研究者業績

中川 誠司

Nakagawa Seiji  (Seiji NAKAGAWA)

基本情報

所属
千葉大学 フロンティア医工学センター 教授
(兼任)大学院 工学研究院 教授
(兼任)大学院 融合理工学府 基幹工学専攻 医工学コース 教授,コース長
(兼任)工学部 総合工学科 医工学コース 教授,コース長
(兼任)医学部附属病院 教授
国立研究開発法人 産業技術総合研究所 客員研究員
東京大学 大学院医学系研究科 客員研究員
Univ. of Washington Visiting Scholar
国立研究開発法人 量子科学技術研究開発機構 客員研究員
学位
博士(工学)(1999年3月 東京大学)

連絡先
s.nakagawa99.alumni.u-tokyo.ac.jp
J-GLOBAL ID
200901063867675418
researchmap会員ID
5000005804

外部リンク

非侵襲的手法による神経生理計測(特に脳機能計測),心理計測,物理計測,さらにはコンピュータ・シミュレーションを駆使して,聴覚を中心とした知覚メカニズムや認知メカニズムの解明を進めています.また,知覚・認知メカニズム研究で得られた成果を利用することで,骨伝導補聴器や骨伝導スマートホンを初めとした福祉機器・医用機器の開発や,室内の視聴覚環境の最適化,騒音の快音化といった応用研究にも取り組んでいます.


論文

 312
  • Irwansyah, Sho Otsuka, Seiji Nakagawa
    Acoustical Science and Technology 2024年  
  • Irwansyah, Sho Otsuka, Seiji Nakagawa
    MethodsX 11 102394-102394 2023年12月  
    Bone conduction hearing aids (BCHAs) offer an alternative solution for individuals with outer or middle ear issues who cannot benefit from traditional air conduction hearing aids. However, the phenomenon of "crosstalk," where sound intended for one ear is mistakenly transmitted to the other ear through bone conduction, presents a challenge. This unintended transmission may limit the benefits of binaural hearing that can be achieved using two BCHAs, such as accurately detecting a sound source's direction. In this article, we present a method to suppress "crosstalk" within the human head using an adaptive algorithm to control two audiometric bone transducers. •Our method involves positioning an error sensor at a location considered close to the cochlea, such as the ear canal or the mastoid, and utilizing an adaptive algorithm to estimate the crosstalk compensation filter. This filter generates an anti-signal, which is then transmitted to one of the two transducers, effectively cancelling the crosstalk.•To verify whether the crosstalk cancellation reaches the cochlea in the inner ear, we provide a procedure for measuring hearing thresholds with and without crosstalk cancellation. This acts as a subjective measure of the efficacy of our crosstalk cancellation method. By leveraging an adaptive algorithm, this approach provides personalized cancellation and has the potential to enhance the performance of binaural BCHAs.
  • IRWANSYAH, Sho OTSUKA, Seiji NAKAGAWA
    INTER-NOISE and NOISE-CON Congress and Conference Proceedings 268(4) 4866-4873 2023年11月30日  
    This study aimed to address the issue of "crosstalk" in bone conduction hearing aids, where sound meant for one ear is mistakenly perceived by the other ear via bone conduction. We explored a potential solution by canceling the crosstalk sound at the cochlea. To achieve this, an accelerometer was placed on the mastoid to monitor the crosstalk sound produced by an audiometric bone transducer on the opposite side of the head, while a second transducer on the same side as the accelerometer was used to cancel it out. The filtered-x least mean square (FxLMS) algorithm was used to optimize the crosstalk compensation (CTC) filter for cancellation at the mastoid. Then, the subjects manually adjusted the filter coefficients through a lateralization task to achieve crosstalk cancellation at the cochlea. This task involved modifying phase and level differences between pure-tone sounds from the two transducers, making the sound seem to originate from the leftmost or rightmost side of the head. Our results indicated successful cancellation of crosstalk sound at the cochlea, as subjects' hearing thresholds under noise masking were lower with crosstalk cancellation.
  • Irwansyah Irwansyah, Sho Otsuka, Seiji Nakagawa
    超音波エレクトロニクスの基礎と応用に関するシンポジウム講演論文集 44 68 2023年11月13日  
  • Hajime Yano, Tetsuya Takiguchi, Seiji Nakagawa
    NeuroReport 35(1) 1-8 2023年10月30日  
    The impressions of heating, ventilation, and air conditioning (HVAC) sounds are important for the comfort people experience in their living spaces. Revealing neural substrates of the impressions induced by HVAC sounds can help to develop neurophysiological indices of the comfort of HVAC sounds. There have been numerous studies on the brain activities associated with the pleasantness of sounds, but few on the brain activities associated with the thermal impressions of HVAC sounds. Seven time-varying HVAC sounds were synthesized as stimuli using amplitude modulation. Six participants took part in subjective evaluation tests and MEG measurements. Subjective coolness of the HVAC sounds was measured using the paired comparison method. Magnetoencephalographic (MEG) measurements were carried out while participants listened to and compared the time-varying HVAC sounds. Time-frequency analysis and cluster-based analysis were performed on the MEG data. The subjective evaluation tests showed that the subjective coolness of the amplitude-modulated HVAC sounds was affected by the modulation frequency, and that there was individual difference in subjective coolness. A cluster-based analysis of the MEG data revealed that the brain activities of two participants significantly differed when they listened to cooler or less cool HVAC sounds. The frontal low-theta (4–5 Hz) and the temporal alpha (8–13 Hz) activities were observed. The frontal low-theta and the temporal alpha activities may be associated with the coolness of HVAC sound. This result suggests that the comfort level of HVAC sound can be evaluated and individually designed using neurophysiological measurements.

