Treating palm oil mill effluent by activated sludge process using submerged mechanical aerator/agitator replacing surface aerator

Activated sludge process (ASP) is gaining recognition as a process technique for the control of biological oxygen demand (BOD) in palm oil mill effluent (POME). Surface aerators or diffusing plates are often used in aeration tanks serving as core of the ASP. For consistent improvement in water quality within the aeration tank utilising the ASP and in particular, mitigating its BOD effluent stream, this study replaced the surface aerator with submerged mechanical aerator/agitator incorporating separate “agitation function” and “agitation diffusing function” intended for use in aeration tank of polishing plant that contains surface aerators. In order to confirm the activated state of the sludge in the aeration tanks, sludge was observed by microscopy (magnification 600 or lower). The water analysis, POME, BOD, ammonium, and total nitrogen were analsyed. As a result of the study, improvement in water quality criteria including the agitation state in the aeration tank, mixed liquid dissolved oxygen, and BOD were observed. The BOD has improved from 34.7% to 93.1% at a maximum removal rate

Different Effects of Palmitoyl-L-carnitine and Palmitoyl-CoA on Mitochondrial Function in Rat Ventricular Myocytes

Although mitochondrial oxidative catabolism of fatty acid (FA) is a major energy source for the adult mammalian heart, cardiac lipotoxity resulting from elevated serum FA and enhanced FA use has been implicated in the pathogenesis of heart failure. To investigate the effects of the intermediates of FA metabolism, palmitoyl-L-carnitine (Pal-car) and palmitoyl-CoA (Pal-CoA), on mitochondrial function, we measured membrane potential(Δψm), opening of the mitochondrial permeability transition pore (mPTP) and the production of reactive oxygen species (ROS) in saponin-treated rat ventricular myocytes with a laser scanning confocal microscope. Our results revealed that: 1) lower concentrations of Pal-car (1 and 5μM) caused a slight hyperpolarization of Δψm (TMRE intensity increased to 115.5 ± 5.4 % and 110.7±1.6 % of the baseline, respectively. p<0.05) but did not open mPTP, 2) a higher concentration of Pal-car (10μM) depolarized Δψm (TMRE intensity decreased to 61.9 ± 12.2 % of the baseline, p<0.01) and opened mPTP (calcein intensity decreased to 70.7 ± 2.8% of the baseline, p<0.01), 3) Pal-CoA depolarized Δψm without opening mPTP, and 4) only the higher concentration of Pal-car (10μM) increased ROS generation (DCF intensity increased to 3.4 ± 0.3 fold of the baseline). We concluded that excessive exogenous intermediates of long chain saturated FA may disturb mitochondrial function in different ways between Pal-car and Pal-CoA. The distinct mechanisms of the deteriorating effects of long chain FA on mitochondrial function are important for our understanding of the development of cardiac diseases in systemic metabolic disorders.浜松医科大学学位論文　医博第517号(平成２０年１０月１７日

Could the mass media\u27s reporting control false rumor on Twitter during disasters?; A qualitative analysis of the Cosmo Oil rumor during the 2011 Great East Japan Earthquake

本研究では東日本大震災時のコスモ石油流言の発生・発展・消滅段階で、NHKなどのマスメディア報道がTwitter 上の災害流言の抑制にどの程度効果があったかを定性的に分析した。著者らは東日本大震災発生から1週間の約18万ツイートのデータから、流言に関する特徴的なツイートを目視で抽出して流言の文脈を解釈した。分析結果によれば、マスメディア報道は発生・発展段階では流言抑制に効果がなかったが、消滅段階ではある程度の効果があったと考えられる。災害時の事実ではないTwitter 流言を抑制するには、流言の発展段階でマスメディアが流言を特定し、人々が状況理解のために求めている情報を的確に発信することが有効と考えられる。This study examined the effectiveness of mass media reporting in controlling the spread of the Cosmo Oil Rumor on Twitter; at birth, adventures, and death stages, during the 2011 Great East Japan Earthquake. Authors manually extracted characteristic tweets and analyzed these texts, from over 180 thousand tweet data for the first week in the disaster. The result suggests that mass media reporting did not contribute to control the rumor at the birth and the development stages, and was effective to some extent at death stage. Mass media reporting will be effective to control false rumor via Twitter during disasters, when it provides right information which people need for understanding their environment at the developemnt stage

Coincidence analysis to search for inspiraling compact binaries using TAMA300 and LISM data

