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4,071 results on '"Shirai, T"'

1. Design of a compact superconducting accelerator for advanced heavy-ion therapy

Author

Iwata, Y., Shirai, T., Mizushima, K., Matsuba, S., Yang, Y., Noda, E., Urata, M., Muramatsu, M., Katagiri, K., Yonai, S., Inaniwa, T., Sato, S., Abe, Y., Fujimoto, T., Sasano, T., Shiraishi, T., Suzuki, T., Takahashi, K., Kondo, Ki., Sakaki, H., Nishiuchi, M., Orikasa, T., Takayama, S., Amano, S., Nakanishi, K., Tachibana, M., Touchi, Y., Tsubomatsu, S., and Nomura, S.

Published
2023
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2. Influence of Earth-Directed Coronal Mass Ejections on the Sun's Shadow Observed by the Tibet-III Air Shower Array

Author

Amenomori, M., Bi, X. J., Chen, D., Chen, T. L., Chen, W. Y., Cui, S. W., Danzengluobu, Ding, L. K., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gou, Q. B., Guo, Y. Q., He, H. H., He, Z. T., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Jia, H. Y., Jiang, L., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Kozai, M., Labaciren, Le, G. M., Li, A. F., Li, H. J., Li, W. J., Liu, C., Liu, J. S., Liu, M. Y., Lu, H., Meng, X. R., Miyazaki, T., Munakata, K., Nakajima, T., Nakamura, Y., Nanjo, H., Nishizawa, M., Niwa, T., Ohnishi, M., Ohta, I., Ozawa, S., Qian, X. L., Qu, X. B., Saito, T., Saito, T. Y., Sakata, M., Sako, T. K., Shao, J., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, H., Wu, H. R., Xue, L., Yamamoto, Y., Yamauchi, K., Yang, Z., Yuan, S. A. F., Zhai, L. M., Zhang, H. M., Zhang, J. L., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, and Zho, X. X.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We examine the possible influence of Earth-directed coronal mass ejections (ECMEs) on the Sun's shadow in the 3~TeV cosmic-ray intensity observed by the Tibet-III air shower (AS) array. We confirm a clear solar-cycle variation of the intensity deficit in the Sun's shadow during ten years between 2000 and 2009. This solar-cycle variation is overall reproduced by our Monte Carlo (MC) simulations of the Sun's shadow based on the potential field model of the solar magnetic field averaged over each solar rotation period. We find, however, that the magnitude of the observed intensity deficit in the Sun's shadow is significantly less than that predicted by MC simulations, particularly during the period around solar maximum when a significant number of ECMEs is recorded. The $\chi^2$ tests of the agreement between the observations and the MC simulations show that the difference is larger during the periods when the ECMEs occur, and the difference is reduced if the periods of ECMEs are excluded from the analysis. This suggests the first experimental evidence of the ECMEs affecting the Sun's shadow observed in the 3~TeV cosmic-ray intensity., Comment: 11 pages, 3 figures, accepted for publication in the ApJ

Published
2018
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3. Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun

Author

Amenomori, M., Bi, X. J., Chen, D., Chen, T. L., Chen, W. Y., Cui, S. W., Danzengluobu, Ding, L. K., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gou, Q. B., Guo, Y. Q., He, H. H., He, Z. T., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Jia, H. Y., Jiang, L., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Kozai, M., Labaciren, Le, G. M., Li, A. F., Li, H. J., Li, W. J., Liu, C., Liu, J. S., Liu, M. Y., Lu, H., Meng, X. R., Miyazaki, T., Mizutani, K., Munakata, K., Nakajima, T., Nakamura, Y., Nanjo, H., Nishizawa, M., Niwa, T., Ohnishi, M., Ohta, I., Ozawa, S., Qian, X. L., Qu, X. B., Saito, T., Saito, T. Y., Sakata, M., Sako, T. K., Shao, J., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, H., Wu, H. R., Xue, L., Yamamoto, Y., Yamauchi, K., Yang, Z., Yuan, S. A. F., Yuda, T., Zhai, L. M., Zhang, H. M., Zhang, J. L., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, and Zho, X. X.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Physics - Space Physics
Abstract

We analyze the Sun's shadow observed with the Tibet-III air shower array and find that the shadow's center deviates northward (southward) from the optical solar disc center in the "Away" ("Toward") IMF sector. By comparing with numerical simulations based on the solar magnetic field model, we find that the average IMF strength in the "Away" ("Toward") sector is $1.54 \pm 0.21_{\rm stat} \pm 0.20_{\rm syst}$ ($1.62 \pm 0.15_{\rm stat} \pm 0.22_{\rm syst}$) times larger than the model prediction. These demonstrate that the observed Sun's shadow is a useful tool for the quantitative evaluation of the average solar magnetic field., Comment: 7 pages, 4 figures

Published
2018
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5. An Experience of Multiple Hematomas in a Coronavirus Disease-19 Patient Administered with ART-123 and Heparin

Author

Shiraki H, Morishita K, Kishino M, Nakatsutsumi K, Kimura K, Shirai T, Ishizuka M, Miyazaki Y, Aiboshi J, and Otomo Y

Subjects
anticoagulation, complication, covid-19, hematoma, tae, Medical emergencies. Critical care. Intensive care. First aid, RC86-88.9
Abstract

Hideto Shiraki,1 Koji Morishita,1 Mitsuhiro Kishino,2 Keita Nakatsutsumi,1 Koichiro Kimura,2 Tsuyoshi Shirai,3 Masahiro Ishizuka,3 Yasunari Miyazaki,3 Junichi Aiboshi,1 Yasuhiro Otomo1 1Department of Acute Critical Care and Disaster Medicine, Tokyo Medical and Dental University Hospital of Medicine, Tokyo, Japan; 2Department of Diagnostic Radiology, Tokyo Medical and Dental University Hospital of Medicine, Tokyo, Japan; 3Department of Respiratory Medicine, Tokyo Medical and Dental University Hospital of Medicine, Tokyo, JapanCorrespondence: Koji MorishitaDepartment of Acute Critical Care and Disaster Medicine, Tokyo Medical and Dental University Hospital of Medicine, 1-5-45 Yushima, Bunkyo-ku, Tokyo, 113-8510, JapanTel +81-3-3813-6111Fax +81-3-5803-0137Email morishita.accm@tmd.ac.jpBackground: Anticoagulant therapy for patients with severe coronavirus disease (COVID-19) pneumonia is considered to improve the hypercoagulable and inflammatory state. However, bleeding complications should also be considered.Case Presentation: A 77-year-old man with a history of falls was diagnosed with COVID-19. Owing to his severe condition, he was intubated and transferred to our hospital for intensive care. Favipiravir, tocilizumab, unfractionated heparin, and ART-123 were administered to treat COVID-19 and manage the antithrombotic prophylaxis for paroxysmal atrial fibrillation (Af). On the 6th day after admission, a hematoma was noted on the left chest wall. Computed tomography (CT) revealed multiple hematomas, including hematomas on his chest wall and obturatorius internus muscle. Emergency angiography transcatheter embolization (TAE) was performed. The patient was transferred to another hospital 23 days after TAE, without complications.Conclusion: Our findings show that anticoagulation therapy and a history of falls induced multiple hematomas in a COVID-19 patient and that the condition was managed with TAE. When anticoagulants are considered in the management of Af and COVID-19 associated coagulopathy, it is necessary to closely monitor potential bleeding complications.Keywords: anticoagulation, complication, COVID-19, hematoma, TAE

Published
2021

6. Observed APO Seasonal Cycle in the Pacific: Estimation of Autumn O2 Oceanic Emissions.

Author

Tohjima, Y., Shirai, T., Ishizawa, M., Mukai, H., Machida, T., Sasakawa, M., Terao, Y., Tsuboi, K., Takao, S., and Nakaoka, S.

Subjects
ATMOSPHERIC carbon dioxide, AUTUMN, ATMOSPHERIC models, ATMOSPHERIC transport, SPRING, ALGAL blooms, ATMOSPHERIC oxygen
Abstract