MISC

 985
  • Masashi Nakayama, Shunsuke Ishimitsu, Seiji Nakagawa
    2009 IEEE INTERNATIONAL CONFERENCE ON NETWORKING, SENSING AND CONTROL, VOLS 1 AND 2 848-+ 2009年  
    Speech-recognition rates decrease in noisy environments. The body-conducted speech, conducted in solids such as body and skins, has a noise-robust characteristics and can be served for recognition systems even in 98 -dBSPL (20 dBSNR) noise environments. However, the body-conduction can not capture high frequency sounds. Conventional methods to improve sound quality of body-conducted speeches need both speeches themselves and body-conducted speeches. In this paper, a new body-conducted speech retrieval technique in sound quality without a speech signal itself is proposed. First, high-frequency components in the body-conducted speech were emphasized using differential acceleration. Second, a conventional noise reduction method was adopted to make a clear body-conducted speech from a retrieval speech which contains constant noise. The recognition experiments using the proposed method showed that it improved recognition rate in all speakers.
  • 伊藤 一仁, 中川 誠司
    生体医工学 47(6) 588-594 2009年  
    To clarify mechanisms of the bone-conducted ultrasonic (BCU) perception, tympanic membrane (TM) vibrations under BCU stimuli were measured in a human subject using a laser Doppler vibrometer (LDV). We presented a signal processing algorithm to increase the SNRs (signal-to-noise ratios) of measured LDV signals by removing only optical noise components from the wave signals. Further, we analyzed the TM vibrations using the presented method to investigate the contribution of nonlinear distortion in the BCU perception, i. e. the possibility of generating the audible subharmonics. As a result, we did not find any audible signals corresponding to the subjective pitch of BCU in the TM vibrations. This suggests that there is no evidence for nonlinear distortion in the outer and middle ear.
  • 籠宮 隆之, 中川 誠司
    日本人間工学会大会講演集 45 184-185 2009年  
  • 岡安 唯, 西村 忠己, 山下 哲範, 柳井 修一, 中川 誠司, 吉田 悠加, 長谷 芳樹, 細井 裕司
    AUDIOLOGY JAPAN 52(5) 379-380 2009年  
  • 保手浜 拓也, 中川 誠司
    日本人間工学会大会講演集 45 186-187 2009年  
  • 中川 誠司
    日本人間工学会大会講演集 45 180-181 2009年  
  • 岡本 洋輔, 中川 誠司
    日本人間工学会大会講演集 45 164-165 2009年  
  • 伊藤 一仁, 中川 誠司
    日本人間工学会大会講演集 45 182-183 2009年  
  • 玉利雄祐, 小谷賢太郎, 朝尾隆文, 堀井健, 中川誠司
    日本人間工学会関西支部大会講演論文集 2008 59-62-62 2008年12月6日  
  • 保手浜 拓也, 中川 誠司
    聴覚研究会資料 38(6) 569-574 2008年10月17日  
  • Akiharu Nakagawa, Miyuki Tsushima, Kazuma Ando, Takeshi Bushimata, Yoon Kyung Choi, Tomoya Hirota, Mareki Honma, Hiroshi Imai, Kenzaburo Iwadate, Takaaki Jike, Seiji Kameno, Osamu Kameya, Ryuichi Kamohara, Yukitoshi Kan-ya, Noriyuki Kawaguchi, Masachika Kijima, Mi Kyoung Kim, Hideyuki Kobayashi, Seisuke Kuji, Tomoharu Kurayama, Toshihisa Maeda, Seiji Manabe, Kenta Maruyama, Makoto Matsui, Naoko Matsumoto, Takeshi Miyaji, Takumi Nagayama, Kayoko Nakamura, Daisuke Nyu, Chung Sik Oh, Toshihiro Omodaka, Tomoaki Oyama, Nicolas Pradel, Satoshi Sakai, Tetsuo Sasao, Katsuhisa Sato, Mayumi Sato, Katsunori M. Shibata, Hiroshi Suda, Yoshiaki Tamura, Kousuke Ueda, Yuji Ueno, Kazuyoshi Yamashita
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 60(5) 1013-1021 2008年10月  
