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5,172 results on '"Sugiyama, K."'

1. Busin Glide-Assisted Pull-Through Insertion of Artificial Corneal Endothelium (EndoArt)

Author

Kobayashi A, Hayashi T, Igarashi A, Shimizu T, Yokogawa H, Yuda K, Bachmann B, Yamagami S, and Sugiyama K

Subjects
endothelial keratoplasty, artificial corneal endothelium, endoart, bullous keratopathy, descemet’s membrane endothelial keratoplasty, Medicine (General), R5-920
Abstract

Akira Kobayashi,1 Takahiko Hayashi,2 Ami Igarashi,2 Toshiki Shimizu,2 Hideaki Yokogawa,1 Kentaro Yuda,3 Björn Bachmann,4 Satoru Yamagami,2 Kazuhisa Sugiyama1 1Department of Ophthalmology, Kanazawa University Hospital, Ishikawa, Japan; 2Department of Ophthalmology and Department of Visual Sciences, Nihon University School of Medicine, Itabashi, Tokyo, Japan; 3Kikuna Yuda Eye Clinic, Yokohama, Japan; 4Department of Ophthalmology, University of Cologne, Faculty of Medicine and University Hospital Cologne, Cologne, GermanyCorrespondence: Akira Kobayashi, Department of Ophthalmology, Kanazawa University Graduate School of Medical Science, Takara-machi 13-1, Kanazawa, Ishikawa-ken, 920-8641, Japan, Tel +81-76-265-2403, Fax +81-76-222-9660, Email eyekoba@gmail.comBackground: Currently, the push-in technique through the corneal tunnel using a blunt-tip spatula is used to insert an artificial corneal endothelium (EndoArt) into the anterior chamber (AC). The device is useful for patients with bullous keratopathy; however, it may be difficult to manipulate the very thin implant through hazy cornea. Unlike DMEK graft, it cannot be stained and the F-mark is faint. So, visualizing and orienting the implant is a real challenge especially through a hazy cornea and inadequate AC visualization. Therefore, alternative EndoArt implantation techniques are needed in patients with advanced endothelial dysfunction to avoid complications.Purpose: To report an alternative technique for EndoArt implantation using a Busin glide.Technique: The EndoArt was loaded onto the Busin glide with the concave side of the EndoArt facing upward and was then pulled/pushed into the Busin glide opening. After the Descemet’s membrane and endothelium were detached and removed in a circular fashion in a patient with advanced corneal endothelial decompensation, the Busin glide was inserted into the corneal incision, and the EndoArt was slowly pulled into the AC using retractor forceps. Finally, the air was injected into the AC.Conclusion: The Busin glide-assisted pull-through technique smoothly and securely inserted the EndoArt into the AC without upside-down attachment. This alternative technique can be useful for patients with a history of repeat intraocular surgeries or trauma with severe corneal edema to avoid potential complications such as epithelial implantation cysts or downgrowth.Keywords: endothelial keratoplasty, artificial corneal endothelium, EndoArt, bullous keratopathy, Descemet’s membrane endothelial keratoplasty

Published
2024

2. A Keplerian disk with a four-arm spiral birthing an episodically accreting high-mass protostar

Author

Burns, R. A., Uno, Y., Sakai, N., Blanchard, J., Rosli, Z., Orosz, G., Yonekura, Y., Tanabe, Y., Sugiyama, K., Hirota, T., Kim, Kee-Tae, Aberfelds, A., Volvach, A. E., Bartkiewicz, A., Garatti, A. Caratti o, Sobolev, A. M., Stecklum, B., Brogan, C., Phillips, C., Ladeyschikov, D. A., Johnstone, D., Surcis, G., MacLeod, G. C., Linz, H., Chibueze, J. O., Brand, J., Eislöffel, J., Hyland, L., Uscanga, L., Olech, M., Durjasz, M., Bayandina, O., Breen, S., Ellingsen, S. P., Heever, S. P. van den, Hunter, T. R., and Chen, X.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

High-mass protostars (M$_{\star} >$ 8 M$_{\odot}$) are thought to gain the majority of their mass via short, intense bursts of growth. This episodic accretion is thought to be facilitated by gravitationally unstable and subsequently inhomogeneous accretion disks. Limitations of observational capabilities, paired with a lack of observed accretion burst events has withheld affirmative confirmation of the association between disk accretion, instability and the accretion burst phenomenon in high-mass protostars. Following its 2019 accretion burst, a heat-wave driven by a burst of radiation propagated outward from the high-mass protostar G358.93-0.03-MM1. Six VLBI (very long baseline interferometry) observations of the raditively pumped 6.7 GHz methanol maser were conducted during this period, tracing ever increasing disk radii as the heat-wave propagated outward. Concatenating the VLBI maps provided a sparsely sampled, milliarcsecond view of the spatio-kinematics of the accretion disk covering a physical range of $\sim$ 50 - 900 AU. We term this observational approach `heat-wave mapping'. We report the discovery of a Keplerian accretion disk with a spatially resolved four-arm spiral pattern around G358.93-0.03-MM1. This result positively implicates disk accretion and spiral arm instabilities into the episodic accretion high-mass star formation paradigm., Comment: Published in Nature Astronomy in 2023

Published
2023
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3. A heat-wave of accretion energy traced by masers in the G358-MM1 high-mass protostar

Author

Burns, R. A., Sugiyama, K., Hirota, T., Kim, Kee-Tae, Sobolev, A. M., Stecklum, B., MacLeod, G. C., Yonekura, Y., Olech, M., Orosz, G., Ellingsen, S. P., Hyland, L., Garatti, A. Caratti o, Brogan, C., Hunter, T. R., Phillips, C., Heever, S. P. van den, Eislöffel, J., Linz, H., Surcis, G., Chibueze, J. O., Baan, W., and Kramer, B.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

High-mass stars are thought to accumulate much of their mass via short, infrequent bursts of disk-aided accretion. Such accretion events are rare and difficult to observe directly but are known to drive enhanced maser emission. In this Letter we report high-resolution, multi-epoch methanol maser observations toward G358.93-0.03 which reveal an interesting phenomenon; the sub-luminal propagation of a thermal radiation "heat-wave" emanating from an accreting high-mass proto-star. The extreme transformation of the maser emission implies a sudden intensification of thermal infrared radiation from within the inner (40 mas, 270 au) region. Subsequently, methanol masers trace the radial passage of thermal radiation through the environment at $\geq$ 4-8\% the speed of light. Such a high translocation rate contrasts with the $\leq$ 10 km s$^{-1}$ physical gas motions of methanol masers typically observed using very long baseline interferometry (VLBI). The observed scenario can readily be attributed to an accretion event in the high-mass proto-star G358.93-0.03-MM1. While being the third case in its class, G358.93-0.03-MM1 exhibits unique attributes hinting at a possible `zoo' of accretion burst types. These results promote the advantages of maser observations in understanding high-mass star formation, both through single-dish maser monitoring campaigns and via their international cooperation as VLBI arrays., Comment: Published in Nature Astronomy in 2020

Published
2023
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4. Ammonia masers toward G358.931-0.030

Author

McCarthy, T. P., Breen, S. L., Kaczmarek, J. F., Chen, X., Parfenov, S., Sobolev, A. M., Ellingsen, S. P., Burns, R. A., MacLeod, G. C., Sugiyama, K., Brierley, A. L., and Heever, S. P. van den

