status Rating Scale, Middle Aged, side efects, Psychiatry and Mental health, Italy, Mental Disorder, Female, he STAR Network ‘Depot Study’ prospectively followed 394 subjects initiating treatment with long-acting injections (LAIs) of antipsychotics under naturalistic conditions for 12 months. LAI discontinuation was frequent in everyday clinical practice in Italy, occurring in almost 40% of the entire sample, side efects, participant refusal to continue LAIs and LAIs no longer being required were the most frequently reported reasons for discontinuation. Paliperidone LAI and aripiprazole LAI were the least discontinued medications (33.9 and 35.4%, respectively), whereas more than half of participants initiating risperidone LAI and olanzapine LAI discontinued during the 12 months of follow-up (51.4 and 62.5%, respectively). In multivariate analysis, being prescribed olanzapine LAI and poor medication adherence at baseline were signifcantly associated with higher discontinuation risk, Human, Antipsychotic Agents, medicine.drug, Psychopathology, Adult, medicine.medical_specialty, Discontinuation, Follow-Up Studie, Medication Adherence, 03 medical and health sciences, medicine, Humans, Paliperidone, Adverse effect, Settore MED/25 - Psichiatria, discontinuation rates, Psychiatric Status Rating Scales, respectively). In multivariate analysis, business.industry, Long-Acting Antipsychotic, long-acting injectable antipsychotics, Survival Analysis, Confidence interval, participant refusal to continue LAIs and LAIs no longer being required were the most frequently reported reasons for discontinuation. Paliperidone LAI and aripiprazole LAI were the least discontinued medications (33.9 and 35.4%, 030227 psychiatry, Prospective Studie, Antipsychotic Agent, occurring in almost 40% of the entire sample, Delayed-Action Preparations, Neurology (clinical), business, 030217 neurology & neurosurgery, being prescribed olanzapine LAI and poor medication adherence at baseline were signifcantly associated with higher discontinuation risk, Follow-Up Studies
Abstract

Background Recent guidelines suggested a wider use of long-acting injectable antipsychotics (LAI) than previously, but naturalistic data on the consequences of LAI use in terms of discontinuation rates and associated factors are still sparse, making it hard for clinicians to be informed on plausible treatment courses. Objective Our objective was to assess, under real-world clinical circumstances, LAI discontinuation rates over a period of 12 months after a first prescription, reasons for discontinuation, and associated factors. Methods The STAR Network ‘Depot Study’ was a naturalistic, multicentre, observational prospective study that enrolled subjects initiating a LAI without restrictions on diagnosis, clinical severity or setting. Participants from 32 Italian centres were assessed at baseline and at 6 and 12 months of follow-up. Psychopathology, drug attitude and treatment adherence were measured using the Brief Psychiatric Rating Scale, the Drug Attitude Inventory and the Kemp scale, respectively. Results The study followed 394 participants for 12 months. The overall discontinuation rate at 12 months was 39.3% (95% confidence interval [CI] 34.4–44.3), with paliperidone LAI being the least discontinued LAI (33.9%; 95% CI 25.3–43.5) and olanzapine LAI the most discontinued (62.5%; 95% CI 35.4–84.8). The most frequent reason for discontinuation was onset of adverse events (32.9%; 95% CI 25.6–40.9) followed by participant refusal of the medication (20.6%; 95% CI 14.6–27.9). Medication adherence at baseline was negatively associated with discontinuation risk (hazard ratio [HR] 0.853; 95% CI 0.742–0.981; p = 0.026), whereas being prescribed olanzapine LAI was associated with increased discontinuation risk compared with being prescribed paliperidone LAI (HR 2.156; 95% CI 1.003–4.634; p = 0.049). Conclusions Clinicians should be aware that LAI discontinuation is a frequent occurrence. LAI choice should be carefully discussed with the patient, taking into account individual characteristics and possible obstacles related to the practicalities of each formulation. Supplementary Information The online version contains supplementary material available at 10.1007/s40263-021-00809-w.

