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Journal articles on the topic 'Transit method'

Author: Grafiati

Published: 4 June 2021

Last updated: 25 July 2025

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1

Windemuth, Diana, Eric Agol, Josh Carter, et al. "An automated method to detect transiting circumbinary planets." Monthly Notices of the Royal Astronomical Society 490, no. 1 (2019): 1313–24. http://dx.doi.org/10.1093/mnras/stz2637.

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ABSTRACT To date a dozen transiting ‘Tatooines’ or circumbinary planets (CBPs) have been discovered, by eye, in the data from the Kepler mission; by contrast, thousands of confirmed circumstellar planets orbiting around single stars have been detected using automated algorithms. Automated detection of CBPs is challenging because their transits are strongly aperiodic with irregular profiles. Here, we describe an efficient and automated technique for detecting circumbinary planets that transit their binary hosts in Kepler light curves. Our method accounts for large transit timing variations (TTV

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Jin, Haitao, Fengjun Jin, Jiao’e Wang, Wei Sun, and Libo Dong. "Competition and Cooperation between Shared Bicycles and Public Transit: A Case Study of Beijing." Sustainability 11, no. 5 (2019): 1323. http://dx.doi.org/10.3390/su11051323.

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As an eco-friendly transportation mode, shared bicycles provide a new option for public transit users in urban areas. China’s bicycle-sharing market began flourishing in July 2016 and reached a plateau in 2017. How shared bicycles influenced public transit systems during this period is an interesting topic. A case study of Beijing is conducted. This study aims to identify the competitive and cooperative influences of shared bicycles on public transit by exploring the changes in public transit trip distances before and after the upsurge in bicycle-sharing. A histogram shifting method is introdu

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Li, Teng, and Eryu Zhu. "Quantifying Carbon Emissions Generated by Monorail Transits: A Life Cycle Assessment Approach." Computational Intelligence and Neuroscience 2022 (March 24, 2022): 1–15. http://dx.doi.org/10.1155/2022/3872069.

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The use of rail transits results in the generation of a large amount of carbon emissions. Throughout the life cycle of a rail transit system, huge amounts of carbon are emitted, which contributes to the threat posed by carbon emission on the city ecosystem. Despite the many methods previously proposed to quantify carbon emissions from rail transit systems, a method that can be applied to measure carbon emissions of monorail systems is yet to be developed. We have used the life cycle assessment (LCA) method to propose a method that can be used to quantify carbon emissions from monorail transits

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Gilbert, Gregory J. "Accurate Modeling of Grazing Transits Using Umbrella Sampling." Astronomical Journal 163, no. 3 (2022): 111. http://dx.doi.org/10.3847/1538-3881/ac45f4.

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Abstract Grazing transits present a special problem for statistical studies of exoplanets. Even though grazing planetary orbits are rare (due to geometric selection effects), for many low to moderate signal-to-noise ratio cases, a significant fraction of the posterior distribution is nonetheless consistent with a grazing geometry. A failure to accurately model grazing transits can therefore lead to biased inferences even for cases where the planet is not actually on a grazing trajectory. With recent advances in stellar characterization, the limiting factor for many scientific applications is n

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Carpintero, D. D., and M. Melita. "An alternative stable solution for the Kepler-419 system, obtained with the use of a genetic algorithm." Astronomy & Astrophysics 620 (November 30, 2018): A88. http://dx.doi.org/10.1051/0004-6361/201731997.

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Context. The mid-transit times of an exoplanet may be nonperiodic. The variations in the timing of the transits with respect to a single period, that is, the transit timing variations (TTVs), can sometimes be attributed to perturbations by other exoplanets present in the system, which may or may not transit the star. Aims. Our aim is to compute the mass and the six orbital elements of an nontransiting exoplanet, given only the central times of transit of the transiting body. We also aim to recover the mass of the star and the mass and orbital elements of the transiting exoplanet, suitably modi

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Liu, Xinyao, Xinqing Hao, and Yuzhu Sun. "Determining the Presence of Transits of the Three Known Companions of Proxima Centauri." Theoretical and Natural Science 107, no. 1 (2025): 243–51. https://doi.org/10.54254/2753-8818/2025.22743.