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We report the detection of ammonia masers in the non-metastable (6, 3), (7, 5) and (6, 5) transitions, the latter is the first unambiguous maser detection of that transition ever made. Our observations include the first VLBI detection of ammonia maser emission, which allowed effective constrain of the (6, 5) maser brightness temperature. The masers were detected towards G358.931-0.030, a site of 6.7-GHz class~II methanol maser emission that was recently reported to be undergoing a period of flaring activity. These ammonia masers appear to be flaring contemporaneously with the class~II methanol masers during the accretion burst event of G358.931-0.030. This newly detected site of ammonia maser emission is only the twelfth such site discovered in the Milky Way. We also report the results of an investigation into the maser pumping conditions, for all three detected masing transitions, through radiative transfer calculations constrained by our observational data. These calculations support the hypothesis that the ammonia (6, 5) maser transition is excited through high colour temperature infrared emission, with the (6, 5) and (7, 5) transition line-ratio implying dust temperatures >400K. Additionally, we detect significant linearly polarised emission from the ammonia (6, 3) maser line. Alongside our observational and radiative transfer calculation results, we also report newly derived rest frequencies for the ammonia (6, 3) and (6, 5) transitions., Comment: Accepted into MNRAS 2023 April 24. 13 pages, 5 figures, 3 tables

Published
2023
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5. Safety of Tocilizumab on Rheumatoid Arthritis in Patients with Interstitial Lung Disease

Author

Otsuji N, Sugiyama K, Owada T, Arifuku H, Koyama K, Hirata H, and Fukushima Y

Subjects
interstitial lung disease, krebs von den lungen-6, kl-6, matrix metalloproteinase-3, mmp-3, rheumatoid arthritis, mortality, tocilizumab, Diseases of the musculoskeletal system, RC925-935
Abstract

Naotatsu Otsuji,1 Kumiya Sugiyama,1,2 Takayoshi Owada,1 Hajime Arifuku,1 Kenya Koyama,1 Hirokuni Hirata,1 Yasutsugu Fukushima1 1Department of Respiratory Medicine and Clinical Immunology, Dokkyo Medical University Saitama Medical Center, Koshigaya, Saitama, Japan; 2National Hospital Organization Utsunomiya Hospital, Utsunomiya, Tochigi, JapanCorrespondence: Kumiya Sugiyama, National Hospital Organization Utsunomiya Hospital, 2160, Shimo-Okamoto, Utsunomiya, Tochigi, 329-1193, Japan, Email sugiyama@dokkyomed.ac.jpPurpose: The prognosis of rheumatoid arthritis (RA) with interstitial lung disease (ILD) is particularly poor. Although drugs that do not contribute to the progression of ILD should be used in RA treatment, none have been established. This study evaluated the safety of tocilizumab in terms of ILD activity.Patients and Methods: This study prospectively enrolled all 55 patients with RA complicated by ILD who were treated with tocilizumab at Dokkyo Medical University Saitama Medical Center from April 2014 to June 2022. The outcome measures were MMP-3 and KL-6 as biomarkers of RA and ILD activity, respectively, and the relationship between them was analyzed.Results: Both MMP-3 and KL-6 were significantly improved at 6 months of treatment (P < 0.001 and P < 0.05, respectively), and a weak correlation between MMP-3 and KL-6 was observed (R2 = 0.086, P = 0.087). The group with increased MMP-3 due to RA progression had significantly higher KL-6 at 6 months compared with the group with RA improvement (P < 0.05). Also, the group with ILD progression on computed tomography had significantly higher MMP-3 compared with the groups with improvement or no change of ILD (P < 0.05 and P < 0.01, respectively). The mortality rate was 0% at 6 months, 2.0% at 1 year, 16.7% at 2 years, and 32.4% at 3 years, and mortality from acute exacerbation of ILD due to respiratory infection increased over time.Conclusion: RA activity and ILD activity were found to be related at 6 months of treatment. Tocilizumab does not seem to affect the mechanism of ILD progression, as most patients showed improvement in both MMP-3 and KL-6 with tocilizumab within 6 months, when this drug would be expected to affect the lungs directly. However, respiratory infection exacerbated ILD from 1 year after the start of treatment. As immunosuppressive drugs, including tocilizumab, have a risk of respiratory infection, it is important to identify early signs of infection.Keywords: interstitial lung disease, Krebs von den Lungen-6, KL-6, matrix metalloproteinase-3, MMP-3, rheumatoid arthritis, mortality, tocilizumab

Published
2024

11. High-power laser experiment on developing supercritical shock propagating in homogeneously magnetized plasma of ambient gas origin

Author

Matsukiyo, S., Yamazaki, R., Morita, T., Tomita, K., Kuramitsu, Y., Tanaka, S. J., Takezaki, T., Isayama, S., Higuchi, T., Murakami, H., Horie, Y., Katsuki, N., Hatsuyama, R., Edamoto, M., Nishioka, H., Takagi, M., Kojima, T., Tomita, S., Ishizaka, N., Kakuchi, S., Sei, S., Sugiyama, K., Aihara, K., Kambayashi, S., Ota, M., Egashira, S., Izumi, T., Minami, T., Nakagawa, Y., Sakai, K., Iwamoto, M., Ozaki, N., and Sakawa, Y.

Subjects
Physics - Plasma Physics, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract

A developing supercritical collisionless shock propagating in a homogeneously magnetized plasma of ambient gas origin having higher uniformity than the previous experiments is formed by using high-power laser experiment. The ambient plasma is not contaminated by the plasma produced in the early time after the laser shot. While the observed developing shock does not have stationary downstream structure, it possesses some characteristics of a magnetized supercritical shock, which are supported by a one-dimensional full particle-in-cell simulation taking the effect of finite time of laser-target interaction into account., Comment: 7 pages, 6 fitures

Published
2022
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12. The evolution of the H2O maser emission in the accretion burst source G358.93-0.03

Author

Bayandina, O. S., Brogan, C. L., Burns, R. A., Garatti, A. Caratti o, Chibueze, J. O., Heever, S. P. van den, Kurtz, S. E., MacLeod, G. C., Moscadelli, L., Sobolev, A. M., Sugiyama, K., Val'tts, I. E., and Yonekura, Y.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract

The massive young stellar object (MYSO) G358.93-0.03-MM1 showed an extraordinary near-infrared- to (sub-)millimetre-dark and far-infrared-loud accretion burst, which is closely associated with flares of several class II methanol maser transitions, and, later, a 22 GHz water maser flare. Water maser flares provide an invaluable insight into ejection events associated with accretion bursts. Although the short timescale of the 22 GHz water maser flare made it impossible to carry out a very long baseline interferometry observation, we could track it with the Karl G. Jansky Very Large Array (VLA). The evolution of the spatial structure of the 22 GHz water masers and their association with the continuum sources in the region is studied with the VLA during two epochs, pre- and post-H2O maser flare. A drastic change in the distribution of the water masers is revealed: in contrast to the four maser groups detected during epoch I, only two newly formed clusters are detected during epoch II. The 22 GHz water masers associated with the bursting source MM1 changed in morphology and emission velocity extent. Clear evidence of the influence of the accretion burst on the ejection from G358.93-0.03-MM1 is presented. The accretion event has also potentially affected a region with a radius of ~2'' (~13 500 AU at 6.75 kpc), suppressing water masers associated with other point sources in this region.