    We present a distance measurement for the semiregular variable S Crateris (S Crt) based on its annual parallax. With the unique dual beam system of the VLBI Exploration for Radio Astrometry (VERA) telescopes, we measured the absolute proper motion of a water maser spot associated with S Crt, referred to the quasar J1147-0724 located at an angular separation of 1.degrees 23. In observations spanning nearly two years, we detected the maser spot at an LSR velocity of 34.7 km s(-1), for which we measured an annual parallax of 2.33 +/- 0.13 mas, corresponding to a distance of 430(-23)(+25) pc. This measurement has an accuracy one order of magnitude better than the parallax measurements of HIPPARCOS. The angular distribution and three-dimensional velocity fieI6 of maser spots indicate a bipolar outflow with the flow axis along the northeast-south west direction. Using the distance and photospheric temperature, we estimated the stellar radius of S Crt and compared it with those of Mira variables.
  • Tomoya Hirota, Kazuma Ando, Takeshi Bushimata, Yoon Kyung Choi, Mareki Honma, Hiroshi Imai, Kenzaburo Iwadate, Takaaki Jike, Seiji Kameno, Osamu Kameya, Ryuichi Kamohara, Yukitoshi Kan-ya, Noriyuki Kawaguchi, Masachika Kijima, Mi Kyoung Kim, Hideyuki Kobayashi, Seisuke Kuji, Tomoharu Kurayama, Seiji Manabe, Makoto Matsui, Naoko Matsumoto, Takeshi Miyaji, Atsushi Miyazaki, Takumi Nagayama, Akiharu Nakagawa, Daichi Namikawa, Daisuke Nyu, Chung Sik Oh, Toshihiro Omodaka, Tomoaki Oyama, Satoshi Sakai, Tetsuo Sasao, Katsuhisa Sato, Mayumi Sato, Katsunori M. Shibata, Yoshiaki Tamura, Kosuke Ueda, Kazuyoshi Yamashita
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 60(5) 961-974 2008年10月  
    We present results of multi-epoch VLBI observations with VERA (VLBI Exploration of Radio Astrometry) of the 22 GHz H2O masers associated with a young stellar object (YSO) IRAS22198+6336 in a dark cloud, L 1204 G. Based on phase-referencing VLBI astrometry, we derived an annual parallax of IRAS 22198+6336 to be 1.309 +/- 0.047 mas, corresponding to the distance of 764 27 pc from the Sun. Although the most principal error source of our astrometry is attributed to the internal structure of the maser spots, we successfully reduced the errors in the derived annual parallax by employing position measurements for all of the 26 detected maser spots. Based on this result, we reanalyzed the spectral energy distribution of IRAS 22198+6336 and found that the bolometric luminosity and total mass of IRAS 22198+6336 are 450 L-circle dot and 7 M-circle dot, respectively. These values are consistent with an intermediate-mass YSO deeply embedded in the dense dust core, which has been proposed to be an intermediate-mass counterpart of a low-mass Class 0 source. In addition, we obtained absolute proper motions of the H2O masers for the most blue-shifted components. We propose that the collimated jets aligned along the east-west direction are the most plausible explanation for the origin of the detected maser features.
  • Yoon Kyung Choi, Tomoya Hirota, Mareki Honma, Hideyuki Kobayashi, Takeshi Bushimata, Hiroshi Imai, Kenzaburo Iwadate, Takaaki Jike, Seiji Kameno, Osamu Kameya, Ryuichi Kamohara, Yukitoshi Kan-ya, Noriyuki Kawaguchi, Masachika Kijima, Mi Kyoung Kim, Seisuke Kuji, Tomoharu Kurayama, Seiji Manabe, Kenta Maruyama, Makoto Matsui, Naoko Matsumoto, Takeshi Miyaji, Takumi Nagayama, Akiharu Nakagawa, Kayoko Nakamura, Chung Sik Oh, Toshihiro Omodaka, Tomoaki Oyama, Satoshi Saka, Tetsuo Sasao, Katsuhisa Sato, Mayumi Sato, Katsunori M. Shibata, Yoshiaki Tamura, Miyuki Tsushima, Kazuyoshi Yamashita