In this work, we investigated the seasonal cycle of atmospheric potential oxygen (APO), a unique tracer of air‐sea gas exchanges of molecular oxygen (O2) and carbon dioxide (CO2), expressed as APO = O2 + 1.1 × CO2. APO data were obtained from flask air samples collected since the late 1990s at three Japanese ground stations and on commercial cargo ships sailing between Japan and Australia/New Zealand, North America, and Southeast Asia. We also analyzed the APO spatial distribution and seasonal cycles with simulations from an atmospheric transport model using climatological oceanic O2 fluxes from an empirical product that relate O2 flux to ocean heat as input. Model simulations reproduced the observed APO seasonal cycles generally well, but with larger amplitudes and earlier occurrence of seasonal minima and maxima than in the observations. Moreover, the observed seasonal cycles exhibited larger APO enhancements than the simulations in autumn and early winter, especially in the North Pacific at 20°N–60°N. These enhancements remained when refining the comparison by adjusting the simulated APO peak‐to‐peak amplitudes and seasonal phases to the observations. This suggests additional O2 emissions in the North Pacific, not well expressed in the air‐sea O2 fluxes used as input for our model simulations. The average autumn enhancement at 40°N–60°N was approximately twice that measured at 20°N–40°N. Confirming previous studies, our results indicate two distinct mechanisms possibly contributing to the additional oceanic O2 emissions: outgassing from a subsurface shallow oxygen maximum at 20°N–40°N and autumn phytoplankton bloom at 40°N–60°N. Plain Language Summary: Seasonal variations of air‐sea molecular oxygen (O2) exchanges are mainly driven by spring/summer emission and autumn/winter absorption. Emission results mainly from O2 production by phytoplankton at the ocean surface; absorption is related to O2 uptake in deep oxygen‐depleted water layers caused by oceanic ventilation. A phytoplankton bloom in autumn and outgassing from water rich in dissolved O2 just below the mixed layer, known as the shallow oxygen maximum, have been suggested as possible mechanisms contributing to the O2 seasonal cycles. Unfortunately, these oceanic autumn O2 emissions are not well characterized. In this study, we analyzed air samples collected in the western and northern Pacific to evaluate the oceanic component of the O2 seasonal cycle, known as "atmospheric potential oxygen" and calculated as the sum of atmospheric O2 and carbon dioxide. By comparing these observations with model simulations that used previous air‐sea O2 flux estimates as input, we identified marked enhancements in autumn at latitudes between 20°N and 60°N in the Pacific. This corresponds to the geographic area where the autumn phytoplankton bloom and the shallow oxygen maximum occur. This result is a strong indication of additional autumn O2 emissions in the extratropical North Pacific. Key Points: We analyzed atmospheric potential oxygen (APO), a tracer of air‐sea exchanges of molecular oxygen (O2) and carbon dioxide, in the PacificThe observed seasonal APO enhancement at 20°N–60°N in autumn, relative to model simulations, suggests additional oceanic O2 emissionsOutgassing from a shallow oxygen maximum (20–40°N) and an autumn phytoplankton bloom (40–60°N) likely contribute to this enhancement [ABSTRACT FROM AUTHOR]

Published
2024
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9. FeNO and Blood Eosinophils as Potential Predictive Biomarkers for Effectiveness of Dupilumab in Real-life Severe Asthma: Japanese Multi-center Prospective Cohort

Author

Mizumura, K., primary, Gon, Y., additional, Harada, N., additional, Yamada, S., additional, Fukuda, A., additional, Maruoka, S., additional, Abe, S., additional, Takahashi, K., additional, Tanaka, A., additional, Sagara, H., additional, Akamatsu, T., additional, Shirai, T., additional, Masaki, K., additional, Fukunaga, K., additional, Kobayashi, K., additional, Nagase, H., additional, Miyahara, N., additional, Kanehiro, A., additional, Kitamura, N., additional, Sugihara, N., additional, Kumasawa, F., additional, Terada-Hirashima, J., additional, Hojo, M., additional, Chibana, K., additional, and Tagaya, E., additional

Published
2024
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10. Probe of the Solar Magnetic Field Using the 'Cosmic-Ray Shadow' of the Sun

Author

Amenomori, M., Bi, X. J., Chen, D., Chen, T. L., Chen, W. Y., Cui, S. W., Danzengluobu, Ding, L. K., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gou, Q. B., Guo, Y. Q., Hakamada, K., He, H. H., He, Z. T., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Jia, H. Y., Jiang, L., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G. M., Li, A. F., Li, H. J., Li, W. J., Liu, C., Liu, J. S., Liu, M. Y., Lu, H., Meng, X. R., Mizutani, K., Munakata, K., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Onuma, H., Ozawa, S., Qian, X. L., Qu, X. B., Saito, T., Saito, T. Y., Sakata, M., Sako, T. K., Shao, J., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, H., Wu, H. R., Xue, L., Yamamoto, Y., Yang, Z., Yasue, S., Yuan, A. F., Yuda, T., Zhai, L. M., Zhang, H. M., Zhang, J. L., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, and Zhou, X. X.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

We report on a clear solar-cycle variation of the Sun's shadow in the 10 TeV cosmic-ray flux observed by the Tibet air shower array during a full solar cycle from 1996 to 2009. In order to clarify the physical implications of the observed solar cycle variation, we develop numerical simulations of the Sun's shadow, using the Potential Field Source Surface (PFSS) model and the Current Sheet Source Surface (CSSS) model for the coronal magnetic field. We find that the intensity deficit in the simulated Sun's shadow is very sensitive to the coronal magnetic field structure, and the observed variation of the Sun's shadow is better reproduced by the CSSS model. This is the first successful attempt to evaluate the coronal magnetic field models by using the Sun's shadow observed in the TeV cosmic-ray flux., Comment: 11 pages, 4 figures, accepted for publication in Physical Review Letters

Published
2013
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11. A Monte Carlo study to measure the energy spectra of the primary cosmic-ray components at the knee using a new Tibet AS core detector array

Author

Collaboration, The Tibet Asγ, Amenomori, M., Bi, X. J., Chen, D., Chen, W. Y., Cui, S. W., Danzengluobu, Ding, L. K., Ding, X. H., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gou, Q. B., Guo, H. W., Guo, Y. Q., He, H. H., He, Z. T., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Li, W. J., Jia, H. Y., Jiang, L., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G. M., Li, A. F., Liu, C., Liu, J. S., Lu, H., Meng, X. R., Mizutani, K., Munakata, K., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Ozawa, S., Qian, X. L., Qu, X. B., Saito, T., Saito, T. Y., Sakata, M., Sako, T. K., Shao, J., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, H., Wu, H. R., Xue, L., Yamamoto, Y., Yang, Z., Yasue, S., Yuan, A. F., Yuda, T., Zhai, L. M., Zhang, H. M., Zhang, J. L., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, and Zhou, X. X.

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

A new hybrid experiment has been started by AS{\gamma} experiment at Tibet, China, since August 2011, which consists of a low threshold burst-detector-grid (YAC-II, Yangbajing Air shower Core array), the Tibet air-shower array (Tibet-III) and a large underground water Cherenkov muon detector (MD). In this paper, the capability of the measurement of the chemical components (proton, helium and iron) with use of the (Tibet-III+YAC-II) is investigated by means of an extensive Monte Carlo simulation in which the secondary particles are propagated through the (Tibet-III+YAC-II) array and an artificial neural network (ANN) method is applied for the primary mass separation. Our simulation shows that the new installation is powerful to study the chemical compositions, in particular, to obtain the primary energy spectrum of the major component at the knee., Comment: 4 pages,7 figures,In Proc 32nd Int. Cosmic Ray Conf. Vol.1,157 (2011)

Published
2013

14. Photon and spin dependence of the resonance lines shape in the strong coupling regime

Author

Miyashita, S., Shirai, T., Mori, T., De Raedt, H., Bertaina, S., and Chiorescu, I.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics, Quantum Physics
Abstract

We study the quantum dynamics of a spin ensemble coupled to cavity photons. Recently, related experimental results have been reported, showing the existence of the strong coupling regime in such systems. We study the eigenenergy distribution of the multi-spin system (following the Tavis-Cummings model) which shows a peculiar structure as a function of the number of cavity photons and of spins. We study how this structure causes changes in the spectrum of the admittance in the linear response theory, and also the frequency dependence of the excited quantities in the stationary state under a probing field. In particular, we investigate how the structure of the higher excited energy levels changes the spectrum from a double-peak structure (the so-called vacuum field Rabi splitting) to a single peak structure. We also point out that the spin dynamics in the region of the double-peak structure corresponds to recent experiments using cavity ringing while in region of the single peak structure, it corresponds to the coherent Rabi oscillation in a driving electromagnetic filed. Using a standard Lindblad type mechanism, we study the effect of dissipations on the line width and separation in the computed spectra. In particular, we study the relaxation of the total spin in the general case of a spin ensemble in which the total spin of the system is not specified. The theoretical results are correlated with experimental evidence of the strong coupling regime, achieved with a spin 1/2 ensemble.

Published
2012
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15. The Variation of the Solar Neutrino Fluxes over Time in the Homestake, GALLEX(GNO) and Super-Kamiokande Experiments

Author

Sakurai, K., Haubold, H. J., and Shirai, T.