Published
2022
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16. A multi-transition methanol maser study of the accretion burst source G358.93-0.03-MM1

Author

Bayandina, O. S., Brogan, C. L., Burns, R. A., Chen, X., Hunter, T. R., Kurtz, S. E., MacLeod, G. C., Sobolev, A. M., Sugiyama, K., Val'tts, I. E., and Yonekura, Y.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract

We present the most complete to date interferometric study of the centimeter wavelength methanol masers detected in G358.93-0.03 at the burst and post-burst epochs. A unique, NIR/(sub)mm-dark and FIR-loud MYSO accretion burst was recently discovered in G358.93-0.03. The event was accompanied by flares of an unprecedented number of rare methanol maser transitions. The first images of three of the newly-discovered methanol masers at 6.18, 12.23, and 20.97 GHz are presented in this work. The spatial structure evolution of the methanol masers at 6.67, 12.18, and 23.12 GHz is studied at two epochs. The maser emission in all detected transitions resides in a region of $\sim$0.2$^{\prime\prime}$ around the bursting source and shows a clear velocity gradient in the north-south direction, with red-shifted features to the north and blue-shifted features to the south. A drastic change in the spatial morphology of the masing region is found: a dense and compact "spiral" cluster detected at epoch I evolved into a disperse, "round" structure at epoch II. During the transition from the first epoch to the second, the region traced by masers expanded. The comparison of our results with the complementary VLA, VLBI, SMA, and ALMA maser data is conducted. The obtained methanol maser data support the hypothesis of the presence of spiral-arm structures within the accretion disk, which was suggested in previous studies of the source.

Published
2022
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17. High-power laser experiment forming a supercritical collisionless shock in a magnetized uniform plasma at rest

Author

Yamazaki, Ryo, Matsukiyo, S., Morita, T., Tanaka, S. J., Umeda, T., Aihara, K., Edamoto, M., Egashira, S., Hatsuyama, R., Higuchi, T., Hihara, T., Horie, Y., Hoshino, M., Ishii, A., Ishizaka, N., Itadani, Y., Izumi, T., Kambayashi, S., Kakuchi, S., Katsuki, N., Kawamura, R., Kawamura, Y., Kisaka, S., Kojima, T., Konuma, A., Kumar, R., Minami, T., Miyata, I., Moritaka, T., Murakami, Y., Nagashima, K., Nakagawa, Y., Nishimoto, T., Nishioka, Y., Ohira, Y., Ohnishi, N., Ota, M., Ozaki, N., Sano, T., Sakai, K., Sei, S., Shiota, J., Shoji, Y., Sugiyama, K., Suzuki, D., Takagi, M., Toda, H., Tomita, S., Tomiya, S., Yoneda, H., Takezaki, T., Tomita, K., Kuramitsu, Y., and Sakawa, Y.

Subjects
Physics - Plasma Physics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We present a new experimental method to generate quasi-perpendicular supercritical magnetized collisionless shocks. In our experiment, ambient nitrogen (N) plasma is at rest and well-magnetized, and it has uniform mass density. The plasma is pushed by laser-driven ablation aluminum (Al) plasma. Streaked optical pyrometry and spatially resolved laser collective Thomson scattering clarify structures of plasma density and temperatures, which are compared with one-dimensional particle-in-cell simulations. It is indicated that just after the laser irradiation, the Al plasma is magnetized by a self-generated Biermann battery field, and the plasma slaps the incident N plasma. The compressed external field in the N plasma reflects N ions, leading to counter-streaming magnetized N flows. Namely we identify the edge of the reflected N ions. Such interacting plasmas form a magnetized collisionless shock., Comment: 17 pages, 12 figures, 1 table. Physical Review E, in press

Published
2022
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21. Cumulative incidence of vancomycin-resistant Enterococcus faecium detection by patient characteristics or possible exposures: prioritization of patients for active screening culture

Author

Furuya, K., Yamagishi, T., Suzuki, K., Sugiyama, K., Yamamoto, M., Koyama, M., Yamada, A., Sasaki, R., Kurioka, J., Kurai, H., Tanaka, K., Nakagawa, M., Kanazawa, Y., Onoda, S., Inoue, H., Koshiko, M., Kurosu, H., Shimada, T., Sunagawa, T., Sugai, M., and Hakamata, Y.

Published
2024
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28. Infrared observations of the flaring maser source G358.93-0.03 -- SOFIA confirms an accretion burst from a massive young stellar object

Author

Stecklum, B., Wolf, V., Linz, H., Garatti, A. Caratti o, Schmidl, S., Klose, S., Eislöffel, J., Fischer, Ch., Brogan, C., Burns, R., Bayandina, O., Cyganowski, C., Gurwell, M., Hunter, T., Hirano, N., Kim, K. -T., MacLeod, G., Menten, K. M., Olech, M., Orosz, G., Sobolev, A., Sridharan, T. K., Surcis, G., Sugiyama, K., van der Walt, J., Volvach, A., and Yonekura, Y.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

Class II methanol masers are signs of massive young stellar objects (MYSOs). Recent findings show that MYSO accretion bursts cause flares of these masers. Thus, maser monitoring can be used to identify such bursts. Burst-induced SED changes provide valuable information on a very intense phase of high-mass star formation. In mid-January 2019, a maser flare of the MYSO G358.93-0.03 was reported. ALMA and SMA imaging resolved the core of the star forming region and proved the association of the masers with the brightest continuum source MM1. However, no significant flux rise of the (sub)mm dust continuum was found. Thus, we performed NIR imaging with GROND and IFU spectroscopy with FIFI-LS aboard SOFIA to detect possible counterparts to the (sub)mm sources, and compare their photometry to archival measurements. The comparison of pre-burst and burst SEDs is of crucial importance to judge whether a luminosity increase due to the burst is present and if it triggered the maser flare. The FIR fluxes of MM1 measured with FIFI-LS exceed those from Herschel significantly, which clearly confirms the presence of an accretion burst. The second epoch data, taken about 16 months later, still show increased fluxes. Our RT modeling yielded major burst parameters and suggests that the MYSO features a circumstellar disk which might be transient. From the multi-epoch SEDs, conclusions on heating and cooling time-scales could be drawn. Circumstances of the burst-induced maser relocation have been explored. The verification of the accretion burst from G358 is another confirmation that Class II methanol maser flares represent an alert for such events. The few events known to date already indicate that there is a broad range in burst strength and duration as well as environmental characteristics. The G358 event is the shortest and least luminous MYSO accretion burst so far., Comment: 22 pages, 11 figures, accepted by A&A. Abstract abridged for arxiv submission

Published
2021
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29. VLBI observations of the G25.65+1.05 water maser superburst

Author

Burns, R. A., Orosz, G., Bayandina, O., Surcis, G., Olech, M., MacLeod, G., Volvach, A., Rudnitskii, G., Hirota, T., Immer, K., Blanchard, J., Marcote, B., van Langevelde, H. J., Chibueze, J. O., Sugiyama, K., Kim, Kee-Tae, Val`tts, I., Shakhvorostova, N., Kramer, B., Baan, W. A., Brogan, C., Hunter, T., Kurtz, S., Sobolev, A. M., Brand, J., and Volvach, L.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

This paper reports observations of a 22 GHz water maser `superburst' in the G25.65+1.05 massive star forming region, conducted in response to an alert from the Maser Monitoring Organisation (M2O). Very long baseline interferometry (VLBI) observations using the European VLBI Network (EVN) recorded a maser flux density of $1.2 \times 10^{4}$ Jy. The superburst was investigated in the spectral, structural and temporal domains and its cause was determined to be an increase in maser path length generated by the superposition of multiple maser emitting regions aligning in the line of sight to the observer. This conclusion was based on the location of the bursting maser in the context of the star forming region, its complex structure, and its rapid onset and decay.