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Upon analyzing TESS data, we searched through 4 months of photometric observations of Proxima Centauri, focusing on Proxima b s 1.5% geometric transit probability. Our primary attention was directed towards four key lightcurves, each with 120-second exposures, as processed by SPOC. To minimize uncertainties from instrumental noise and stellar flares, we implemented some advanced data processing techniques. Searching for transits, we zeroed in on times corresponding to integral multiples of Proxima Centauri b's known 11.2-day period. To evaluate our sensitivity, we injected synthetic transits a

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Kipping, David. "Transit origami: a method to coherently fold exomoon transits in time series photometry." Monthly Notices of the Royal Astronomical Society 507, no. 3 (2021): 4120–31. http://dx.doi.org/10.1093/mnras/stab2013.

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ABSTRACT One of the simplest ways to identify an exoplanetary transit is to phase fold a photometric time series upon a trial period – leading to a coherent stack when using the correct value. Such phase-folded transits have become a standard data visualization in modern transit discovery papers. There is no analogous folding mechanism for exomoons, which would have to represent some kind of double fold: once for the planet and then another for the moon. Folding with the planet term only, a moon imparts a small decrease in the surrounding out-of-transit averaged intensity, but its incoherent n

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Zhao, Fang, Lee-Fang Chow, Min-Tang Li, Ike Ubaka, and Albert Gan. "Forecasting Transit Walk Accessibility: Regression Model Alternative to Buffer Method." Transportation Research Record: Journal of the Transportation Research Board 1835, no. 1 (2003): 34–41. http://dx.doi.org/10.3141/1835-05.

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A description is given of a methodology for estimating transit walk accessibility at the home end of transit trips and for forecasting transit walk accessibility at the home end for a future year, given forecast population and employment data, transit route information, and type of street configuration. The methodology for estimating transit walk accessibility overcomes the problems associated with natural and man-made barriers such as water bodies and community walls and the problem of uneven distribution of population. A comparison of the results with those from the traditional buffer method

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9

Heller, René, and Michael Hippke. "Signal preservation of exomoon transits during light curve folding." Astronomy & Astrophysics 657 (January 2022): A119. http://dx.doi.org/10.1051/0004-6361/202142403.

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In the search for moons around extrasolar planets (exomoons), astronomers are confronted with a stunning observation. Although 3400 of the 4500 exoplanets were discovered with the transit method and although there are well over 25 times as many moons than planets known in the Solar System (two of which are larger than Mercury), no exomoon has been discovered to date. In the search for exoplanet transits, stellar light curves are usually phase-folded over a range of trial epochs and periods. This approach, however, is not applicable in a straightforward manner to exomoons. Planet-moon transits

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10

Dong, Kailing. "Analysis of Urban Rail Transit Station Planning Combining Simulated Annealing Algorithm." Discrete Dynamics in Nature and Society 2022 (March 7, 2022): 1–8. http://dx.doi.org/10.1155/2022/3941554.

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As a crucial node in the network system of urban transportation infrastructure, the consistent planning of the urban rail transit stations scientifically and reasonably is of highly significant importance to have a thorough understanding of the functional area division of a city and assess the improvement of facilities correlated with the rail transit infrastructure. In this study, the simulated annealing algorithm (SAA) is applied to the data analysis of the rail transit stations in a city. The method for the analysis of the urban rail transit stations combined with the SAA can achieve the di

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11

Szabó, Gyula M., A. E. Simon, Laszlo L. Kiss, and Zsolt Regály. "Practical suggestions on detecting exomoons in exoplanet transit light curves." Proceedings of the International Astronomical Union 6, S276 (2010): 556–57. http://dx.doi.org/10.1017/s174392131102120x.