Subjects
Physics - General Physics, Astrophysics - Solar and Stellar Astrophysics
Abstract

Using the records of the fluxes of solar neutrinos from the Homestake, GALLEX (GNO), and Super-Kamiokande experiments, their statistical analyses were performed to search for whether there existed a time variation of these fluxes. The results of the analysis for the three experiments indicate that these fluxes are varying quasi-biennially. This means that both efficiencies of the initial p-p and the pp-III reactions of the proton-proton chain are varying quasi-biennially together with a period of about 26 months. Since this time variation prospectively generated by these two reactions strongly suggests that the efficiency of the proton-proton chain as the main energy source of the Sun has a tendency to vary quasi-biennially due to some chaotic or non-linear process taking place inside the gravitationally stabilized solar fusion reactor. It should be, however, remarked that, at the present moment, we have no theoretical reasoning to resolve this mysterious result generally referred to as the quasi-biennial periodicity in the time variation of the fluxes of solar neutrinos. There is an urgent need to search for the reason why such a quasi-biennial periodicity is caused through some physical process as related to nuclear fusion deep inside the Sun., Comment: 11 pages, pdf

Published
2011

16. On Temporal Variations of the Multi-TeV Cosmic Ray Anisotropy using the Tibet III Air Shower Array

Author

Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., Ding, X. H., Fan, C., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gao, X. Y., Geng, Q. X., Gou, Q. B., Guo, H. W., He, H. H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Huang, Q., Jia, H. Y., Jiang, L., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G. M., Li, A. F., Li, H. C., Li, J. Y., Liu, C., Lou, Y. -Q., Lu, H., Meng, X. R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Ozawa, S., Saito, T., Saito, T. Y., Sakata, M., Sako, T. K., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B., Wang, H., Wang, Y., Wang, Y. G., Wu, H. R., Xue, L., Yamamoto, Y., Yan, C. T., Yang, X. C., Yasue, S., Ye, Z. H., Yu, G. C., Yuan, A. F., Yuda, T., Zhang, H. M., Zhang, J. L., Zhang, N. J., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, and Zhou, X. X.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We analyze the large-scale two-dimensional sidereal anisotropy of multi-TeV cosmic rays by Tibet Air Shower Array, with the data taken from 1999 November to 2008 December. To explore temporal variations of the anisotropy, the data set is divided into nine intervals, each in a time span of about one year. The sidereal anisotropy of magnitude about 0.1% appears fairly stable from year to year over the entire observation period of nine years. This indicates that the anisotropy of TeV Galactic cosmic rays remains insensitive to solar activities since the observation period covers more than a half of the 23rd solar cycle., Comment: 18 pages, 2 figures, accepted by The Astrophysical Journal

Published
2010
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17. Observation of TeV Gamma Rays from the Fermi Bright Galactic Sources with the Tibet Air Shower Array

Author

Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., Ding, X. H., Fan, C., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gao, X. Y., Geng, Q. X., Gou, Q. B., Guo, H. W., He, H. H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Huang, Q., Jia, H. Y., Jiang, L., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G. M., Li, A. F., Li, H. C., Li, J. Y., Liu, C., Lou, Y. -Q., Lu, H., Meng, X. R., Mizutani, K., Mu, J., Munakata, K., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Ozawa, S., Saito, T., Saito, T. Y., Sakata, M., Sako, T. K., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B., Wang, H., Wang, Y., Wang, Y. G., Wu, H. R., Xue, L., Yamamoto, Y., Yan, C. T., Yang, X. C., Yasue, S., Ye, Z. H., Yu, G. C., Yuan, A. F., Yuda, T., Zhang, H. M., Zhang, J. L., Zhang, N. J., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, and Zhou, X. X.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Using the Tibet-III air shower array, we search for TeV gamma-rays from 27 potential Galactic sources in the early list of bright sources obtained by the Fermi Large Area Telescope at energies above 100 MeV. Among them, we observe 7 sources instead of the expected 0.61 sources at a significance of 2 sigma or more excess. The chance probability from Poisson statistics would be estimated to be 3.8 x 10^-6. If the excess distribution observed by the Tibet-III array has a density gradient toward the Galactic plane, the expected number of sources may be enhanced in chance association. Then, the chance probability rises slightly, to 1.2 x 10^-5, based on a simple Monte Carlo simulation. These low chance probabilities clearly show that the Fermi bright Galactic sources have statistically significant correlations with TeV gamma-ray excesses. We also find that all 7 sources are associated with pulsars, and 6 of them are coincident with sources detected by the Milagro experiment at a significance of 3 sigma or more at the representative energy of 35 TeV. The significance maps observed by the Tibet-III air shower array around the Fermi sources, which are coincident with the Milagro >=3sigma sources, are consistent with the Milagro observations. This is the first result of the northern sky survey of the Fermi bright Galactic sources in the TeV region., Comment: 17 pages, 2 figures, 1 table, Accepted for publication in ApJ Letters

Published
2009
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18. Large-scale sidereal anisotropy of multi-TeV galactic cosmic rays and the heliosphere

Author

Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., Ding, X. H., Fan, C., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gao, X. Y., Geng, Q. X., Gou, Q. B., Guo, H. W., He, H. H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Huang, Q., Jia, H. Y., Jiang, L., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G. M., Li, A. F., Li, H. C., Li, J. Y., Liu, C., Lou, Y. -Q., Lu, H., Meng, X. R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Ozawa, S., Saito, T., Saito, T. Y., Sakata, M., Sako, T. K., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B., Wang, H., Wang, Y., Wang, Y. G., Wu, H. R., Xue, L., Yamamoto, Y., Yan, C. T., Yang, X. C., Yasue, S., Ye, Z. H., Yu, G. C., Yuan, A. F., Yuda, T., Zhang, H. M., Zhang, J. L., Zhang, N. J., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhang, Ying, Zhaxisangzhu, Zhou, X. X., and Kota, J.

Subjects
Astrophysics - Galaxy Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

We develop a model anisotropy best-fitting to the two-dimensional sky-map of multi-TeV galactic cosmic ray (GCR) intensity observed with the Tibet III air shower (AS) array. By incorporating a pair of intensity excesses in the hydrogen deflection plane (HDP) suggested by Gurnett et al., together with the uni-directional and bi-directional flows for reproducing the observed global feature, this model successfully reproduces the observed sky-map including the "skewed" feature of the excess intensity from the heliotail direction, whose physical origin has long remained unknown. These additional excesses are modeled by a pair of the northern and southern Gaussian distributions, each placed ~50 degree away from the heliotail direction. The amplitude of the southern excess is as large as ~0.2 %, more than twice the amplitude of the northern excess. This implies that the Tibet AS experiment discovered for the first time a clear evidence of the significant modulation of GCR intensity in the heliotail and the asymmetric heliosphere., Comment: 4 pages, 1 figure, 31st International Cosmic Ray Conference (Lodz, Poland), 2009

Published
2009

19. New estimation of the spectral index of high-energy cosmic rays as determined by the Compton-Getting anisotropy

Author

Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., Ding, X. H., Fan, C., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gao, X. Y., Geng, Q. X., Guo, H. W., He, H. H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Huang, Q., Jia, H. Y., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G. M., Li, A. F., Li, J. Y., Lou, Y. -Q., Lu, H., Lu, S. L., Meng, X. R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Onuma, H., Ouchi, T., Ozawa, S., Ren, J. R., Saito, T., Saito, T. Y., Sakata, M., Sako, T. K., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B., Wang, H., Wang, X., Wang, Y., Wang, Y. G., Wu, H. R., Xue, L., Yamamoto, Y., Yan, C. T., Yang, X. C., Yasue, S., Ye, Z. H., Yu, G. C., Yuan, A. F., Yuda, T., Zhang, H. M., Zhang, J. L., Zhang, N. J., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhaxisangzhu, and Zhou, X. X.

Subjects
Astrophysics
Abstract

The amplitude of the Compton-Getting (CG) anisotropy contains the power-law index of the cosmic-ray energy spectrum. Based on this relation and using the Tibet air-shower array data, we measure the cosmic-ray spectral index to be $-3.03 \pm 0.55_{stat} \pm < 0.62_{syst}$ between 6 TeV and 40 TeV, consistent with $-$2.7 from direct energy spectrum measurements. Potentially, this CG anisotropy analysis can be utilized to confirm the astrophysical origin of the ``knee'' against models for non-standard hadronic interactions in the atmosphere., Comment: accepted to ApJL

Published
2007
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20. Future plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array : simulation and sensitivity

Author

Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., Ding, X. H., Fan, C., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gao, X. Y., Geng, Q. X., Guo, H. W., He, H. H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Huang, Q., Jia, H. Y., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G. M., Li, A. F., Li, J. Y., Lou, Y. -Q., Lu, H., Lu, S. L., Meng, X. R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Onuma, H., Ouchi, T., Ozawa, S., Ren, J. R., Saito, T., Saito, T. Y., Sakata, M., Sako, T. K., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B., Wang, H., Wang, X., Wang, Y., Wang, Y. G., Wu, H. R., Xue, L., Yamamoto, Y., Yan, C. T., Yang, X. C., Yasue, S., Ye, Z. H., Yu, G. C., Yuan, A. F., Yuda, T., Zhang, H. M., Zhang, J. L., Zhang, N. J., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhaxisangzhu, and Zhou, X. X.

Subjects
Astrophysics
Abstract

The Tibet air shower array, which has an effective area of 37,000 square meters and is located at 4300 m in altitude, has been observing air showers induced by cosmic rays with energies above a few TeV. We have a plan to add a large muon detector array to it for the purpose of increasing its sensitivity to cosmic gamma rays in the 100 TeV energy region by discriminating them from cosmic-ray hadrons. We have deduced the attainable sensitivity of the muon detector array using our Monte Carlo simulation. We report here on the detailed procedure of our Monte Carlo simulation., Comment: 4 pages, 5 figures, 30th International Cosmic Ray Conference

Published
2007

21. Future plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array : physics goal and overview

Author

Amenomori, M., Bi, X. J., Chen, D., Cui, S. W., Danzengluobu, Ding, L. K., Ding, X. H., Fan, C., Feng, C. F., Feng, Zhaoyang, Feng, Z. Y., Gao, X. Y., Geng, Q. X., Guo, H. W., He, H. H., He, M., Hibino, K., Hotta, N., Hu, Haibing, Hu, H. B., Huang, J., Huang, Q., Jia, H. Y., Kajino, F., Kasahara, K., Katayose, Y., Kato, C., Kawata, K., Labaciren, Le, G. M., Li, A. F., Li, J. Y., Lou, Y. -Q., Lu, H., Lu, S. L., Meng, X. R., Mizutani, K., Mu, J., Munakata, K., Nagai, A., Nanjo, H., Nishizawa, M., Ohnishi, M., Ohta, I., Onuma, H., Ouchi, T., Ozawa, S., Ren, J. R., Saito, T., Saito, T. Y., Sakata, M., Sako, T. K., Shibata, M., Shiomi, A., Shirai, T., Sugimoto, H., Takita, M., Tan, Y. H., Tateyama, N., Torii, S., Tsuchiya, H., Udo, S., Wang, B., Wang, H., Wang, X., Wang, Y., Wang, Y. G., Wu, H. R., Xue, L., Yamamoto, Y., Yan, C. T., Yang, X. C., Yasue, S., Ye, Z. H., Yu, G. C., Yuan, A. F., Yuda, T., Zhang, H. M., Zhang, J. L., Zhang, N. J., Zhang, X. Y., Zhang, Y., Zhang, Yi, Zhaxisangzhu, and Zhou, X. X.