Published
2019
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30. Detection of new methanol maser transitions associated with G358.93-0.03

Author

MacLeod, G. C., Sugiyama, K., Hunter, T. R., Quick, J., Baan, W., Breen, S. L., Brogan, C. L., Burns, R. A., Garatti, A. Caratti o, Chen, X., Chibueze, J. O., Houde, M., Kaczmarek, J. F., Linz, H., Rajabi, F., Saito, Y., Schmidl, S., Sobolev, A. M., Stecklum, B., Heever, S. P. van den, and Yonekura, Y.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

We report the detection of new 12.178, 12.229, 20.347, and 23.121 GHz methanol masers in the massive star-forming region G358.93-0.03, which are flaring on similarly short timescales (days) as the 6.668 GHz methanol masers also associated with this source. The brightest 12.178 GHz channel increased by a factor of over 700 in just 50 d. The masers found in the 12.229 and 20.347 GHz methanol transitions are the first ever reported and this is only the fourth object to exhibit associated 23.121 GHz methanol masers. The 12.178 GHz methanol maser emission appears to have a higher flux density than that of the 6.668 GHz emission, which is unusual. No associated near-infrared flare counterpart was found, suggesting that the energy source of the flare is deeply embedded., Comment: 9 pages, 3 figures, 2 tables, Published in MNRAS

Published
2019
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31. Sub-arcsecond (sub)millimeter imaging of the massive protocluster G358.93-0.03: Discovery of 14 new methanol maser lines associated with a hot core

Author

Brogan, C. L., Hunter, T. R., Towner, A. P. M., McGuire, B. A., MacLeod, G. C., Gurwell, M. A., Cyganowski, C. J., Brand, J., Burns, R. A., Garatti, A. Caratti o, Chen, X., Chibueze, J. O., Hirano, N., Hirota, T., Kim, K. -T., Kramer, B. H., Linz, H., Menten, K. M., Remijan, A., Sanna, A., Sobolev, A. M., Sridharan, T. K., Stecklum, B., Sugiyama, K., Surcis, G., Van der Walt, J., Volvach, A. E., and Volvach, L. N.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

We present (sub)millimeter imaging at 0.5'' resolution of the massive star-forming region G358.93-0.03 acquired in multiple epochs at 2 and 3 months following the recent flaring of its 6.7 GHz methanol maser emission. Using SMA and ALMA, we have discovered 14 new Class II methanol maser lines ranging in frequency from 199 GHz to 361 GHz, which originate mostly from vt=1 torsionally-excited transitions and include one vt=2 transition. The latter detection provides the first observational evidence that Class II maser pumping involves levels in the vt=2 state. The masers are associated with the brightest continuum source (MM1), which hosts a line-rich hot core. The masers present a consistent curvilinear spatial velocity pattern that wraps around MM1, suggestive of a coherent physical structure 1200 au in extent. In contrast, the thermal lines exhibit a linear pattern that crosses MM1 but at progressive position angles that appear to be a function of either increasing temperature or decreasing optical depth. The maser spectral profiles evolved significantly over one month, and the intensities dropped by factors of 3.0 to 7.2, with the vt=2 line showing the largest change. A small area of maser emission from only the highest excitation lines closest to MM1 has disappeared. There are seven additional dust continuum sources in the protocluster, including another hot core (MM3). We do not find evidence for a significant change in (sub)millimeter continuum emission from any of the sources during the one month interval, and the total protocluster emission remains comparable to prior single dish measurements., Comment: 10 pages, 2 figures, 3 tables, accepted for publication in The Astrophysical Journal Letters. All maser transitions detected in this object can be displayed via an option on the advanced interface of http://splatalogue.net

Published
2019
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33. Equatorial jet in the lower to middle cloud layer of Venus revealed by Akatsuki

Author

Horinouchi, T., Murakami, S., Satoh, T., Peralta, J., Ogohara, K., Kouyama, T., Imamura, T., Kashimura, H., Limaye, S. S., McGouldrick, K., Nakamura, M., Sato, T. M., Sugiyama, K., Takagi, M., Watanabe, S., Yamada, M., Yamazaki, A., and Young, E. F.

Subjects
Astrophysics - Earth and Planetary Astrophysics, Physics - Atmospheric and Oceanic Physics
Abstract

The Venusian atmosphere is in a state of superrotation where prevailing westward winds move much faster than the planet's rotation. Venus is covered with thick clouds that extend from about 45 to 70 km altitude, but thermal radiation emitted from the lower atmosphere and the surface on the planet's nightside escapes to space at narrow spectral windows of the near-infrared. The radiation can be used to estimate winds by tracking the silhouettes of clouds in the lower and middle cloud regions below about 57 km in altitude. Estimates of wind speeds have ranged from 50 to 70 m/s at low to mid-latitudes, either nearly constant across latitudes or with winds peaking at mid-latitudes. Here we report the detection of winds at low latitude exceeding 80 m/s using IR2 camera images from the Akatsuki orbiter taken during July and August 2016. The angular speed around the planetary rotation axis peaks near the equator, which we suggest is consistent with an equatorial jet, a feature that has not been observed previously in the Venusian atmosphere. The mechanism producing the jet remains unclear. Our observations reveal variability in the zonal flow in the lower and middle cloud region that may provide clues to the dynamics of Venus's atmospheric superrotation., Comment: 23 pages, 4 figures

Published
2017
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34. Fcc-Based Superstructure in CrCoNi System Induced by Annealing of Amorphous Cr-Co-Ni-Si-B-P Alloy.

Author

Kawamata, T., Ban, T., Shibata, M., Murayama, H., Yasuhara, A., Yubuta, K., and Sugiyama, K.

Subjects
SCANNING transmission electron microscopy, ENERGY dispersive X-ray spectroscopy, FACE centered cubic structure, SYNCHROTRON radiation, X-ray scattering
Abstract

Chemically ordered face-centered cubic (fcc) phases consisting mainly of Cr, Co, and Ni were synthesized by annealing a Cr26.7Co26.7Ni26.7Si10B5P5 amorphous alloy. The annealed Cr26.7Co26.7Ni26.7Si10B5P5 sample was composed of Cr4.5BP2, Cr3 Co5Si2, and fcc phases. Synchrotron radiation anomalous X-ray scattering (AXS) measurements confirmed that the annealed Cr26.7Co26.7Ni26.7Si10B5P5 sample had superlattice reflections from an L10-, and/or L12-, and D022-type ordered structure. The diffraction intensities of the superlattice reflections observed in the AXS measurements indicated strong dependence on the incident X-ray energy. The diffraction intensity of the superlattice reflection increased at the X-ray energy near the K-edge of Cr, suggesting that Cr is mainly ordered in the L10- and D022-type structures. Microstructural analysis using scanning transmission electron microscopy (STEM) revealed crystal grains with diameters of approximately 20 nm, showing diffraction spots corresponding to superlattice reflections of 001 and 110, in addition to a two-dimensional diffraction pattern corresponding to the fcc structure. Simultaneous STEM--energy dispersive X-ray spectroscopy analysis indicated that the grains had a higher Cr concentration than the mother alloy composition of Cr26.7Co26.7Ni26.7Si10B5P5. [ABSTRACT FROM AUTHOR]

Published
2024
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38. Lattice Boltzmann Simulations of Droplet formation in confined Channels with Thermocapillary flows

Author

Gupta, A., Sbragaglia, M., Belardinelli, D., and Sugiyama, K.