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 60(5) 1007-1012 2008年10月  
    We report on astrometric observations of H2O masers around the red supergiant VY Canis Majoris carried out with VLBI Exploration of Radio Astrometry (VERA). Based on astrometric monitoring for 13 months, we successfully measured a trigonometric parallax of 0.88 +/- 0.08 mas, corresponding to a distance of 1.14(-0.09)(+0.11) kpc. This is the most accurate determined distance to VY CMa and the first one based on an annual parallax measurement. The luminosity of VY CMa has been overestimated due to a previously accepted distance. With our result, we re-estimated the luminosity of VY CMa to be (3 +/- 0.5) x 10(5) L-circle dot using the bolometric flux integrated over optical and IR wavelengths. This improved luminosity value makes the location of VY CMa on the Hertzsprung-Russell (HR) diagram much closer to the theoretically allowable zone (i.e. the left side of the Hayashi track) than previous ones, though the uncertainty in the effective temperature of the stellar surface still does not permit us to make a final conclusion.
  • Mayumi Sato, Tomoya Hirota, Mareki Honma, Hideyuki Kobayashi, Tetsuo Sasao, Takeshi Bushimata, Yoon Kyung Choi, Hiroshi Imai, Kenzaburo Iwadate, Takaaki Jike, Seiji Kameno, Osamu Kameya, Ryuichi Kamohara, Yukitoshi Kan-ya, Noriyuki Kawaguchi, Mi Kyoung Kim, Seisuke Kuji, Tomoharu Kurayama, Seiji Manabe, Makoto Matsui, Naoko Matsumoto, Takeshi Miyaji, Takumi Nagayama, Akiharu Nakagawa, Kayoko Nakamura, Chung Sik Oh, Toshihiro Omodaka, Tomoaki Oyama, Satoshi Sakai, Katsuhisa Sato, Katsunori M. Shibata, Yoshiaki Tamura, Kazuyoshi Yamashita
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 60(5) 975-989 2008年10月  
    We have used the Japanese VLBI array VERA to perform high-precision astrometry of an H2O maser source in the Galactic star-forming region NGC 281 West, which has been considered to be part of a 300-pc superbubble. We successfully detected a trigonometric parallax of 0.355 +/- 0.030 mas, corresponding to a source distance of 2.82 +/- 0.24 kpc. Our direct distance determination of NGC 281 has resolved a large distance discrepancy between previous photometric and kinematic studies; likely NGC 281 is in the far side of the Perseus spiral arm. The source distance as well as the absolute proper motions were used to demonstrate the 3D structure and expansion of the NGC 281, superbubble, similar to 650pc in size parallel to the Galactic disk and with a shape slightly elongated along the disk or spherical, but not vertically elongated, indicating that the superbubble expansion may be confined to the disk. We estimate the expansion velocity of the superbubble as being similar to 20 km s(-1), both perpendicular to and parallel to the Galactic disk with a consistent timescale of similar to 20 Myr.
  • 保手浜拓也, 保手浜拓也, 中川誠司
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.1-R-7-450 2008年9月3日  
  • 籠宮隆之, 中川誠司
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.1-R-22 2008年9月3日  
  • 中川誠司, 大久保裕子, 保手浜拓也, 神原文
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.1-R-5-524 2008年9月3日  