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AbstractThe number of known transiting exoplanets is rapidly increasing, which has recently inspired significant interest as to whether they can host a detectable moon. Although there has been no such example where the presence of a satellite was proven, several methods have already been investigated for such a detection in the future. All these methods utilize post-processing of the measured light curves, and the presence of the moon is decided by the distribution of a timing parameter. Here we propose a method for the detection of the moon directly in the raw transit light curves. When the m

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12

Bryson, Steve, and Michelle Kunimoto. "Transit-APP: A Centroid-free Method of Identifying Background Transit False Positives." Research Notes of the AAS 9, no. 4 (2025): 81. https://doi.org/10.3847/2515-5172/adcb3a.

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Abstract We present a centroid-free method to identify which star is the source of a known transit signal from pixel data. This method is based on observed and simulated difference images, and provides a relative probability of a star being the source of the transit compared to other known stars. This method is robust at low S/N compared to common centroid-based methods, and is well suited for space-based transit surveys such as Kepler and TESS.

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Novaes, Antonio G. N. "RAPID-TRANSIT EFFICIENCY ANALYSIS WITH THE ASSURANCE-REGION DEA METHOD." Pesquisa Operacional 21, no. 2 (2001): 179–97. http://dx.doi.org/10.1590/s0101-74382001000200004.

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Rapid-transit services are a relevant part of the transportation network in most cities of the world. An important aspect of transport policy is the supply of public urban transportation. In particular, it is of interest to determine whether rapid-transit operators are working in a technically and scale-efficient way. Production analysis of transit services has been characterized by the econometric study of average practice technologies. A more recent method to study such production frontiers is Data Envelopment Analysis (DEA). It is a non-parametric method, but its application to rapid-transi

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Yang, Jingxuan. "Fine calculation method for carbon emission of urban rail transit." E3S Web of Conferences 528 (2024): 03005. http://dx.doi.org/10.1051/e3sconf/202452803005.

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As an important part of modern integrated transportation system, urban rail transit generates carbon emissions mainly by consuming electric energy. Aiming at the problems such as single index and weak accuracy of the current carbon emissions accounting method for urban rail transit, this study builds a refined carbon emissions calculation model based on existing industry standards and norms, puts forward refined carbon emissions calculation factors under different conditions, and designs efficient algorithms to solve them. The research hopes to provide a basis for differentiated policy formula

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Fatheddin, Hossein, and Sedighe Sajadian. "Singular Spectrum Analysis of Exoplanetary Transits." Astronomical Journal 168, no. 2 (2024): 71. http://dx.doi.org/10.3847/1538-3881/ad582f.

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Abstract Transit photometry is currently the most efficient and sensitive method for detecting extrasolar planets (exoplanets) and a large majority of confirmed exoplanets have been detected with this method. The substantial success of space-based missions such as NASA’s Kepler/K2 and Transiting Exoplanet Survey Satellite has generated a large and diverse sample of confirmed and candidate exoplanets. Singular spectrum analysis (SSA) provides a useful tool for studying photometric time series and exoplanetary transits. SSA is a technique for decomposing a time series into a sum of its main comp

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Armstrong, David, David V. Martin, and Don Pollacco. "Detecting Circumbinary Exoplanets: Understanding Transit Timing." Proceedings of the International Astronomical Union 8, S299 (2013): 273–74. http://dx.doi.org/10.1017/s1743921313008557.

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AbstractWe have derived and tested a simple analytical model for placing limits on the transit timing variations of circumbinary exoplanets. These are generally of days in magnitude, dwarfing those found in multi-planet systems. The derived method is fast, efficient and is accurate to approximately 1% in predicting limits on the possible times of transits over a 3-year campaign.

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17

Zimmer, T., J. B. Duluc, and N. Lewis. "Method for BJT transit time evaluation." Electronics Letters 34, no. 20 (1998): 1979. http://dx.doi.org/10.1049/el:19981219.

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An, Shi, Lei Wang, Haiqiang Yang, and Jian Wang. "Discovering Public Transit Riders’ Travel Pattern from GPS Data: A Case Study in Harbin." Journal of Sensors 2017 (2017): 1–8. http://dx.doi.org/10.1155/2017/5290795.