Subjects
Physics - Fluid Dynamics, Condensed Matter - Statistical Mechanics, Nonlinear Sciences - Chaotic Dynamics
Abstract

Based on mesoscale lattice Boltzmann simulations with the "Shan-Chen" model, we explore the influence of thermocapillarity on the break-up properties of fluid threads in a microfluidic T-junction, where a dispersed phase is injected perpendicularly into a main channel containing a continuous phase, and the latter induces periodic break-up of droplets due to the cross-flowing. Temperature effects are investigated by switching on/off both positive/negative temperature gradients along the main channel direction, thus promoting a different thread dynamics with anticipated/delayed break-up. Numerical simulations are performed at changing the flow-rates of both the continuous and dispersed phases, as well as the relative importance of viscous forces, surface tension forces and thermocapillary stresses. The range of parameters is broad enough to characterize the effects of thermocapillarity on different mechanisms of break-up in the confined T-junction, including the so-called "squeezing" and "dripping" regimes, previously identified in the literature. Some simple scaling arguments are proposed to rationalize the observed behaviour, and to provide quantitative guidelines on how to predict the droplet size after break-up., Comment: 18 pages, 9 figures

Published
2016
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39. Author Correction: A Keplerian disk with a four-arm spiral birthing an episodically accreting high-mass protostar

Author

Burns, R. A., Uno, Y., Sakai, N., Blanchard, J., Rosli, Z., Orosz, G., Yonekura, Y., Tanabe, Y., Sugiyama, K., Hirota, T., Kim, Kee-Tae, Aberfelds, A., Volvach, A. E., Bartkiewicz, A., Caratti o Garatti, A., Sobolev, A. M., Stecklum, B., Brogan, C., Phillips, C., Ladeyschikov, D. A., Johnstone, D., Surcis, G., MacLeod, G. C., Linz, H., Chibueze, J. O., Brand, J., Eislöffel, J., Hyland, L., Uscanga, L., Olech, M., Durjasz, M., Bayandina, O., Breen, S., Ellingsen, S. P., van den Heever, S. P., Hunter, T. R., and Chen, X.

Published
2023
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42. Rotating and infalling motion around the high-mass young stellar object Cepheus A-HW2 observed with the methanol maser at 6.7 GHz

Author

Sugiyama, K., Fujisawa, K., Doi, A., Honma, M., Kobayashi, H., Murata, Y., Motogi, K., Niinuma, K., Ogawa, H., Wajima, K., Sawada-Satoh, S., and Ellingsen, S. P.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

We have measured the internal proper motions of the 6.7 GHz methanol masers associated with Cepheus A (Cep A) HW2 using Very Long Baseline Interferometery (VLBI) observations. We conducted three epochs of VLBI monitoring observations of the 6.7 GHz methanol masers in Cep A-HW2 with the Japanese VLBI Network (JVN) over the period between 2006-2008. In 2006, we were able to use phase-referencing to measure the absolute coordinates of the maser emission with an accuracy of a few milliarcseconds. We compared the maser distribution with other molecular line observations that trace the rotating disk. We measured the internal proper motions for 29 methanol maser spots, of which 19 were identified at all three epochs and the remaining ten at only two epochs. The magnitude of proper motions ranged from 0.2 to 7.4 km/s, with an average of 3.1 km/s. Although there are large uncertainties in the observed internal proper motions of the methanol maser spots in Cep A, they are well fitted by a disk that includes both rotation and infall velocity components. The derived rotation and infall velocities at the disk radius of 680 au are 0.5 +- 0.7 and 1.8 +- 0.7 km/s, respectively. Assuming that the modeled disk motion accurately represents the accretion disk around the Cep A-HW2 high-mass YSO, we estimated the mass infall rate to be 3 x 10^{-4} n_8 Msun/yr (n_8 is the gas volume density in units of 10^{8} cm^{-3}). The combination of the estimated mass infall rate and the magnitude of the fitted infall velocity suggests that Cep A-HW2 is at an evolutionary phase of active gas accretion from the disk onto the central high-mass YSO. The infall momentum rate is estimated to be 5 x 10^{-4} n_8 Msun/yr km/s, which is larger than the estimated stellar radiation pressure of the HW2 object, supporting the hypothesis that this object is in an active gas accretion phase., Comment: 16 pages, 6 figures, 5 tables, accepted for publication in Astronomy & Astrophysics

Published
2013
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43. iStent Trabecular Micro-Bypass Stent Implantation with Cataract Surgery in a Japanese Glaucoma Population

Author

Nitta K, Yamada Y, Morokado S, and Sugiyama K

Subjects
microinvasive glaucoma surgery (migs), istent, trabecular micro-bypass, japanese, normal-tension glaucoma, Ophthalmology, RE1-994
Abstract

Koji Nitta,1 Yutaro Yamada,1 Satomi Morokado,1 Kazuhisa Sugiyama2 1Department of Ophthalmology, Fukui-Ken Saiseikai Hospital, Fukui, Fukui Prefecture, Japan; 2Department of Ophthalmology, Kanazawa University, Kanazawa, Ishikawa Prefecture, JapanCorrespondence: Koji NittaFukui-Ken Saiseikai Hospital, Funabashi 7-1, Wadanaka-Cho, Fukui City, Fukui 918-8503, JapanTel +81 776 23 1111Email nitta.koji7001@fukui.saiseikai.or.jpIntroduction: This study assesses two-year efficacy and safety following implantation of a single trabecular micro-bypass stent (iStent®) with concomitant phacoemulsification cataract surgery in Japanese patients with open-angle glaucoma (OAG).Materials and Methods: This retrospective, consecutive case series included eyes that underwent iStent implantation with phacoemulsification and were followed for 24 months postoperative. Efficacy and safety measures included intraocular pressure (IOP), number of glaucoma medications, adverse events, secondary surgeries, visual fields, and endothelial cell counts.Results: Of 73 operated eyes, 53 eyes had 24 months of follow-up and are analyzed. Diagnoses included primary open-angle glaucoma (POAG, n=25), normal-tension glaucoma (NTG, n=16), and pseudoexfoliative glaucoma (PXG, n=12). At 24 months, mean IOP reduced by 18% to 13.6± 3.0 mmHg versus 16.5± 3.4 mmHg preoperatively (p< 0.0001), and mean medication number reduced by 81% to 0.37± 0.74 versus 1.96± 0.98 preoperatively (p< 0.0001). The percentage of medication-free eyes was 77% versus 0% preoperatively, and 81% of eyes had IOP ≤ 15 mmHg versus 42% preoperatively. Results were similarly favorable across glaucoma subtypes (POAG, NTG, PXG). Notably, mean IOP in NTG eyes decreased to 12.8± 1.4 mmHg from 14.4± 3.0 mmHg preoperatively (p=0.03), and medications decreased by 87% to 0.31± 0.70 versus 2.38± 0.72 preoperatively (p< 0.0001). At 24 months, 81% of NTG eyes were medication-free (versus 0% preoperatively); 2 NTG eyes (13%) were on ≥ 2 medications (versus 100% preoperatively). Throughout the follow-up, visual fields and endothelial cell counts remained stable; 1 eye (1.9%) underwent filtration surgery.Discussion: Favorable safety and significant IOP and mediation reductions were achieved through two years following iStent implantation with phacoemulsification in a Japanese population. These gains were achieved across all glaucoma subtypes (including POAG, NTG, PXG).Conclusion: This real-world study supports the viability of iStent implantation to treat Japanese patients with glaucoma and shows that the benefits extend to those with NTG or PXG in addition to POAG.Keywords: microinvasive glaucoma surgery, MIGS, iStent, trabecular micro-bypass, Japanese, normal-tension glaucoma