  • 伊藤一仁, 中川誠司
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.1-R-4 2008年9月3日  
  • 添田喜治, 下倉良太, 中川誠司
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.1-R-12 2008年9月3日  
  • 中川 誠司, 藤崎 恵美子, 岡本 洋輔
    情報科学技術フォーラム講演論文集 7(3) 51-53 2008年8月20日  
  • 中川誠司, 藤崎恵美子, 岡本洋輔
    情報科学技術フォーラム FIT 2008(3) 51-53-53 2008年8月20日  
  • 中山 仁史, 石光 俊介, 中川 誠司
    電子情報通信学会技術研究報告. SIP, 信号処理 108(71) 39-44 2008年5月30日  
    体内伝導音は固定伝播であるため,騒音の影響を受けにくい性質がある.この性質により,発声される音声よりも周囲の雑音が大きい環境下でも認識が可能とある.しかし,加速度ピックアップで抽出した体内伝導音はマイクロフォンで抽出した音声と比較して,高周波成分において周波数特性が悪く,こもった信号になる.このような理由から,明瞭な信号へ変換するための研究が行われてきた.従来の研究では目標となる音声信号などを必要としていた.そこで,本研究では目標となる音声信号などを用いずに体内伝導音のみで周波数特性を改善する方法を提案する.提案法は加速度差分と雑音除去手法を併用し,明瞭度の高い信号を推定することができた.最後に,音声から推定した音響モデルを用いた単語認識実験で単語認識率の改善が得られることも確認した.
  • 中山 仁史, 石光 俊介, 中川 誠司
    電子情報通信学会技術研究報告. EA, 応用音響 108(69) 39-44 2008年5月30日  
    体内伝導音は固定伝播であるため,騒音の影響を受けにくい性質がある.この性質により,発声される音声よりも周囲の雑音が大きい環境下でも認識が可能とある.しかし,加速度ピックアップで抽出した体内伝導音はマイクロフォンで抽出した音声と比較して,高周波成分において周波数特性が悪く,こもった信号になる.このような理由から,明瞭な信号へ変換するための研究が行われてきた.従来の研究では目標となる音声信号などを必要としていた.そこで,本研究では目標となる音声信号などを用いずに体内伝導音のみで周波数特性を改善する方法を提案する.提案法は加速度差分と雑音除去手法を併用し,明瞭度の高い信号を推定することができた.最後に,音声から推定した音響モデルを用いた単語認識実験で単語認識率の改善が得られることも確認した.
  • 中川誠司
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.2-9-10 2008年3月10日  
  • 中川誠司, 藤崎恵美子, 岡本洋輔
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.2-P-5 2008年3月10日  
  • 伊藤一仁, 中川誠司
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.2-P-6 2008年3月10日  
  • 保手浜拓也, 保手浜拓也, 中川誠司
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.2-9-11 2008年3月10日  
  • 中山仁史, 中山仁史, 石光俊介, 中川誠司
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.1-P-28 2008年3月10日  
  • 高見健治, 浅見敏彦, 石光俊介, 中川誠司
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.2-P-2 2008年3月10日  
  • 中川誠司, 萬谷惇, 萬谷惇
    日本音響学会研究発表会講演論文集(CD−ROM) 2008 ROMBUNNO.2-P-4 2008年3月10日  
  • 高見健治, 浅見敏彦, 石光俊介, 中川誠司
    日本機械学会中国四国支部総会・講演会講演論文集 46th 253-254-254 2008年2月26日  
  • 高見 健治, 浅見 敏彦, 石光 俊介, 中川 誠司
    中国四国支部総会・講演会 講演論文集 2008 253-254 2008年  
  • 高見 健治, 石光 俊介, 中川 誠司, 浅見 敏彦
    環境工学総合シンポジウム講演論文集 2008 105-108 2008年  
    The production concept of car engine sound has been changing from finding a solution to noise to designing sound. Although many studies have been conducted on creating comfortable car-engine sound, the psychoacoustic effects of time-varying rate for accelerating-engine sounds are still unclear. Thus, we investigated the effects of increasing the frequency rate of car interior noise on auditory impressions using psychological and neurophysiological methods. Harmonic complex tones that simulate acceleration noise were used as stimuli. First, subjective evaluations were examined using the semantic differential (SD) method. Second, neuronal activities of the auditory cortex evoked by these stimuli were measured by magnetoencephalography (MEG). The results indicated that has a significant effect on subjective impressions and on neuronal activities of the auditory cortex.
  • 添田喜治, 中川誠司
    日本生体磁気学会誌特別号 21(1) 66-67 2008年  
  • 高見健治, 石光俊介, 中川誠司, 浅見敏彦
    日本機械学会環境工学総合シンポジウム講演論文集 18th 105-108-108 2008年  
  • 岡本 洋輔, 中川 誠司
    照明学会 全国大会講演論文集 41 64-64 2008年  