Subjects
Astrophysics
Abstract

The Tibet air shower array, which has an effective area of 37,000 square meters and is located at 4300 m in altitude, has been observing air showers induced by cosmic rays with energies above a few TeV. We are planning to add a large muon detector array to it for the purpose of increasing its sensitivity to cosmic gamma rays in the 100 TeV (10 - 1000 TeV) energy region by discriminating them from cosmic-ray hadrons. We report on the possibility of detection of gamma rays in the 100 TeV energy region in our field of view, based on the improved sensitivity of our air shower array deduced from the full Monte Carlo simulation., Comment: 4 pages, 3 figures, 30th International Cosmic Ray Conference

Published
2007

22. Risk profiles and one-year outcomes of patients with newly diagnosed atrial fibrillation in India: Insights from the GARFIELD-AF Registry

Author

Kakkar, Ajay K., Bassand, Jean-Pierre, John Camm, A., Fitzmaurice, David A., Goldhaber, Samuel Z., Goto, Shinya, Haas, Sylvia, Hacke, Werner, Mantovani, Lorenzo G., Misselwitz, Frank, Pieper, Karen S., Turpie, Alexander G.G., van Eickels, Martin, Verheugt, Freek W.A., Kayani, Gloria, Fox, Keith A.A., Gersh, Bernard J., Luciardi, Hector Lucas, Gibbs, Harry, Brodmann, Marianne, Cools, Frank, Barretto, Antonio Carlos Pereira, Connolly, Stuart J., Spyropoulos, Alex, Eikelboom, John, Corbalan, Ramon, Hu, Dayi, Jansky, Petr, Nielsen, Jørn Dalsgaard, Ragy, Hany, Raatikainen, Pekka, Le Heuzey, Jean-Yves, Darius, Harald, Keltai, Matyas, Kakkar, Sanjay, Sawhney, Jitendra Pal Singh, Agnelli, Giancarlo, Ambrosio, Giuseppe, Koretsune, Yukihiro, Sánchez Díaz, Carlos Jerjes, Ten Cate, Hugo, Atar, Dan, Stepinska, Janina, Panchenko, Elizaveta, Lim, Toon Wei, Jacobson, Barry, Oh, Seil, Viñolas, Xavier, Rosenqvist, Marten, Steffel, Jan, Angchaisuksiri, Pantep, Oto, Ali, Parkhomenko, Alex, Al Mahmeed, Wael, Fitzmaurice, David, Hu, D.Y., Chen, K.N., Zhao, Y.S., Zhang, H.Q., Chen, J.Z., Cao, S.P., Wang, D.W., Yang, Y.J., Li, W.H., Yin, Y.H., Tao, G.Z., Yang, P., Chen, Y.M., He, S.H., Wang, Ying, Wang, Yong, Fu, G.S., Li, X., Wu, T.G., Cheng, X.S., Yan, X.W., Zhao, R.P., Chen, M.S., Xiong, L.G., Chen, P., Jiao, Y., Guo, Y., Xue, L., Wang, F.Z., Li, H., Yang, Z.M., Bai, C.L., Chen, J., Chen, J.Y., Chen, X., Feng, S., Fu, Q.H., Gao, X.J., Guo, W.N., He, R.H., He, X.A., Hu, X.S., Huang, X.F., Li, B., Li, J., Li, L., Li, Y.H., Liu, T.T., Liu, W.L., Liu, Y.Y., Lu, Z.C., Luo, X.L., Ma, T.Y., Peng, J.Q., Sheng, X., Shi, X.J., Sun, Y.H., Tian, G., Wang, K., Wang, L., Wu, R.N., Xie, Q., Xu, R.Y., Yang, J.S., Yang, L.L., Yang, Q., Ye, Y., Yu, H.Y., Yu, J.H., Yu, T., Zhai, H., Zhan, Q., Zhang, G.S., Zhang, Q., Zhang, R., Zhang, Y., Zheng, W.Y., Zhou, B., Zhou, Z.H., Zhu, X.Y., Kakkar, S., Sawhney, J.P.S., Jadhav, P., Durgaprasad, R., Ravi Shankar, A.G., Rajput, R.K., Bhargava, K., Sarma, R., Srinivas, A., Roy, D., Nagamalesh, U.M., Chopda, M., Kishore, R., Kulkarni, G., Chandwani, P., Pothiwala, R.A., Padinhare Purayil, M., Shah, S., Chawla, K., Kothiwale, V.A., Raghuraman, B., Vijayaraghavan, G., Vijan, V.M., Bantwal, G., Bisne, V., Khan, A., Gupta, J.B., Kumar, S., Jain, D., Abraham, S., Adak, D., Barai, A., Begum, H., Bhattacharjee, P., Dargude, M., Davies, D., Deshpande, B., Dhakrao, P., Dhyani, V., Duhan, S., Earath, M., Ganatra, A., Giradkar, S., Jain, V., Karthikeyan, R., Kasala, L., Kaur, S., Krishnappa, S., Lawande, A., Lokesh, B., Madarkar, N., Meena, R., More, P., Naik, D., Prashanth, K., Rao, M., Rao, N.M., Sadhu, N., Shah, D., Sharma, M., Shiva, P., Singhal, S., Suresh, S., Vanajakshamma, V., Panse, S.G., Koretsune, Y., Kanamori, S., Yamamoto, K., Kumagai, K., Katsuda, Y., Sadamatsu, K., Toyota, F., Mizuno, Y., Misumi, I., Noguchi, H., Ando, S., Suetsugu, T., Minamoto, M., Oda, Hiroshi, Shiraishi, K., Adachi, S., Chiba, K., Norita, H., Tsuruta, M., Koyanagi, T., Ando, H., Higashi, T., Okada, K., Azakami, S., Komaki, S., Kumeda, K., Murayama, T., Matsumura, J., Oba, Y., Sonoda, R., Goto, K., Minoda, K., Haraguchi, Y., Suefuji, H., Miyagi, H., Kato, H., Nakamura, Tadashi, Nakamura, Tsugihiro, Nandate, H., Zaitsu, R., Fujiura, Yoshihisa, Yoshimura, A., Numata, H., Ogawa, J., Tatematsu, H., Kamogawa, Y., Murakami, K., Wakasa, Y., Yamasawa, M., Maekawa, H., Abe, S., Kihara, H., Tsunoda, S., Saito, Katsumi, Saito, Kazuyuki, Fudo, T., Obunai, K., Tachibana, H., Oba, I., Kuwahata, T., Higa, S., Gushiken, M., Eto, T., Yoshida, H., Ikeda, D., Fujiura, Yoshitake, Ishizawa, M., Nakatsuka, M., Murata, K., Ogurusu, C., Shimoyama, M., Akutsu, M., Takamura, I., Hoshino, F., Yokota, N., Iwao, T., Tsuchida, K., Takeuchi, M., Hatori, Y., Kitami, Y., Nakamura, Yoichi, Oyama, R., Ageta, M., Oda, Hiroyuki, Go, Y., Mishima, K., Unoki, T., Morii, S., Shiga, Yuhei, Sumi, H., Nagatomo, T., Sanno, K., Fujisawa, K., Atsuchi, Y., Nagoshi, T., Seto, T., Tabuchi, T., Kameko, M., Nii, K., Oshiro, K., Takezawa, H., Nagano, S., Miyamoto, N., Iwaki, M., Nakamura, Yuichiro, Fujii, M., Okawa, M., Abe, Masahiko, Abe, Masatake, Abe, Mitsunori, Saito, T., Mito, T., Nagao, K., Minami, J., Mita, T., Sakuma, I., Taguchi, T., Marusaki, S., Doi, H., Tanaka, M., Fujito, T., Matsuta, M., Kusumoto, T., Kakinoki, S., Ashida, K., Yoshizawa, N., Agata, J., Arasaki, O., Manita, M., Ikemura, M., Fukuoka, S., Murakami, H., Matsukawa, S., Hata, Y., Taniguchi, T., Ko, T., Kubo, H., Imamaki, M., Akiyama, M., Inagaki, M., Odakura, H., Ueda, T., Katsube, Y., Nakata, A., Watanabe, H., Techigawara, M., Igarashi, M., Taga, K., Kimura, T., Tomimoto, S., Shibuya, M., Nakano, M., Ito, K., Seo, T., Hiramitsu, S., Hosokawa, H., Hoshiai, M., Hibino, M., Miyagawa, K., Horie, Hajime, Sugishita, N., Shiga, Yukio, Soma, A., Neya, K., Yoshida, Tetsuro, Yoshida, Tomoki, Mizuguchi, M., Ishiguro, M., Minagawa, T., Wada, M., Mukawa, H., Okuda, F., Nagasaka, S., Abe, Y., Adachi, Sen, Adachi, Susumu, Adachi, T., Akahane, K., Amano, T., Aoki, K., Aoyama, T., Arai, H., Arima, S., Arino, T., Asano, H., Asano, T., Azuma, J., Baba, T., Betsuyaku, T., Chibana, H., Date, H., Doiuchi, J., Emura, Y., Endo, M., Fujii, Y., Fujiki, R., Fujisawa, A., Fujisawa, Y., Fukuda, T., Fukui, T., Furukawa, N., Furukawa, T., Furumoto, W., Goto, T., Hamaoka, M., Hanazono, N., Hasegawa, K., Hatsuno, T., Hayashi, Y., Higuchi, K., Hirasawa, K., Hirayama, H., Hirose, M., Hirota, S., Honda, M., Horie, Hideki, Ido, T., Iiji, O., Ikeda, H., Ikeda, K., Ikeoka, K., Imaizumi, M., Inaba, H., Inoue, T., Iseki, F., Ishihara, A., Ishioka, N., Ito, N., Iwase, T., Kakuda, H., Kamata, J., Kanai, H., Kanda, H., Kaneko, M., Kano, H., Kasai, T., Kato, T., Kato, Y., Kawada, Y., Kawai, K., Kawakami, K., Kawakami, S., Kawamoto, T., Kawano, S., Kim, J., Kira, T., Kitazawa, H., Kitazumi, H., Kito, T., Kobayashi, T., Koeda, T., Kojima, J., Komatsu, H., Komatsu, I., Koshibu, Y., Kotani, T., Kozuka, T., Kumai, Y., Kumazaki, T., Maeda, I., Maeda, K., Maruyama, Y., Matsui, S., Matsushita, K., Matsuura, Y., Mineoi, K., Mitsuhashi, H., Miura, N., Miyaguchi, S., Miyajima, S., Miyamoto, H., Miyashita, A., Miyata, S., Mizuguchi, I., Mizuno, A., Mori, T., Moriai, O., Morishita, K., Murai, O., Nagai, Sho, Nagai, Shunichi, Nagata, E., Nagata, H., Nakagomi, A., Nakahara, S., Nakamura, M., Nakamura, R., Nakanishi, N., Nakayama, T., Nakazato, R., Nanke, T., Nariyama, J., Niijima, Y., Niinuma, H., Nishida, Y., Nishihata, Y., Nishino, K., Nishioka, H., Nishizawa, K., Niwa, I., Nomura, K., Nomura, S., Nozoe, M., Ogawa, T., Ohara, N., Okada, M., Okamoto, K., Okita, H., Okuyama, M., Ono, H., Ono, T., Onuki Pearce, Y., Oriso, S., Ota, A., Otaki, E., Saito, Y., Sakai, H., Sakamoto, N., Sakamoto, Y., Samejima, Y., Sasagawa, Y., Sasaguri, H., Sasaki, A., Sasaki, T., Sato, Kazuki, Sato, Kiyoharu, Sawano, M., Seki, S., Sekine, Y., Seta, Y., Sezaki, K., Shibata, N., Shiina, Y., Shimono, H., Shimoyama, Y., Shindo, T., Shinohara, H., Shinohe, R., Shinozuka, T., Shirai, T., Shiraiwa, T., Shozawa, Y., Suga, T., Sugimoto, C., Suzuki, Kazuo, Suzuki, Keita, Suzuki, Shu, Suzuki, Shunji, Suzuki, Susumu, Suzuki, Y., Tada, M., Taguchi, A., Takagi, T., Takagi, Y., Takahashi, K., Takahashi, S., Takai, H., Takanaka, C., Take, S., Takeda, H., Takei, K., Takenaka, K., Tana, T., Tanabe, G., Taya, K., Teragawa, H., Tohyo, S., Toru, S., Tsuchiya, Y., Tsuji, T., Tsuzaki, K., Uchiyama, H., Ueda, O., Ueyama, Y., Wakaki, N., Wakiyama, T., Washizuka, T., Watanabe, M., Yamada, T., Yamagishi, T., Yamaguchi, H., Yamamoto, Kenichi, Yamamoto, Kentaro, Yamamoto, Kunihiko, Yamamoto, T., Yamaura, M., Yamazoe, M., Yasui, K., Yokoyama, Y., Yoshida, K., Lim, T.W., Ching, C.K., Foo, C.G., Chow, J.H., Chen, D.D., Jaufeerally, F.R., Lee, Y.M., Lim, G., Lim, W.T., Thng, S., Yap, S.Y., Yeo, C., Oh, S., Pak, H.N., Kim, J.-B., Kim, J.H., Jang, S.-W., Kim, D.H., Ryu, D.R., Park, S.W., Kim, D.-K., Choi, D.J., Oh, Y.S., Cho, M.-C., Kim, S.-H., Jeon, 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E.J., Yun, S.Y., Angchaisuksiri, P., Chawanadelert, S., Mongkolwongroj, P., Kanokphatcharakun, K., Cheewatanakornkul, S., Laksomya, T., Pattanaprichakul, S., Chantrarat, T., Rungaramsin, S., Silaruks, S., Wongcharoen, W., Siriwattana, K., Likittanasombat, K., Katekangplu, P., Boonyapisit, W., Cholsaringkarl, D., Chatlaong, B., Chattranukulchai, P., Santanakorn, Y., Hutayanon, P., Khunrong, P., Bunyapipat, T., Jai-Aue, S., Kaewsuwanna, P., Bamungpong, P., Gunaparn, S., Hongsuppinyo, S., Inphontan, R., Khattaroek, R., Khunkong, K., Kitmapawanont, U., Kongsin, C., Naratreekoon, B., Ninwaranon, S., Phangyota, J., Phrommintikul, A., Phunpinyosak, P., Pongmorakot, K., Poomiphol, S., Pornnimitthum, N., Pumprueg, S., Ratchasikaew, S., Sanit, K., Sawanyawisuth, K., Silaruks, B., Sirichai, R., Sriwichian, A., Suebjaksing, W., Sukklad, P., Suttana, T., Tangsirira, A., Thangpet, O., Tiyanon, W., Vorasettakarnkij, Y., Wisaratapong, T., Wongtheptien, W., Wutthimanop, A., Yawila, S., Oto, A., Altun, A., Ozdogru, I., Ozdemir, K., Yilmaz, O., Aydinlar, A., Yilmaz, M.B., Yeter, E., Ongen, Z., Cayli, M., Pekdemir, H., Ozdemir, M., Sucu, M., Sayin, T., Demir, M., Yorgun, H., Ersanli, M., Okuyan, E., Aras, D., Abdelrahman, H., Aktas, O., Alpay, D., Aras, F., Bireciklioglu, M.F., Budeyri, S., Buyukpapuc, M., Caliskan, S., Esen, M., Felekoglu, M.A., Genc, D., Ikitimur, B., Karaayvaz, E.B., Kılıç Karataş, S., Okutucu, S., Ozcelik, E., Quisi, A., Sag, H., Sahiner, L., Sayin, B.Y., Seker, T., Uzun Alkan, D., Yildirim, E., Yildirim, R., Yilmaz, F., Yuksekdag, V., Luciardi, H.L., Vensentini, N., Ingaramo, A.C., Sambadaro, G.A., Fernandez Caputi, V., Berman, S.G., Dragotto, P., Kleiban, A.J., Centurion, N., Giacomi, G., Ahuad Guerrero, R.A., Conde, D., Zapata, G., Di Paola, L.A., Ramos, J.L., Dran, R.D., Egido, J., Fernandez, A.A., Fosco, M.J., Sassone, S., Sinisi, V.A., Cartasegna, L.R., Berli, M.A., Gomez Vilamajo, O.A., Ferroni, F., Alaguibe, E.D., Alvarez D'Amelio, A., Arabetti, C., Arias, L., Belardi, J.A., Bergesio, L., Berli, F., Berli, M., Borchowiec, S., Buzzetti, C., Cabrini, R., Campisi, V., Cappi, A.L., Carrizo, R., Colombo Berra, F., Costabel, J.P., Costamagna, O.J.A., Damonte, A.A., De Urquiza, I.N., Diez, F., Edén, M.F., Fanuele, M., Fernandez Voena, F., Foa Torres, M., Funosas, C., Giacomi, M.P., Gimenez, C.H., Gurfinkel, E.P., de L.M. 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Epelde Gonzalo, F., Almeida Fernández, C.A., Del Val Plana, N., Escrivá Montserrat, E., Montero Alía, J.J., Barreda González, M., Moleiro Oliva, M.A., Iglesias Sanmartín, J., Jiménez González, M., Rodriguez Álvarez, M., Herreros Melenchon, J., Ripoll Vera, T., Ridocci Soriano, F., Garcia Riesco, L., Marco Macian, M.D., Quiles Granado, J., Jimenez Navarro, M., Cosin Sales, J., Vaquer Perez, J.V., Vazquez Caamano, M., Arcocha Torres, M.F., Marcos Gomez, G., Iñiguez Romo, A., Prieto Diaz, M.A., Alonso, Carmela, Alonso, Concepcion, Alvarez, D., Alvarez, M., Amaro, M., Andere, N., Aracil Villar, J., Armitano Ochoa, R., Austria, A., Barbeira, S., Barraquer Feu, E., Bartes, A., Becerra Munoz, V., Bermudez Jimenez, F.J., Branjovich Tijuan, A., Cabeza Ramirez, J., Cabrera Ramos, M., Calvo Martinez, E., Campo Moreno, M., Cancho Corchado, G., Casanova Gil, M., Castillo Orive, M., Castro Fernandez, D., Cebollada del Misterio, M., Codinachs Alsina, R., Cortada Cabrera, A., Costa Pinto Prego de 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S., de