Published
2020

44. In vivo Imaging of Reis–Bücklers and Thiel–Behnke Corneal Dystrophies Using Anterior Segment Optical Coherence Tomography

Author

Nishino T, Kobayashi A, Mori N, Yokogawa H, and Sugiyama K

Subjects
reis-bücklers corneal dystrophy, thiel-behnke corneal dystrophy, anterior segment optical coherence tomography, genetic mutational analysis, human transforming growth factor beta-induced gene, tgfbi, Ophthalmology, RE1-994
Abstract

Tsubasa Nishino, Akira Kobayashi, Natsuko Mori, Hideaki Yokogawa, Kazuhisa Sugiyama Department of Ophthalmology, Kanazawa University Graduate School of Medical Science, Kanazawa, JapanCorrespondence: Akira KobayashiDepartment of Ophthalmology, Kanazawa University Graduate School of Medical Science, 13-1 Takara-Machi, Kanazawa-shi, Ishikawa-ken 920-8641, JapanTel +81-76-265-2403Fax +81-76-222-9660Email eyekoba@gmail.comPurpose: To investigate in vivo corneal changes of genetically confirmed Reis–Bücklers corneal dystrophy (RBCD) and Thiel–Behnke corneal dystrophy (TBCD) using anterior segment optical coherence tomography (AS-OCT).Design: A single-center, prospective, comparative case series.Methods: Seven patients from 3 pedigrees (3 males, 4 females) with RBCD [Arg124Leu (R124L) heterozygous missense mutation of human transforming growth factor beta-induced (TGFBI) gene] and 4 patients from 3 pedigrees (3 males, 1 female) with TBCD [Arg555Gln (R555Q) heterozygous missense mutation of TGFBI gene] were examined. Six patients with RBCD and three patients with TBCD exhibited recurrence after corneal surgery including penetrating keratoplasty, phototherapeutic keratectomy, and electrolysis. All patients were examined by slit-lamp biomicroscopy followed by AS-OCT. Selected AS-OCT images of the cornea were evaluated qualitatively for changes in shape and degree of light reflection of corneal deposits.Results: Slit-lamp biomicroscopy showed characteristic irregular gray opacities in Bowman’s layer in each dystrophy: a geographic pattern in RBCD and a honeycomb pattern in TBCD. In each dystrophy, distinct characteristic deposits were observed by AS-OCT as a banding lesion in Bowman’s layer and its adjacent epithelium/stroma. In RBCD, the banding lesion was highly reflective and sharply margined at the stroma. In contrast, deposits in TBCD in the same layer showed a saw-tooth pattern toward the epithelium and poorly margined at the stroma.Conclusion: AS-OCT is able to clearly identify characteristic in vivo corneal microstructural changes associated with RBCD and TBCD. As a result, in vivo differentiation of RBCD and TBCD can be achieved.Keywords: Reis–Bücklers corneal dystrophy, Thiel–Behnke corneal dystrophy, anterior segment optical coherence tomography, genetic mutational analysis, human transforming growth factor beta-induced gene, TGFBI

Published
2020

45. Visibility of the Retina Through an Air-Filled Anterior Chamber During Simultaneous Vitrectomy and Descemet’s Stripping Automated Endothelial Keratoplasty

Author

Yokogawa H, Kobayashi A, Mori N, Nishino T, and Sugiyama K

Subjects
descemet’s stripping automated endothelial keratoplasty, pars plana vitrectomy, Ophthalmology, RE1-994
Abstract

Hideaki Yokogawa, Akira Kobayashi, Natsuko Mori, Tsubasa Nishino, Kazuhisa Sugiyama Department of Ophthalmology, Kanazawa University Graduate School of Medical Science, Kanazawa, JapanCorrespondence: Hideaki YokogawaDepartment of Ophthalmology, Kanazawa University Graduate School of Medical Science, 13-1 Takara-machi, Kanazawa-shi, Ishikawa-ken 920-8641, JapanTel +81-76-265-2403Fax +81-76-222-9660Email hyoko@med.kanazawa-u.ac.jpPurpose: To describe the visibility of the retina through an air-filled anterior chamber during simultaneous pars plana vitrectomy (PPV) and Descemet’s stripping automated endothelial keratoplasty (DSAEK), and to discuss the technical challenges of a fluid-air exchange under such conditions.Methods: Six eyes from 6 patients with coexisting bullous keratopathy and posterior segment problems such as vitreous opacity, retained silicon oil, intraocular lens subluxation, or aphakia underwent simultaneous PPV and DSAEK. In all cases, after completion of 25-gauge PPV with/without flanged intrascleral intraocular lens fixation, DSAEK donor tissue was inserted into the anterior chamber. Air was then injected into the anterior chamber to attach the donor graft to the back surface of the host cornea. At this point, the visibility of the retina was evaluated using endoillumination and a wide-angle viewing system.Results: In all cases, visibility of the retina through an air-filled anterior chamber, with the DSAEK donor attached, was sufficient to perform a fluid-air exchange.Conclusion: Our clinical observations of such rare but clinically important conditions indicate that simultaneous PPV and DSAEK is possible with fair visualization of the posterior segment including the retina.Keywords: Descemet’s stripping automated endothelial keratoplasty, pars plana vitrectomy

Published
2020

46. Predicting Lifetime Transition Risk of Severe Visual Field Defects Using Monte Carlo Simulation in Japanese Patients with Primary Open-Angle Glaucoma

Author

Nitta K, Tachibana G, Wajima R, Inoue S, Ohigashi T, Otsuka N, Kurashima H, Santo K, Hashimoto M, Shibahara H, Hirukawa M, and Sugiyama K

Subjects
glaucoma, epidemiology, prognosis, risk factors, simulation, Ophthalmology, RE1-994
Abstract