Published
2021

20. Van Allen Probes Observations of Magnetic Field Dipolarization and Its Associated O+ Flux Variations in the Inner Magnetosphere at L 6.6

Author

Nose, M, Keika, K, Kletzing, C. A, Spence, H. E, Smith, C. W, MacDowall, R. J, Reeves, G. D, Larsen, B. A, and Mitchell, D. G

Subjects
Space Sciences (General)
Abstract

We investigate the magnetic field dipolarization in the inner magnetosphere and its associated ion flux variations, using the magnetic field and energetic ion flux data acquired by the Van Allen Probes. From a study of 74 events that appeared at L= 4.5-6.6 between 1 October 2012 and 31 October 2013, we reveal the following characteristics of the dipolarization in the inner magnetosphere: (1) its time scale is approximately 5 min; (2) it is accompanied by strong magnetic fluctuations that have a dominant frequency close to the O+ gyrofrequency; (3) ion fluxes at 20-50 keV are simultaneously enhanced with larger magnitudes for O+ than for H+; (4) after a few minutes of the dipolarization, the flux enhancement at 0.1-5 keV appears with a clear energy-dispersion signature only for O+; and (5) the energy-dispersed O+ flux enhancement appears in directions parallel or antiparallel to the magnetic field. From these characteristics, we discuss possible mechanisms that can provide selective acceleration to O+ ions at > 20 keV. We conclude that O+ ions at L= 5.4-6.6 undergo nonadiabatic local acceleration caused by oscillating electric field associated with the magnetic fluctuations and/or adiabatic convective transport from the plasma sheet to the inner magnetosphere by the impulsive electric field. At L= 4.5-5.4, however, only the former acceleration is plausible. We also conclude that the field-aligned energy-dispersed O+ ions at 0.1-5 keV originate from the ionosphere and are extracted nearly simultaneously to the onset of the dipolarization.

Published
2016
Full Text
View/download PDF

23. Erratum: Safety of psychotropic medications in people with COVID-19: Evidence review and practical recommendations (BMC Medicine (2020) 18 (215) DOI: 10.1186/s12916-020-01685-9)

Author

Ostuzzi, G., Papola, D., Gastaldon, C., Schoretsanitis, G., Bertolini, F., Amaddeo, F., Cuomo, A., Emsley, R., Fagiolini, A., Imperadore, G., Kishimoto, T., Michencigh, G., Nose, M., Purgato, M., Dursun, S., Stubbs, B., Taylor, D., Thornicroft, G., Ward, P. B., Hiemke, C., Correll, C. U., and Barbui, C.

Published
2020

31. Energetic O+ and H+ Ions in the Plasma Sheet: Implications for the Transport of Ionospheric Ions

Author

Ohtani, S, Nose, M, Christon, S. P, and Lui, A. T

Subjects
Geophysics
Abstract

The present study statistically examines the characteristics of energetic ions in the plasma sheet using the Geotail/Energetic Particle and Ion Composition data. An emphasis is placed on the O+ ions, and the characteristics of the H+ ions are used as references. The following is a summary of the results. (1) The average O+ energy is lower during solar maximum and higher during solar minimum. A similar tendency is also found for the average H+ energy, but only for geomagnetically active times; (2) The O+ -to -H+ ratios of number and energy densities are several times higher during solar maximum than during solar minimum; (3) The average H+ and O+ energies and the O+ -to -H+ ratios of number and energy densities all increase with geomagnetic activity. The differences among different solar phases not only persist but also increase with increasing geomagnetic activity; (4) Whereas the average H+ energy increases toward Earth, the average O+ energy decreases toward Earth. The average energy increases toward dusk for both the H+ and O+ ions; (5) The O+ -to -H+ ratios of number and energy densities increase toward Earth during all solar phases, but most clearly during solar maximum. These results suggest that the solar illumination enhances the ionospheric outflow more effectively with increasing geomagnetic activity and that a significant portion of the O+ ions is transported directly from the ionosphere to the near ]Earth region rather than through the distant tail.

Published
2011
Full Text
View/download PDF

38. Molecular-beam epitaxial growth and characterization of Bi-Sr-Co-O thin films

Author

Tsukada, I., Nose, M., and Uchinokura, K.

Subjects
Epitaxy -- Research, Thin films -- Research, High temperature superconductors -- Research, Physics
Abstract

The thin-film growth of Co oxides and layered Bi-Sr-Co-O compounds were studied in detail under an ozone ambient. All samples were produced by a molecular-beam-epitaxy machine modified for the growth of Bi-based high-temperature superconductors. Findings revealed that the Co-232 films had resistivities on the order of 1 milliohm-cm. and that the carriers are holes, similar to those of Bi(sub 2)Sr(sub 2)Ca(sub n-1)Cu(sub n)O(sub 2n+4+delta) superconductors.

Published
1996

39. First record of chambered hexactinellid sponges from the Palaeozoic

Author

Nose, M. and Nose, M.