Japanese laser interferometric gravitational wave detectors, TAMA300 and LISM, performed a coincident observation during 2001. We perform a coincidence analysis to search for inspiraling compact binaries. The length of data used for the coincidence analysis is 275 hours when both TAMA300 and LISM detectors are operated simultaneously. TAMA300 and LISM data are analyzed by matched filtering, and candidates for gravitational wave events are obtained. If there is a true gravitational wave signal, it should appear in both data of detectors with consistent waveforms characterized by masses of stars, amplitude of the signal, the coalescence time and so on. We introduce a set of coincidence conditions of the parameters, and search for coincident events. This procedure reduces the number of fake events considerably, by a factor $\sim 10^{-4}$ compared with the number of fake events in single detector analysis. We find that the number of events after imposing the coincidence conditions is consistent with the number of accidental coincidences produced purely by noise. We thus find no evidence of gravitational wave signals. We obtain an upper limit of 0.046 /hours (CL $= 90$) to the Galactic event rate within 1kpc from the Earth. The method used in this paper can be applied straightforwardly to the case of coincidence observations with more than two detectors with arbitrary arm directions.Comment: 28 pages, 17 figures, Replaced with the version to be published in Physical Review

Results of the search for inspiraling compact star binaries from TAMA300's observation in 2000-2004

We analyze the data of TAMA300 detector to search for gravitational waves from inspiraling compact star binaries with masses of the component stars in the range 1-3Msolar. In this analysis, 2705 hours of data, taken during the years 2000-2004, are used for the event search. We combine the results of different observation runs, and obtained a single upper limit on the rate of the coalescence of compact binaries in our Galaxy of 20 per year at a 90% confidence level. In this upper limit, the effect of various systematic errors such like the uncertainty of the background estimation and the calibration of the detector's sensitivity are included.Comment: 8 pages, 4 Postscript figures, uses revtex4.sty The author list was correcte

The Japanese space gravitational wave antenna; DECIGO

DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. DECIGO is expected to open a new window of observation for gravitational wave astronomy especially between 0.1 Hz and 10 Hz, revealing various mysteries of the universe such as dark energy, formation mechanism of supermassive black holes, and inflation of the universe. The pre-conceptual design of DECIGO consists of three drag-free spacecraft, whose relative displacements are measured by a differential Fabry– Perot Michelson interferometer. We plan to launch two missions, DECIGO pathfinder and pre- DECIGO first and finally DECIGO in 2024

DECIGO pathfinder

DECIGO pathfinder (DPF) is a milestone satellite mission for DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) which is a future space gravitational wave antenna. DECIGO is expected to provide us fruitful insights into the universe, in particular about dark energy, a formation mechanism of supermassive black holes, and the inflation of the universe. Since DECIGO will be an extremely large mission which will formed by three drag-free spacecraft with 1000m separation, it is significant to gain the technical feasibility of DECIGO before its planned launch in 2024. Thus, we are planning to launch two milestone missions: DPF and pre-DECIGO. The conceptual design and current status of the first milestone mission, DPF, are reviewed in this article

Observation results by the TAMA300 detector on gravitational wave bursts from stellar-core collapses

We present data-analysis schemes and results of observations with the TAMA300 gravitational-wave detector, targeting burst signals from stellar-core collapse events. In analyses for burst gravitational waves, the detection and fake-reduction schemes are different from well-investigated ones for a chirp-wave analysis, because precise waveform templates are not available. We used an excess-power filter for the extraction of gravitational-wave candidates, and developed two methods for the reduction of fake events caused by non-stationary noises of the detector. These analysis schemes were applied to real data from the TAMA300 interferometric gravitational wave detector. As a result, fake events were reduced by a factor of about 1000 in the best cases. The resultant event candidates were interpreted from an astronomical viewpoint. We set an upper limit of 2.2x10^3 events/sec on the burst gravitational-wave event rate in our Galaxy with a confidence level of 90%. This work sets a milestone and prospects on the search for burst gravitational waves, by establishing an analysis scheme for the observation data from an interferometric gravitational wave detector

The status of DECIGO

DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and cosmologically significant sources mainly between 0.1 Hz and 10 Hz and thus to open a new window for gravitational wave astronomy and for the universe. DECIGO will consists of three drag-free spacecraft arranged in an equilateral triangle with 1000 km arm lengths whose relative displacements are measured by a differential Fabry-Perot interferometer, and four units of triangular Fabry-Perot interferometers are arranged on heliocentric orbit around the sun. DECIGO is vary ambitious mission, we plan to launch DECIGO in era of 2030s after precursor satellite mission, B-DECIGO. B-DECIGO is essentially smaller version of DECIGO: B-DECIGO consists of three spacecraft arranged in an triangle with 100 km arm lengths orbiting 2000 km above the surface of the earth. It is hoped that the launch date will be late 2020s for the present