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This paper proposes a public transit riders’ travel pattern measuring method based on divided cells and public transit vehicle’s GPS data. The method consists of two parts: detecting urban origin and destination areas and measuring the public transit riders’ travel pattern. Moreover, a series of indicators are proposed to reflect the public transit riders’ travel pattern. A case study is carried out to evaluate the methods, which use the GPS data collected from taxis and buses in Harbin, China. The study is expected to provide a better understanding of public transit riders’ travel patterns.

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Panwar, Vatsal, Jean-Michel Désert, Kamen O. Todorov, et al. "A new method to measure the spectra of transiting exoplanet atmospheres using multi-object spectroscopy." Monthly Notices of the Royal Astronomical Society 510, no. 3 (2021): 3236–65. http://dx.doi.org/10.1093/mnras/stab3646.

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ABSTRACT Traditionally, ground-based spectrophotometric observations probing transiting exoplanet atmospheres have employed a linear map between comparison and target star light curves (e.g. via differential spectrophotometry) to correct for systematics contaminating the transit signal. As an alternative to this conventional method, we introduce a new Gaussian Processes (GP) regression-based method to analyse ground-based spectrophotometric data. Our new method allows for a generalized non-linear mapping between the target transit light curves and the time-series used to detrend them. This rep

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Fidanoğlu, Akif, and Ilgın Gökaşar. "A Method for Public Transit OD Estimation Using Transit Smart Card Data." Journal of Transportation and Logistics 7, no. 2 (2022): 479–88. http://dx.doi.org/10.26650/jtl.2022.1192128.

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21

Schiszler, Istvan, Minoru Tomita, Yasuo Fukuuchi, Norio Tanahashi, and Koji Inoue. "New optical method for analyzing cortical blood flow heterogeneity in small animals: validation of the method." American Journal of Physiology-Heart and Circulatory Physiology 279, no. 3 (2000): H1291—H1298. http://dx.doi.org/10.1152/ajpheart.2000.279.3.h1291.

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In pentobarbital-anesthetized male Sprague-Dawley rats, a small cranial window was trephined, and the cortex was transilluminated with a fine glass fiber inserted into the brain parenchyma. The light intensity at the surface area of 2 × 2 mm was recorded during intracarotid injection of 25 μl of carbon black (CB) solution. The region of interest (ROI) was divided into a 50 × 50 matrix, and the mean transit time of CB transport was calculated in each matrix element. We found rapid transits of CB along the microvasculature, with considerable heterogeneity in the avascular area, and heterogeneous

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22

Kostogryz, Nadia M., Taras M. Yakobchuk, Olexandr V. Morozhenko, and Anatolij P. Vidmachenko. "Polarization of the transiting planetary system of the K dwarf HD 189733." Proceedings of the International Astronomical Union 6, S276 (2010): 480–81. http://dx.doi.org/10.1017/s1743921311020886.

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AbstractWe model the polarization in the system HD 189733 resulting from the planetary transit. This system has a short-period (2.2d) Jupiter-like planet with the radii ratio Rp/R* = 0.148, orbiting at the distance of 0.031 AU around the star.We calculated the polarization of the system HD189733 to be 0.022% at the limb, which is consistent with the recent observational data. We suggest the shapes of the polarization parameters curves to be used for deriving the planet orbit inclination at the near limb transits as an alternative to standard transit method.

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Fang, Wenlong. "Comparisons of Detection Paradigm of Planet: Transit and Radial Velocity." Highlights in Science, Engineering and Technology 38 (March 16, 2023): 226–34. http://dx.doi.org/10.54097/hset.v38i.5811.

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The transit and radial velocity method are two most widely used approach in exoplanet detection. This paper compares the advantages and disadvantages of two methods based on the characteristics of planets they found and different calculation results. Different distribution of parameters brings the preference for two methods. In detail, the radial velocity method discovered more gigantic planets while still have most planets with smaller size like that of the transit method. The minimum and maximum of orbital period are all relatively lower for transit method. Significant difference in the comp

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Rodenbeck, Kai, René Heller, Michael Hippke, and Laurent Gizon. "Revisiting the exomoon candidate signal around Kepler-1625 b." Astronomy & Astrophysics 617 (September 2018): A49. http://dx.doi.org/10.1051/0004-6361/201833085.