Koji Nitta,1,2 Gaku Tachibana,1,2 Ryotaro Wajima,1,2 Sachie Inoue,3 Tatsuya Ohigashi,4 Naomi Otsuka,4 Hiroaki Kurashima,4 Kazunori Santo,4 Masayo Hashimoto,4 Hidetoshi Shibahara,3 Mai Hirukawa,3 Kazuhisa Sugiyama2 1Department of Ophthalmology, Fukui-Ken Saiseikai Hospital, Fukui, Japan; 2Department of Ophthalmology, Kanazawa University Graduate School of Medical Science, Kanazawa, Japan; 3CRECON Medical Assessment Inc., Tokyo, Japan; 4Japan Medical Affairs Group, Santen Pharmaceutical Co., Ltd., Osaka, JapanCorrespondence: Koji Nitta Email nitta.koji7001@fukui.saiseikai.or.jpPurpose: To maintain visual fields and quality of life over a lifetime, medical practice must be conducted taking into consideration not only visual field progression but also future visual field changes that occur over the patients’ expected lifespan. The purpose of this study is to investigate the feasibility of establishing a model that predicts prognosis, estimating the proportion of glaucoma patients with severe visual field defects.Patients and Methods: The data of 191 patients with primary open-angle glaucoma, with a predominance of normal-tension glaucoma, were used for this study. The model was developed based on patients’ backgrounds and risk factors, using Monte Carlo simulation. A “severe visual field defect” was defined as ≤-20 dB. The mean deviation (MD) value for 10,000 virtual patients in each simulation pattern (144 patterns) was calculated using a predictive formula to estimate the MD slope, and the effects of risk factors and intraocular pressure (IOP) reduction on the proportion of patients with severe visual field defects were evaluated.Results: Younger age, later-stage disease, more severe glaucomatous structural abnormalities and the presence of disc hemorrhage were associated with an increase in the progression rate of patients with severe visual field defects. Conversely, lower IOP was associated with a decrease in this rate.Conclusion: Combining regression analysis with Monte Carlo simulation could be a useful method for developing predictive models of prognosis in glaucoma patients.Keywords: glaucoma, epidemiology, prognosis, risk factors, simulation

Published
2020

47. The Effect of Brimonidine 0.1% on Disc Hemorrhage in Primary Open-Angle Glaucoma Patients

Author

Nitta K, Shimamoto S, Wajima R, Tachibana G, Yamada Y, Domoto M, Takeda R, Takahashi Y, and Sugiyama K

Subjects
disc hemorrhage, intraocular pressure, brimonidine, primary open-angle glaucoma, normal-tension glaucoma, Ophthalmology, RE1-994
Abstract

Koji Nitta,1,2 Shiro Shimamoto,3 Ryotaro Wajima,2 Gaku Tachibana,2 Yutaro Yamada,1,2 Miyuki Domoto,1 Ryuji Takeda,4,5 Yoshinari Takahashi,6 Kazuhisa Sugiyama2 1Fukui-ken Saiseikai Hospital, Fukui, Japan; 2Department of Ophthalmology, Kanazawa University Graduate School of Medical Science, Kanazawa, Japan; 3Shimamoto Ophthalmology Clinic, Fukui, Japan; 4Department of Nutritional Sciences for Well-Being, Faculty of Health Sciences for Welfare, Kansai University of Welfare Sciences, Osaka, Japan; 5Department of Applied Biological Chemistry, Faculty of Agriculture, Kindai University, Nara, Japan; 6Inary Co., Ltd., Tokyo, JapanCorrespondence: Koji NittaDepartment of Ophthalmology, Fukui-ken Saiseikai Hospital, 7-1 Funabashi, Wadanaka-cho, Fukui 918-8503, JapanTel +81 776 23 1111Fax +81 776 28 8515Email nitta.koji7001@fukui.saiseikai.or.jpBackground: This retrospective study evaluated the effect of adjunctive administration of brimonidine 0.1% on disc hemorrhage (DH) in patients with primary open-angle glaucoma or normal-tension glaucoma who were already treated with other anti-glaucoma drugs.Methods: Patients with DH, before adjunctive therapy with brimonidine, were enrolled. Subjects were excluded if their treatment regimen was changed within 1 year after initiation of adjunctive therapy with brimonidine. We investigated the frequency of DH and intraocular pressure (IOP). Both parameters were compared before and after adjunctive administration of brimonidine.Results: The frequency of DH before and after brimonidine administration was 0.67± 0.68 and 0.31± 0.72 times/year, respectively, with a significant decrease (P=0.01), and the mean IOP before and after brimonidine administration was 12.5± 1.9 and 11.2± 2.2 mmHg, respectively, (P=0.0006) with a significant reduction after adjunctive administration.Conclusion: The results of this study supported the hypothesis that the frequency of DH is reduced by brimonidine alongside lowering of IOP.Keywords: disc hemorrhage, intraocular pressure, brimonidine, primary open-angle glaucoma, normal-tension glaucoma

Published
2020

49. Correction: Epidemiology and outcomes of early-onset AKI in COVID-19-related ARDS in comparison with non-COVID-19-related ARDS: insights from two prospective global cohort studies (Critical Care, (2023), 27, 1, (3), 10.1186/s13054-022-04294-5)