Kare-Silver, N., Gilliland, A., Strieder, E., Howitt, A., Vishwanathan, B., Bird, N., Gray, D., Clark, M., Bisatt, J., Litchfield, J., Fisher, E., Fooks, T., Kelsall, A.R., Alborough, E., Wakeling, J., Parfitt, M., Milne, K., Rogers, S., Priyadharshan, R., Oliver, J.L., Davies, E., Abushal, S., Jacobs, M., Hutton, C., Walls, N.I., Thompson, R., Chigbo, C., Zaidi, S.M.A., Howard, M., Butter, K.C., Barrow, S., Little, H., Haq, I.U., Gibbons, L., Glencross, S., McLeod, A.J., Poland, K., Mulholland, C., Warke, A., Conn, P., Burns, G., Smith, R.N., Lowe, S., Kamath, R., Dau, H.S., Webster, J., Hodgins, I., Vercoe, S., Roome, P.C., Pinnock, H., Patel, J.R.A., Ali, A., Hart, N., Davies, R., Stuart, E., Neden, C.A., Danielsen, M., Heath, R., Sharma, P., Galloway, S., Hawkins, C., Oliver, R., Aylward, M., Mannion, S., Braddick, M., Edwards, D., Rothwell, A.C., Sabir, A., Choudhary, F., Khalaque, S., Wilson, A., Peters, S., Coulson, W., Roberts, N., Heer, A., Coates, S., Ward, B., 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A., Colquhoun, D., Kiat, H., Eccleston, D., French, J., Zimmett, L., Ayres, B., Phan, T., Blombery, P., Crimmins, D., O'Donnell, D., Choi, A., Astridge, P., Arstall, M., Jepson, N., Binnekamp, M., Lee, A., Rogers, J., Starmer, G., Carroll, P., Faunt, J., Aggarwala, A., Barry, L., Batta, C., Beveridge, R., Black, A., Bonner, M., Boys, J., Buckley, E., Campo, M., Carlton, L., Connelly, A., Conway, B., Cresp, D., Dimitri, H., Dixon, S., Dolman, M., Duroux, M., Eskandari, M., Eslick, R., Ferreira-Jardim, A., Fetahovic, T., Fitzpatrick, D., Geraghty, R., Gibbs, J., Grabek, T., Modi, M.H., Hayes, K., Hegde, M.P., Hesketh, L., Hoffmann, B., Jacobson, B., Johnson, K., Juergens, C., Kassam, I., Lawlor, V., Lehman, M., Lehman, S., Leung, D., Mackay, S., MacKenzie, M., McCarthy, C., McIntosh, C., McKeon, L., Morrison, H., Mussap, C., Myers, J.-D., Nagalingam, V., Oldfield, G., O'May, V., Palmer, J., Parsons, L., Patching, K., Patching, T., Paul, V., Plotz, M., Preston, S., Rashad, H., Ratcliffe, M., Raynes, S., Rose, J., Sanders, L., Seremetkoska, M., Setio, H., Shone, S., Shrestha, P., Singh, C., Singleton, C., Stoyanov, N., Sutcliffe, S., Swaraj, K., Tarrant, J., Thompson, S., Tsay, I.M., Vorster, M., Waldman, A., Wallis, L., Wilford, E., Wong, K., Connolly, S.J., Spyropoulos, A., Eikelboom, J., Luton, R., Gupta, M., Pandey, A.S., Cheung, S., Leader, R., Beaudry, P., Ayala-Paredes, F., Berlingieri, J., Heath, J., Poirier, G., Du Preez, M., Nadeau, R., Dresser, G., Dhillon, R., Hruczkowski, T., Schweitzer, B., Coutu, B., Angaran, P., MacDonald, P., Vizel, S., Fikry, S., Parkash, R., Lavoie, A., Cha, J., Ramjattan, B., Bonet, J., Ahmad, K., Aro, L., Aves, T., Beaudry, K., Bergeron, C., Bigcanoe, J., Bignell, N., Breakwell, L., Burke, E., Carroll, L., Clarke, B., Cleveland, T., Daheb, S., Dehghani, P., Denis, I., Djaidani, Z., Dorian, P., Douglass, S., Dunnigan, J., Ewert, A., Farquhar, D., Fearon, A., Ferleyko, L., Fournier, D., Fox, B., Grenier, M.-C., Gulliver, W., Haveman, K., Hines, C., Hines, K., Jackson, A.M., Jean, C., Jethoo, G., Kahlon, R., Kelly, S., Kim, R., Korley, V., Kornder, J., Kwan, L., Largy, J., Lewis, C., Lewis, S., Mangat, I., Moor, R., Navratil, J., Neas, I., Otis, J., Otis, R., Pandey, M., Petrie, F., Pinter, A., Raines, M., Roberts, P., Robinson, M., Sas, G., Schulman, S., Snell, L., Spearson, S., Stevenson, J., Trahey, T., Wong, S., Wright, D., Ragy, H., Abd El-Aziz, A., Abou Seif, S.K., El Din, M.G., El Etriby, S., Elbahry, A., El-Etreby, A., Elkhadem, M., Katta, A., Khairy, T., Mowafy, A., Nawar, M., Ohanissian, A., Reda, A., Reda, M., Salem, H., Sami, N., Samir, S., Setiha, M., Sobhy, M., Soliman, A., Taha, N., Tawfik, M., Zaatout, E., Kettles, D., Bayat, J., Siebert, H., Horak, A., Kelfkens, Y., Garda, R., Pillay, T., Guerra, M., van Zyl, L., Theron, H., Murray, A., Louw, R., Greyling, D., Mntla, P., Ueckermann, V., Loghdey, R., Ismail, S., Ahmed, F., Engelbrecht, J., Ramdass, A., Maharajh, S., Oosthuysen, W., Angel, G., Bester, C., Booysen, M., Boshoff, C., Cannon, C., Cassimjee, S., Chami, C., Conway, G., Davids, A., de Meyer, L., Du Plessis, G., Ellis, T., Henley, L., Karsten, M., Loyd, E., Marks, J., Mavhusa, L., Mostert, M., Page, A., Rikhotso, L., Salie, M., Sasto, J., Shaik, F., Skein, A., Smith, L., Tarr, G., Tau, T., van Zyl, F., Al Mahmeed, W., Yousef, G., Agrawal, A., Nathani, M., Ibrahim, M., Esheiba, E.M., Singh, R., Naguib, A., Abu-Mahfouz, M., Al Omairi, M., Al Naeemi, A., Maruthanayagam, R., Bazargani, N., Wassef, A., Gupta, R., Khan, M., Subbaraman, B., Abdul, A., Al Mulla, A., El Bardisy, S., Haridas, P., Jadhav, S., Magdaluyo, K., Makdad, M., Maqsood, I., Mohamed, R., Sharma, N., Sharma, R., Thanzeel, M., Goldhaber, S.Z., Canosa, R., Rama, P., Blumberg, E., Garcia, J., Mullen, P., Wilson, V., Quick, A., Ferrick, K., Kutayli, W.M., Cox, M., Franco, M., Falkowski, S., Mendelson, R., Williams, M., Miller, S., Beach, S., Alfieri, A., Gutowski, T., Haque, I., Reddy, R., Ahmed, W., Delafontaine, P., Diercks, D., Theodoro, D., Remmel, K., Alberts, M., Ison, R., Noveck, H., Duffy, P., Pitta, S., Nishijima, D., Treasure, C., Asafu-Adjaye, N., Ball, K., Bartlett, M., Bentley, M., Bowers, S., Brown, A., Browne, A., Cameron-Watts, J., Canova, M., Cassidy, D., Cervellione, K., Congal, S., DePauw, J., Dickerson, A., Eley, M., Evans, L., Felpel, S., Ferdinand, K., Fielder, D., Gentry, P., Haideri, A., Hakimi, F., Harbour, T., Hartranft, E., Hawkins, B., Headlee, M., Henson, L., Herrick, C., Hicks, T., Jasinski, S., Jones, A., Jones, L., Jones, P., Karl, S., Keeling, M., Kerr, J., Knowles, P., Langdon, J., Lay, M., Lee, J.A., Lincoln, T., Malone, E., Merliss, A., Merritt, D., Minardo, J., Mooso, B., Orosco, C., Palumbo, V., Parker, M., Parrott, T., Paserchia, S., Pearl, G., Peterson, J., Pickelsimer, N., Purcell, T., Raynor, J., Raziano, S., Richard, C., Richardson, T., Robertson, C., Sage, A., Sanghera, T., Shaw, P., Shoemaker, J., Smith, K., Stephanie, B., Thatcher, A., Theobald, H., Thompson, N., Treasure, L., Tripti, T., Verdi, C., Worthy, V., Sawhney, Jitendra PS., Kothiwale, Veerappa A., Bisne, Vikas, Durgaprasad, Rajashekhar, Jadhav, Praveen, Chopda, Manoj, Vanajakshamma, Velam, Meena, Ramdhan, Vijayaraghavan, Govindan, Chawla, Kamaldeep, and Allu, Jagan