Abstract

Most chambered sponges (the polyphyletic group of "Sphinctozoa") are hypercalcified types and most of them probably belong to the Demospongia. "Spinctozoa" occur from the Cambrian to the Recent and are the most abundant sponges in Late Palaeozoic and Triassic reefs and shallow water limestones. Among hexactinellid sponges, chambered forms are very rare including taxa only from the Late Jurassic and the Late Triassic of Europe, Russia, Tadjikistan, Iran or China. There are five genera described Casearia Quenstedt, Caucasocoelia Boiko, Dracolychnos Wu & Xiao, Pseudo-verticillites Boiko and Innaecoelia Boiko, the latter of which is synomised with Casearia by most authors.

Published
2019

48. NEW RECORD OF HALIMEDACEAN ALGAE FROM THE UPPER TRIASSIC OF THE SOUTHERN ALPS (DOLOMITES, ITALY)

Author

Nose, M., Schlagintweit, F., and Alexander Nützel

Subjects
010504 meteorology & atmospheric sciences, halimedaceans, Dolomites, lcsh:QE1-996.5, green algae, Heiligkreuz Formation, Late Triassic, 010502 geochemistry & geophysics, 01 natural sciences, lcsh:Geology, lcsh:Paleontology, lcsh:QE701-760, 0105 earth and related environmental sciences
Abstract

A new record of halimedacean algae is reported from the Upper Triassic (Carnian) of the Dolomites (Southern Alps) near Cortina d’Ampezzo. Based on the gross morphology (non-segmented non-branched thalli) and the internal skeletal arrangement (e.g., medulla with thicker siphons, sometimes bifurcating at high angles; cortex with thinner siphons with multiple Y-like branching), the material can be assigned to the genus Boueina. It is the first record of halimedacean algae from the Upper Triassic of the Southern Alps (Dolomites) and the highly diverse San Cassiano Formation sensu lato (Heiligkreuz Formation). Although the fossilization potential of these algae was low, it is likely that they were much more common than suggested by this sparse fossil record and that they contributed considerably to carbonate production in early Mesozoic times., Rivista Italiana di Paleontologia e Stratigrafia (Research In Paleontology and Stratigraphy), V. 124, N. 3 (2018)

Published
2018
Full Text
View/download PDF

49. Microscopic observations of pulsating aurora associated with chorus element structures:coordinated arase satellite‐PWING observations

Author

Ozaki, M. (M.), Shiokawa, K. (K.), Miyoshi, Y. (Y.), Hosokawa, K. (K.), Oyama, S. (S.), Yagitani, S. (S.), Kasahara, Y. (Y.), Kasaba, Y. (Y.), Matsuda, S. (S.), Kataoka, R. (R.), Ebihara, Y. (Y.), Ogawa, Y. (Y.), Otsuka, Y. (Y.), Kurita, S. (S.), Moore, R. C. (R. C.), Tanaka, Y. -. (Y. -M.), Nose, M. (M.), Nagatsuma, T. (T.), Connors, M. (M.), Nishitani, N. (N.), Katoh, Y. (Y.), Hikishima, M. (M.), Kumamoto, A. (A.), Tsuchiya, F. (F.), Kadokura, A. (A.), Nishiyama, T. (T.), Inoue, T. (T.), Imamura, K. (K.), Matsuoka, A. (A.), and Shinohara, I. (I.)

Subjects
Physics::Space Physics, Physics::Geophysics
Abstract

Rapid (

Published
2018

50. The Appearance of In vivo ANA Positivity after a Period of 17 years in a Patient with Lupus Nephritis who had Received both Methylprednisolone and Cyclophosphamide Pulse Therapy

Author

Yan K, Sumiishi A, Matsubara S, Sano K, Kudo A, K Fukuoka, Arimura Y, Nose M, and Nakabayashi K

Subjects
Pathology, medicine.medical_specialty, biology, medicine.diagnostic_test, Cyclophosphamide, business.industry, Lupus nephritis, Autopsy, medicine.disease, Methylprednisolone, In vivo, Biopsy, medicine, biology.protein, Immunohistochemistry, Antibody, business, medicine.drug
Abstract

In vivo anti-nuclear antibody positive phenomenon in the renal tissues except for necropsy/autopsy cases or very severe cases of systemic lupus erythematosus is a controversial issue until today. However, we experienced a case of lupus nephritis that showed in vivo anti-nuclear antibody-positive cells in the renal tissues. Four successive renal biopsies over 17 years were studied with immunofluorescence as well as immunohistochemical and immuneelectron microscopic staining. The first, second and third biopsies did not reveal any in vivo anti-nuclear antibodypositive cells. However, the fourth biopsy in relapse showed positive cells, and the transfer of the patient’s serum into the mice provoked in vivo anti-nuclear antibody-positive cells in the mouse intestines. We present this case in detail and discuss the implications of these observations.

Published
2018

Catalog

Books, media, physical & digital resources
See catalog results