Author

McNicholas B. A., Mcnicholas, B, Rezoagli, E, Simpkin, A, Khanna, S, Suen, J, Yeung, P, Brodie, D, Bassi, G, Pham, T, Bellani, G, Fraser, J, Laffey, J, Al-Dabbous, T, Alfoudri, H, Shamsah, M, Alhadad, Q, Hanan, M, Elapavaluru, S, Berg, A, Horn, C, Abdelhalim, A, Amer, A, Elnaggar, C, Hassan, A, Abdelaziz, A, Abdelhalim, M, Orabi, Y, Alaraji, Z, Muhaisen, M, Almasri, L, Mustafa, D, Hamdan, S, Al-Saba'a, Y, Dalloul, Z, Alkahlout, M, Jaber, H, Aldabbourosama, O, Hussein, A, Emad, Z, Khaled, S, Mohamed, N, Hassanin, E, Hamdi, A, Ragab, A, Azizeldin, M, Mayasi, Y, Schroll, S, Meyer, D, Velazco, J, Ploskanych, L, Fikes, W, Bagewadi, R, Dao, M, White, H, Laviena, A, Ehlers, A, Shalabi-McGuire, M, Witt, T, Grazioli, L, Lorini, L, Grandin, E, Nunez, J, Reyes, T, O'Briain, D, Hunter, S, Ramanan, M, Affleck, J, Veerendra, H, Rai, S, Russell-Brown, J, Nourse, M, Joseph, M, Mitchell, B, Tenzer, M, Abe, R, Cho, H, Jeong, I, Rahman, N, Kakar, V, Sun, H, Hanley, A, Brozzi, N, Mehkri, O, Krishnan, S, Duggal, A, Houltham, S, Graf, J, Diaz, R, Orrego, R, Delgado, C, Gonzalez, J, Sanchez, M, Piagnerelli, M, Sarrazin, J, Zabert, G, Espinosa, L, Delgado, P, Delgado, V, Rincon, D, Yanten, A, Duque, M, Abouelmagd, K, Elhazmi, A, Al-Hudaib, A, Javidfar, J, Callahan, M, Dong, A, D'Orleans, C, Taufik, M, Wardoyo, E, Gunawan, M, Trisnaningrum, N, Irawany, V, Rayhan, M, Panigada, M, Pesenti, A, Zanella, A, Grasselli, G, Colombo, S, Martinet, C, Florio, G, Antonelli, M, Carelli, S, Grieco, D, Asaki, M, Hoshino, K, Salazar, L, Monsalve, M, Cosgrave, D, Atif, M, Qutishat, F, Laffey, C, Van Der Walt, M, Mccaffrey, J, Bone, A, Hakeem, Y, Winearls, J, Tallott, M, Thomson, D, Joubert, I, Arnold-Day, C, Piercy, J, van Zyl Smit, R, Miller, M, Seymour, L, van Heyningen, F, Teyangesikayi, G, Fredericks, D, Hssain, A, Aliudin, J, Alqahtani, A, Mohamed, K, Mohamed, A, Tan, D, Villanueva, J, Zaqout, A, Kurtzman, E, Ademi, A, Dobrita, A, El Aoudi, K, Segura, J, Giwangkancana, G, Ohshimo, S, Osatnik, J, Joosten, A, Torres, A, Yang, M, Motos, A, Luna, C, Arancibia, F, Williams, V, Noel, A, Luque, N, Fantini, M, Garcia, R, Alvarez, E, Greti, A, Ceccato, A, Sanchez, A, Vazquez, A, Roche-Campo, F, Franch-Llasat, D, Tuazon, D, Amato, M, Cassimiro, L, Pola, F, Ribeiro, F, Fonseca, G, Dalton, H, Desai, M, Osborn, E, Deeb, H, Arcadipane, A, Martucci, G, Panarello, G, Vitiello, S, Bianco, C, Occhipinti, G, Rossetti, M, Cuffaro, R, Cho, S, Whitman, G, El Sayed, M, Mokhtar, W, El-Shenawy, E, Shimizu, H, Moriyama, N, Kim, J, Kitamura, N, Gebauer, J, Yokoyama, T, Al-Fares, A, Buabbas, S, Alamad, E, Alawadhi, F, Alawadi, K, Khalefa, M, Al Ajeel, N, Aly, M, Al-Saleh, A, Naanouh, A, Elshourbgy, A, Gad, M, Elrazaz, R, Khadadah, I, Almumin, A, Altarakma, H, Albannay, H, Alsaleh, M, Radwan, M, Saadallah, I, Tanaka, H, Hashimoto, S, Yamazaki, M, Oh, T, Epler, M, Forney, C, Kruse, L, Feister, J, Williamson, J, Grobengieser, K, Gnall, E, Golden, S, Caroline, M, Shapiro, T, Karaj, C, Thome, L, Sher, L, Vanderland, M, Welch, M, Mcdermott, S, Brain, M, Mineall, S, Unwin, M, Chen, L, Trezise, T, Mckeon, L, Kimura, D, Brazzi, L, Sales, G, Montrucchio, G, Ogston, T, Nagpal, D, Fischer, K, Lorusso, R, van Bussell, B, De Piero, M, Mariani, S, Rangappa, R, Shetty, R, Rai, P, Ganesan, A, Esperatti, M, Fuentes, N, Gonzalez, M, Carton, E, Sen, A, Palacios, A, Rainey, D, Samoukoviv, G, Campisi, J, Durham, L, Neumann, E, Seefeldt, C, Falcucci, O, Emmrich, A, Guy, J, Johns, C, Potzner, K, Zimmermann, C, Espinal, A, Buchtele, N, Schwameis, M, Korhnfehl, A, Brock, R, Staudinger, T, Stecher, S, Barnikel, M, Anton, S, Pawlikowski, A, Zaaqoq, A, Galloway, L, Merley, C, Nichol, A, Csete, M, Quesada, L, Saba, I, Kasugai, D, Hiraiwa, H, Tanaka, T, Marwali, E, Purnama, Y, Dewayanti, S, Ardiyan, Juzar, D, Siagian, D, Chen, Y, Ogino, M, Nasa, P, Matthew, C, Majeed, N, Ratsep, I, Post, A, Sillaots, P, Krund, A, Lehiste, M, Lepik, T, Manetta, F, Mihelis, E, Sarmiento, I, Narasimhan, M, Varrone, M, Komats, M, Garcia-Diaz, J, Harmon, C, Satyapriya, S, Bhatt, A, Mokadam, N, Uribe, A, Gonzalez, A, Shi, H, Mckeown, J, Pasek, J, Fiorda, J, Echeverria, M, Moreno, R, Zakhary, B, Cavana, M, Cucino, A, Foti, G, Giani, M, Fumagalli, B, Chiumello, D, Castagna, V, Dell'Amore, A, Navalesi, P, Shum, H, Vuysteke, A, Usman, A, Acker, A, Smood, B, Mergler, B, Sertic, F, Subramanian, M, Sperry, A, Rizer, N, Burhan, E, Rasmin, M, Akmal, E, Sitompul, F, Lolong, N, Naivedh, B, Erickson, S, Barrett, P, Dean, D, Daugherty, J, Loforte, A, Khan, I, Quraishi, M, Desantis, O, So, D, Kandamby, D, Mandei, J, Natanael, H, Yudhalantang, E, Lantang, A, Wijaya, S, Jung, A, Ng, G, Ng, W, Ng, P, Fang, S, Tabah, A, Ratcliffe, M, Duroux, M, Alajeeli, A, Tarhabat, A, Adachi, S, Nakao, S, Blanco, P, Prieto, A, Sanchez, J, Nicholson, M, Butt, W, Serratore, A, Delzoppo, C, Janin, P, Yarad, E, Totaro, R, Coles, J, Pujo, B, Balk, R, Vissing, A, Kapania, E, Hays, J, Fox, S, Yantosh, G, Mishin, P, Yuliarto, S, Santoso, K, Djajalaksana, S, Fatoni, A, Fukuda, M, Liu, K, Pelosi, P, Battaglini, D, Jimenez, J, Bastos, D, Gaiao, S, Rusmawatiningtyas, D, Cho, Y, Lee, S, Kawasaki, T, Munshi, L, Sakiyalak, P, Nitayavardhana, P, Elagili, M, Salem, T, Seitz, T, Arora, R, Kent, D, Marino, D, Parwar, S, Cheng, A, Miller, J, Fujitani, S, Shimizu, N, Madhok, J, Owyang, C, Buscher, H, Reynolds, C, Maasikas, O, Aleksanbeljantsev, Mihnovits, V, Akimoto, T, Aizawa, M, Horibe, K, Onodera, R, Hodgson, C, Burrell, A, Young, M, George, T, Shekar, K, Mcguinness, N, Irvine, L, Flynn, B, Endo, T, Sugiyama, K, Shimizu, K, Fan, E, Exconde, K, Ichiba, S, Binnawara, M, Lussier, L, Lotz, G, Malfertheiner, M, Maier, L, Dreier, E, Kusumastuti, N, Mccloskey, C, Dabaliz, A, Elshazly, T, Smith, J, Szuldrzynski, K, Bielanski, P, Wille, K, Murthy, S, Parhar, K, Fiest, K, Codan, C, Shahid, A, Fayed, M, Evans, T, Gutierrez, A, Song, T, Rose, R, Bennett, S, Richardson, D, Peek, G, Arora, L, Rappapport, K, Rudolph, K, Sibenaller, Z, Stout, L, Walter, A, Herr, D, Vedadi, 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Abstract

Following publication of the original article [1], the authors identified that the collaborating authors part of the collaborating author group CCCC Consortium was missing. The collaborating author group is available and included as Additional file 1 in this article.

Published
2023

50. Numerical simulations of compressible Rayleigh-Taylor turbulence in stratified fluids

Author

Scagliarini, A., Biferale, L., Sbragaglia, M., Sugiyama, K., and Toschi, F.

Subjects
Physics - Fluid Dynamics
Abstract

We present results from numerical simulations of Rayleigh-Taylor turbulence, performed using a recently proposed lattice Boltzmann method able to describe consistently a thermal compressible flow subject to an external forcing. The method allowed us to study the system both in the nearly-Boussinesq and strongly compressible regimes. Moreover, we show that when the stratification is important, the presence of the adiabatic gradient causes the arrest of the mixing process., Comment: 15 pages, 11 figures. Proceedings of II Conference on Turbulent Mixing and Beyond (TMB-2009)

Published
2010
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