Published
2018
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24. High Power Model Fabrication of Biperiodic L-Support Disk-and-Washer Structure

Author

Ao, H., Iwashita, Y., Shirai, T., Noda, A., Inoue, M., Kawakita, T., Ohkubo, K., and Nakanishi, K.

Subjects
Physics - Accelerator Physics
Abstract

The high power test model of biperiodic L-support disk-and- washer was fabricated. Among some trouble in the fabrication, the main one was a vacuum leak in a brazing process. The repair test of the leak showed a good result; four units were recovered out of five leak units (recover rate 80%). While an accelerating mode frequency was tuned at an operating frequency of 2857 MHz by squeezing method, a coupling mode frequency of 2847MHz and the 3.4% field flatness (peak to peak ratio) were achieved., Comment: 3 pages Linac2000 Poster TUA22 (5 figures available from author)

Published
2000

34. Mechanisms that influence the formation of high‐ozone regions in the boundary layer downwind of the Asian continent in winter and spring

Author

Kondo, Y, Hudman, RC, Nakamura, K, Koike, M, Chen, G, Miyazaki, Y, Takegawa, N, Blake, DR, Simpson, IJ, Ko, M, Kita, K, Shirai, T, and Kawakami, S

Subjects
Earth Sciences, Atmospheric Sciences, Climate-Related Exposures and Conditions, Climate Action, Meteorology & Atmospheric Sciences
Abstract

The seasonal variation of ozone (O3) in the boundary layer (BL) over the western Pacific is investigated using a chemistry-transport model. The model results for January and April-May 2002 were evaluated by comparison with PEACE aircraft observations. In January, strong northwesterlies efficiently transported NOx from the continent, leading to an O3 increase of approximately 5-10 ppbv over a distance of about 3000 km. In April, southwesterlies dominated due to anticyclone development over the western Pacific. Along this flow, O3 continued to be produced by NO x emitted from East Asia. This resulted in the formation of a high-O3 (> 50 ppbv) region extending along the coastal areas of East Asia. This seasonal change in O3 was driven in part by a change in the net O3 production rate due to increases in solar UV and H 2O. Its exact response depended on the NOx values in the BL. The net O3 production rate increased between winter and spring over the Asian continent and decreased over the remote western Pacific. Model simulations show that about 25% of the total O3 (of 10-20 ppbv) increase over the coastal region of Northeast Asia was due to local production from NOx emissions from China, and the rest was due to changes in background levels as well as emissions from Korea, Japan, and east Siberia. Uplift of BL air over Asia, horizontal transport in the free troposphere, and subsidence were the principal mechanisms of transporting Asian O3 to the central and eastern North Pacific Copyright 2008 by the American Geophysical Union.

Published
2008

37. Seasonal variations of atmospheric C2-C7 nonmethane hydrocarbons in Tokyo

Author

Shirai, T, Yokouchi, Y, Blake, DR, Kita, K, Izumi, K, Koike, M, Komazaki, Y, Miyazaki, Y, Fukuda, M, and Kondo, Y

Subjects
Meteorology & Atmospheric Sciences
Abstract

Eighteen C2-C7 NMHCs (nonmethane hydrocarbons) were measured hourly during the Integrated Measurement Program for Aerosol and Oxidant Chemistry in Tokyo (IMPACT) measurement campaigns conducted in central Tokyo during four different periods (summer/autumn of 2003 and winter/summer of 2004). The ambient atmospheric concentrations of NMHCs showed an inverse correlation with wind speed and mixing height and were significantly affected by mesoscale weather conditions. The mixing ratio of isoprene tightly correlated with solar flux and temperature in summer, as it was dominantly emitted by the local vegetation. All the observed NMHCs except isoprene showed high correlation with each other in winter (r2 > 0.5), suggesting concurrent accumulation under stagnant condition and common sources. Emission ratios were calculated on the basis of the correlation with carbon monoxide and ethyne. Compared to the typical winter NMEC composition, during summer there was a significant increase (up to 7 times higher than wintertime) of C4-C5 alkanes from ftiel evaporation; of C2-C3 alkenes, n-hexane and benzene from chemical industry; and of toluene from local manufacturers, reflecting the temperature dependence of these evaporative emissions. In addition to the online measurements in Tokyo, canister sampling at a suburban site (Kisai) followed by multidimensional GC analyses was conducted during the summer campaign in 2004. The atmospheric concentrations of longer-lived compounds (≥ several days) at Kisai showed the buildup under sea breeze circulation. The average ambient, concentration of toluene was 2 times higher than that in central Tokyo, likely because of substantial emissions from local industries as reported in the prefectural statistics. Copyright 2007 by the American Geophysical Union.

Published
2007

38. Measurements of reactive nitrogen produced by tropical thunderstorms during BIBLE-C

Author

Koike, M, Kondo, Y, Kita, K, Takegawa, N, Nishi, N, Kashihara, T, Kawakami, S, Kudoh, S, Blake, D, Shirai, T, Liley, B, Ko, MK, Miyazaki, Y, Kawasaki, Z, and Ogawa, T

Subjects
Meteorology & Atmospheric Sciences
Abstract

The Biomass Burning and Lightning Experiment phase C (BIBLE-C) aircraft mission was carried out near Darwin, Australia (12°S, 131°E) in December 2000. This was the first aircraft experiment designed to estimate lightning NO production rates in the tropics, where production is considered to be most intense. During the two flights (flights 10 and 13 made on December 9 and 11-12, respectively) enhancements of NOx (NO + NO2) up to 1000 and 1600 parts per trillion by volume (pptv, 10-s data) were observed at altitudes between 11.5 and 14 km. The Geostationary Meteorological Satellite (GMS) cloud (brightness temperature) data and ground-based lightning measurements by the Global Positioning and Tracking System (GPATS) indicate that there were intensive lightning events over the coast of the Gulf of Carpentaria, which took place upstream from our measurement area 10 to 14 h prior to the measurements. For these two flights, air in which NOx exceeded 100 pptv extended over 620 × 140 and 400 × 170 km2 (wind direction x perpendicular direction), respectively, suggesting a significant impact of lightning NO production on NOx levels in the tropics. We estimate the amount of NOx observed between 11.5 and 14 km produced by the thunderstorms to be 3.3 and 1.8 × 1025 NO molecules for flights 10 and 13, respectively. By using the GPATS lightning flash count data, column NO production rates are estimated to be 1.9-4.4 and 21-49 × 1025 NO molecules per single flash for these two flight data sets. In these estimations, it is assumed that the column NO production between 0 and 16 km is greater than the observed values between 11.5 and 14 km by a factor of 3.2, which is derived using results reported by Pickering et al. (1998). There are however large uncertainties in the GPATS lightning data in this study and care must be made when the production rates are referred. Uncertainties in these estimates are discussed. The impact on the ozone production rate is also described. Copyright 2007 by the American Geophysical Union.

Published
2007

39. Evolution of mixing state of black carbon particles: Aircraft measurements over the western Pacific in March 2004

Author

Moteki, N, Kondo, Y, Miyazaki, Y, Takegawa, N, Komazaki, Y, Kurata, G, Shirai, T, Blake, DR, Miyakawa, T, and Koike, M

Subjects
Meteorology & Atmospheric Sciences
Abstract

We report the evolution of the mixing state of black carbon (BC) particles in urban plumes measured by an airborne single particle soot photometer. The aircraft observations were conducted over the ocean near the coast of Japan in March 2004. The number fiaction of coated BC particles with a core diameter of 180 mn increased from 0.35 to 0.63 within 12 hours (h), namely 2.3% h-1, after being emitted from the Nagoya urban area in Japan. BC particles with a core diameter of 250 nm increased at the slower rate of 1.0% h-1. The increase in coated BC particles was associated with increases in non-sea salt sulfate and water-soluble organic carbon by a factor of approximately two, indicating that these compounds contributed to the coating on the BC particles. These results give direct evidence that BC particles become internally mixed on a time scale of 12 h in urban plumes. Copyright 2007 by the American Geophysical Union.