    輝度が正弦波状に時間変化する点滅光刺激(正弦波パターン)を呈示した場合,その変化(ちらつき)に対する知覚感度は10 Hz付近にピークを持つ帯域通過型の周波数特性を示す.これは網膜レベルに存在する低域通過型とそれに続く高域通過型フィルタの影響によると考えられている.一方,複数の正弦波パターンを合成した刺激や,輝度変化を振幅変調した刺激(振幅変調パターン)に対しては,輝度の時間変化のエンベロープに対応した周期性が知覚される.このエンベロープ成分の知覚メカニズムに関して,網膜レベルでの非線形性によって生成された歪成分であるとする説が提案されているものの,否定的な意見も存在する.従来の研究においては,振幅変調パターンのキャリア周波数が高い場合にはエンベロープ周期の検出閾が上昇した.つまり,エンベロープ成分の知覚に低域通過型の周波数特性が見られることから,エンベロープ情報は網膜の低域通過型フィルタより後の視覚路で抽出されていると考えることができる.仮にエンベロープ成分が低域通過型と高域通過型フィルタの間で生じた歪成分であるとすると,エンベロープ知覚特性にはその後の高域通過型フィルタの影響が見られるはずである.一方,エンベロープ情報が高域通過型フィルタの後の視覚路で抽出されているならば,エンベロープ知覚特性は高域通過型フィルタの影響を受けないであろう.本研究では,脳磁界計測によって観察された大脳視覚野活動から,エンベロープ知覚特性とその神経生理メカニズムについて検討を行った.
  • 作山努, 小谷賢太郎, 堀井健, 中川誠司
    日本人間工学会関西支部大会講演論文集 2007 129-132-132 2007年12月1日  
  • 伊藤 一仁, 中川 誠司
    聴覚研究会資料 37(9) 737-742 2007年11月20日  
  • 中川 誠司
    聴覚研究会資料 37(8) 619-624 2007年10月19日  
  • 保手浜 拓也, 中川 誠司
    聴覚研究会資料 37(8) 613-618 2007年10月19日  
  • Yoshiharu Soeta, Seiji Nakagawa
    Huanan Ligong Daxue Xuebao/Journal of South China University of Technology (Natural Science) 35 80-83 2007年10月1日  
    Auditory evoked magnetic fields (AEFs) in relation to the factors extracted from autocorrelation function (ACF) and interaural cross-correlation function (IACF) were examined by magnetoencephalography (MEG). First, the effects of the peak amplitude of the ACF, φ 1 , on AEFs were examined. The strength of the pitch corresponded well to φ 1 . The amplitude of the Nlm, which was found above the left and right temporal lobes around 100 ms after the stimulus onset, increased with increasing φ 1 . The results suggest that stronger pitch sounds lead to an increase in the Nlm amplitude. Then, the effects of IACC and τ IACC on AEFs were examined. Human lateralization performance deteriorated with decreasing IACC. When the IACC was 0.95, the Nlm amplitudes increased with increasing τ IACC . However, the effect of τ IACC on the N1m amplitudes was not significant when the IACC was 0. 5. The results suggest that the lateralization performance is reflected in N1m amplitudes.
  • Tomoya Hirota, Takeshi Bushimata, Yoon Kyung Choi, Mareki Honma, Hiroshi Imai, Kenzaburo Iwadate, Takaaki Jike, Seiji Kameno, Osamu Kameya, Ryuichi Kamohara, Yukitoshi Kan-Ya, Noriyuki Kawaguchi, Masachika Kijima, Mi Kyoung Kim, Hideyuki Kobayashi, Seisuke Kuji, Tomoharu Kurayama, Seiji Manabe, Kenta Maruyama, Makoto Matsui, Naoko Matsumoto, Takeshi Miyaji, Takumi Nagayama, Akiharu Nakagawa, Kayoko Nakamura, Chung Sik Oh, Toshihiro Omodaka, Tomoaki Oyama, Satoshi Sakai, Tetsuo Sasao, Katsuhisa Sato, Mayumi Sato, Katsunori M. Shibata, Motonobu Shintani, Yoshiaki Tamura, Miyuki Tsushima, Kazuyoshi Yamashita
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 59(5) 897-903 2007年10月  
    We present the initial results of multiepoch VLBI observations of 22 GHz H2O masers in the Orion KL region with VERA (VLBI Exploration of Radio Astrometry). With the VERA dual-beam receiving system, we carried out phase-referencing VLBI astrometry, and successfully detected the annual parallax of Orion KL to be 2.29 +/- 0.10 mas, corresponding to a distance of 437 +/- 19 pc from the Sun. The distance to Orion KL was determined for the first time with the trigonometric parallax method in these observations. Although this value is consistent with that previously reported, 480 +/- 80 pc, which was estimated from a statistical parallax method using the proper motions and radial velocities of the H2O maser features, our new results provide a much more accurate value with an uncertainty of only 4%. In addition to the annual parallax, we detected an absolute proper motion of the maser feature, suggesting an outflow motion powered by the radio source I along with the systematic motion of source I itself.