Published
2007

40. Photochemistry of ozone over the western Pacific from winter to spring

Author

Kondo, Y, Nakamura, K, Chen, G, Takegawa, N, Koike, M, Miyazaki, Y, Kita, K, Crawford, J, Ko, M, Blake, DR, Kawakami, S, Shirai, T, Liley, B, Wang, Y, and Ogawa, T

Subjects
ozone, troposphere, western Pacific, Meteorology & Atmospheric Sciences
Abstract

Aircraft measurements of ozone (O3) and its precursors, including NO, CO, H2O, and nonmethane hydrocarbons (NMHCs), were made over the western Pacific in the 20° - 45°N latitude range in January and April-May 2002 during the Pacific Exploration of Asian Continental Emission (PEACE)-A and B campaigns. These measurements have provided data sets that, in combination with Transport and Chemical Evolution over the Pacific (TRACE-P) data taken in March 2001, enable studies of O3 photochemistry from winter to late spring. A photochemical box model is used to calculate ozone formation (F(O3)) and destruction (D(O3)) rates constrained by the observed species concentrations. The values of F(O3) and D(O3) are controlled directly by NO, J(O1D) (O3 photolysis frequency), H2O, OH, and HO2. Changes in HO2 concentration cause corresponding changes in both F(O3) and D(O3) leading to their coupling. Concentrations of these species, which are strongly influenced by photochemistry and transport from the Asian continent, underwent large seasonal variations. In the boundary layer (0-3 km), NO was much higher in January than in April-May, because of stronger winds, lower convective activities, and lower oxidation rates by OH in winter. The net O3 formation rate, given by P(O3) = F(O3) - D(O3), was largely positive in the boundary layer at 30°-45°N (1.5-4 ppbv d-1) in January, mainly because of high NO and low H2O values. Net O3 formation continued from January to the end of March, demonstrating that the western Pacific is an important O3 source region during this season. Net O3 formation nearly ceased by late April/May because of the decrease in NO and the increase in H2O. In the latitude range of 20°-30°N, P(O3) in the boundary layer was positive in January and turned negative by March. The earlier transition was mainly due to lower NO and higher H2O concentrations, combined with weaker transport and higher temperatures than those at 30°-45°N. The upper troposphere (6-12 km) has been shown to be a region of net O3 formation throughout most of the year because of high NO and low H2O. The present study illustrates that a decrease in the net O3 formation rate at 20°-45°N latitude from winter to late spring is explained systematically by the increases in J(O1D), H2O, OH, and HO2 (primarily due to increases in temperature and solar radiation) and the decrease in NO (primarily due to decrease in transport from the Asian continent). Differences in the seasonal variation of O3 photochemistry observed over the North American continent are interpreted in terms of the differences in factors controlling O3 formation and destruction. Copyright 2004 by the American Geophysical Union.

Published
2004

41. Removal of NOx and NOy in Asian outflow plumes: Aircraft measurements over the western Pacific in January 2002

Author

Takegawa, N, Kondo, Y, Koike, M, Chen, G, Machida, T, Watai, T, Blake, DR, Streets, DG, Woo, J‐H, Carmichael, GR, Kita, K, Miyazaki, Y, Shirai, T, Liley, JB, and Ogawa, T

Subjects
Climate Action, reactive nitrogen, removal process, Asian outflow, Meteorology & Atmospheric Sciences
Abstract

The Pacific Exploration of Asian Continental Emission Phase A (PEACE-A) aircraft measurement campaign was conducted over the western Pacific in January 2002. Correlations of carbon monoxide (CO) with carbon dioxide (CO2) and back trajectories are used to identify plumes strongly affected by Asian continental emissions. ΔCO/ΔCO2 ratios (i.e., linear regression slopes of CO-CO2) in the plumes generally fall within the variability range of the CO/CO2 emission ratios estimated from an emission inventory for east Asia, demonstrating the consistency between the aircraft measurements and the emission characterization. Removal rates of reactive nitrogen (NOx and NOy) for the study region (altitude

Published
2004

42. Asian chemical outflow to the Pacific in late spring observed during the PEACE‐B aircraft mission

Author

Oshima, N, Koike, M, Nakamura, H, Kondo, Y, Takegawa, N, Miyazaki, Y, Blake, DR, Shirai, T, Kita, K, Kawakami, S, and Ogawa, T

Subjects
Climate Action, transport, convection, chemical outflow, Meteorology & Atmospheric Sciences
Abstract

The Pacific Exploration of Asian Continental Emission phase B (PEACE-B) aircraft mission was conducted over the western Pacific during April-May 2002. During several flights large enhancements of CO greater than 200 parts per billion by volume (ppbv) were served at altitudes between 5 and 10 km. In this paper, we describe vertical transport mechanisms over east Asia that were responsible for these enhancements, using the European Centre for Medium-Range Weather Forecasts (ECMWF) meteorological data and infrared cloud data obtained by the Geostationary Meteorological Satellite (GMS)-5. A case study for the highest CO event shows that it was likely due to vertical transport of pollutants caused by deep cumulus convection along a quasi-stationary frontal zone, which was formed over central China (around the Yangtze River at 30°N). In the mean meteorological field during the PEACE-B period, the warm, moist low-level southerlies converged into the frontal zone, sustaining cross-frontal temperature and moisture contrasts. Along the frontal zone, the mean vertical motion was distinctively upward, and a subtropical jet aloft was found to transport uplifted air parcels efficiently into the western Pacific. In this study, criteria to identify deep convection are defined using both the ECMWF and GMS data. The results show that convective activity, which was generally high below the subtropical jet, played an important role in producing updrafts over central China. The convective transport resulted mainly from a limited number of episodes, each of which followed the development of a weak cyclonic disturbance. Back trajectories of air parcels sampled at altitudes between 4 and 13 km on board the aircraft during PEACE-B show that among the air parcels originating from the 800-hPa level or below, 69% were likely to have undergone convective uplifting. In addition to convection, sloping isentropes often observed along the quasi-stationary jet axis yielded persistent slow quasi-adiabatic uplifting of air over the Far East, which was occasionally intensified with a classical warm conveyor belt (WCB) airstream on the passage of migratory cyclonic disturbances. Meteorological conditions during PEACE-B were thus favorable for the upliffing of boundary layer air influenced by anthropogenic emissions over central China. These results are consistent with the relatively high levels of Halon 1211 (CF2ClBr), a good tracer of Chinese anthropogenic emissions, observed in the air parcels that were likely uplifted in the frontal zone. Coyright 2004 by the American Geophysical Union.

Published
2004

44. NMHCs and halocarbons in Asian continental outflow during the Transport and Chemical Evolution over the Pacific (TRACE-P) Field Campaign: Comparison with PEM-West B

Author

Blake, NJ, Blake, DR, Simpson, IJ, Meinardi, S, Swanson, AL, Lopez, JP, Katzenstein, AS, Barletta, B, Shirai, T, Atlas, E, Sachse, G, Avery, M, Vay, S, Fuelberg, HE, Kiley, CM, Kita, K, and Rowland, FS

Subjects
NMHCs, halocarbons, methyl bromide, methyl chloride, Halon-1211, Meteorology & Atmospheric Sciences
Published
2003

45. Photochemistry of ozone over the Western Pacific in Winter and Spring

Author

Kondo, Y, Chen, G, Hudman, R, Jacob, D, Koike, M, Nakamura, K, Takegawa, N, Kita, K, Miyazaki, Y, Blake, DR, Shirai, T, Kawakami, S, Takigawa, M, Akimoto, H, and Ogawa, T

Subjects
Geochemistry, Geology, Physical Geography and Environmental Geoscience, Geochemistry & Geophysics
Published
2003

49. Black carbon in aerosol during BIBLE B

Author

Liley, J Ben, Baumgardner, D, Kondo, Y, Kita, K, Blake, DR, Koike, M, Machida, T, Takegawa, N, Kawakami, S, Shirai, T, and Ogawa, T

Subjects
Earth Sciences, Atmospheric Sciences, Climate Action, black carbon, biomass burning, NHMC, Meteorology & Atmospheric Sciences
Published
2003

50. Effects of biomass burning and lightning on atmospheric chemistry over Australia and South-east Asia

Author

Kondo, Y, Takegawa, N, Miyazaki, Y, Ko, M, Koike, M, Kita, K, Kawakami, S, Shirai, T, Ogawa, T, Blake, DR, Liley, B, and Russell-Smith, J

Subjects
Forestry Sciences, Environmental Science and Management, Ecology, Forestry
Abstract

In situ aircraft measurements of trace gases and aerosols were made in the boundary layer (BL) and free troposphere (FT) over Indonesia and Australia during the Biomass Burning and Lightning Experiment (BIBLE)-A and B conducted in August-October 1998 and 1999. Concentrations of ozone (O3) and its precursors [CO, reactive nitrogen (NOx), non-methane hydrocarbons (NMHCs)] were measured in these campaigns to identify the sources of NOx and to estimate the effects of biomass burning and lightning on photochemical production of O3. Over Indonesia, in-situ production of NOx by lightning was found to be a major source of reactive nitrogen in the upper troposphere during BIBLE-A. In some circumstances, increases in reactive nitrogen were often associated with enhancements in CO and NMHCs, suggesting that the sources were biomass burning and fossil fuel combustion, followed by upward transport by cumulus convection. Over Australia the levels of O3, CO, reactive nitrogen, and NMHCs were elevated throughout the troposphere compared to those observed in the tropical Pacific. However, the mechanisms responsible for the enhanced concentrations in the BL and FT are distinctly different. The emissions from biomass burning that occurred in northern Australia were restricted to the BL because of strong subsidence in the period. In the FT over Australia, elevated concentrations of O3 and its precursors result from injections of emissions as the air masses travel over Africa, South America, the Indian Ocean, and Indonesia en route to Australia. In all cases, O3 levels in the biomass burning plumes were enhanced due to photochemical production.

Published
2003

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