  • Mareki Honma, Takeshi Bushimata, Yoon Kyung Choi, Tomoya Hirota, Hiroshi Imai, Kenzaburo Iwadate, Takaaki Jike, Osamu Kameya, Ryuichi Kamohara, Yukitoshi Kan-Ya, Noriyuki Kawaguchi, Masachika Kijima, Hideyuki Kobayashi, Seisuke Kuji, Tomoharu Kurayama, Seiji Manabe, Takeshi Miyaji, Takumi Nagayama, Akiharu Nakagawa, Chung Sik Oh, Toshihiro Omodaka, Tomoaki Oyama, Satoshi Sakai, Katsuhisa Sato, Tetsuo Sasao, Katsunori M. Shibata, Motonobu Shintani, Hiroshi Suda, Yoshiaki Tamura, Miyuki Tsushima, Kazuyoshi Yamashita
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 59(5) 889-895 2007年10月  
    We have performed high-precision astrometry of H2O maser sources in the Galactic star-forming region Sharpless 269 (S269) with VERA. We successfully detected a trigonometric parallax of 189 8 mu as, corresponding to a source distance of 5.2 8(-0.22)(+0.24) kpc. This is the smallest parallax ever measured, and the first one detected beyond 5 kpc. The source distance as well as the proper motions were used to constrain the outer rotation curve of the Galaxy, demonstrating that the difference of rotation velocities at the Sun and at S269 (which is 13.1 kpc away from the Galaxy's center) is less than 3%. This gives the strongest constraint on the flatness of the outer rotation curve, and provides a direct confirmation of the existence of a large amount of dark matter in the Galaxy's outer disk.
  • Takao Nakagawa, Keigo Enya, Masayuki Hirabayashi, Hidehiro Kaneda, Tsuneo Kii, Yoshiyuki Kimura, Toshio Matsumoto, Hiroshi Murakami, Masahide Murakami, Katsuhiro Narasaki, Masanao Narita, Akira Ohnishi, Shoji Tsunematsu, Seiji Yoshida
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 59 S377-S387 2007年10月  
    We describe the flight performance of the cryogenic system of the infrared astronomical satellite AKARI, which was successfully launched on 2006 February 21 (UT). AKARI carries a 68.5 cm telescope together with two focal-plane instruments, Infrared Cameras and Far Infrared Surveyor, all of which are cooled down to cryogenic temperature to achieve superior sensitivity. AKARI has a unique cryogenic system, which consists of cryogen (liquid helium) and mechanical coolers (2-stage Stirling coolers). With the help of mechanical coolers, 179 L (26.0 kg) of super-fluid liquid helium can keep the instruments cryogenically cooled for more than 500 days. The on-orbit performance of the AKARI cryogenics is consistent with the design and a pre-flight test, and the boil-off gas flow rate is as small as 0.32 mg s(-1). We observed an increase in the major axis of the AKARI orbit, which can be explained by thrust due to the thermal pressure of vented helium gas.
  • 中川 誠司
    生活支援工学系学会連合大会講演予稿集 5回 170-170 2007年10月  
  • 坂口敦, 坂口敦, 中川誠司, 藤坂洋一, 藤坂洋一, 阪口剛史, 渡辺好章
    日本音響学会研究発表会講演論文集(CD−ROM) 2007 2-Q-19 2007年9月12日  
  • 伊藤一仁, 中川誠司
    日本音響学会研究発表会講演論文集(CD−ROM) 2007 2-Q-14 2007年9月12日  

書籍等出版物

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担当経験のある科目(授業)

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共同研究・競争的資金等の研究課題

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