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Context. Transit photometry of the Jupiter-sized exoplanet candidate Kepler-1625 b has recently been interpreted as showing hints of a moon. This exomoon, the first of its kind, would be as large as Neptune and unlike any moon we know from the solar system. Aims. We aim to clarify whether the exomoon-like signal is indeed caused by a large object in orbit around Kepler-1625 b, or whether it is caused by stellar or instrumental noise or by the data detrending procedure. Methods. To prepare the transit data for model fitting, we explore several detrending procedures using second-, third-, and fo

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Robnik, Jakob, and Uroš Seljak. "Matched filtering with non-Gaussian noise for planet transit detections." Monthly Notices of the Royal Astronomical Society 504, no. 4 (2021): 5829–39. http://dx.doi.org/10.1093/mnras/stab1178.

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ABSTRACT We develop a method for planet detection in transit data, which is based on the matched filter technique, combined with the Gaussianization of the noise outliers. The method is based on Fourier transforms and is as fast as the existing methods for planet searches. The Gaussianized matched filter (GMF) method significantly outperforms the standard baseline methods in terms of the false positive rate, enabling planet detections at up to 30 per cent lower transit amplitudes. Moreover, the method extracts all the main planet transit parameters, amplitude, period, phase, and duration. By c

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Tan, Xiao Yu, Jin Li, and Wen Deng. "Signal Strategy of Conditional Transit Priority Based on Transit Schedule." Advanced Materials Research 156-157 (October 2010): 298–302. http://dx.doi.org/10.4028/www.scientific.net/amr.156-157.298.

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Combined with the actual situation of China, drawing on foreign models based on the quantitative methods, this paper gets a model based on conditional bus priority for signal timing design which is combined with the traditional model through the application of conditional bus priority. The model considers more about the actual situation of the intersection, as well as a variety of other general vehicles which also need to pass through the intersection; it is a more moderate, harmonious, and better public transport priority method which does not use at the expense of other general vehicles.

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Hou, Bowen, Yang Cao, Dongye Lv, and Shuzhi Zhao. "Transit-Based Evacuation for Urban Rail Transit Line Emergency." Sustainability 12, no. 9 (2020): 3919. http://dx.doi.org/10.3390/su12093919.

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Urban rail systems are the backbone of urban transit networks and are characterized by large passenger volumes, high speeds, punctuality, and low environmental impacts. However, unforeseen events such as rail transit line emergencies can lead to unexpected costs and delays. As a means of disruption management, we divide the decision support system for urban rail transit line emergency situations into two stages—transit-based evacuation and bus bridging management. This paper focuses on the transit-based evacuation under emergency scenarios on a single rail line. The model determines the vehicl

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Asnicar, Francesco, Emily R. Leeming, Eirini Dimidi, et al. "Blue poo: impact of gut transit time on the gut microbiome using a novel marker." Gut 70, no. 9 (2021): 1665–74. http://dx.doi.org/10.1136/gutjnl-2020-323877.

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Background and aimsGut transit time is a key modulator of host–microbiome interactions, yet this is often overlooked, partly because reliable methods are typically expensive or burdensome. The aim of this single-arm, single-blinded intervention study is to assess (1) the relationship between gut transit time and the human gut microbiome, and (2) the utility of the ‘blue dye’ method as an inexpensive and scalable technique to measure transit time.MethodsWe assessed interactions between the taxonomic and functional potential profiles of the gut microbiome (profiled via shotgun metagenomic sequen

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Kálmán, Szilárd, Gyula M. Szabó, and Csaba Kiss. "Exocomet Models in Transit: Light Curve Morphology in the Optical—Near Infrared Wavelength Range." Publications of the Astronomical Society of the Pacific 136, no. 8 (2024): 084401. http://dx.doi.org/10.1088/1538-3873/ad4fe3.

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Abstract Following the widespread practice of exoplanetary transit simulations, various presumed components of an extrasolar system can be examined in numerically simulated transits, including exomoons, rings around planets, and the deformation of exoplanets. Template signals can then be used to efficiently search for light curve features that mark specific phenomena in the data, and they also provide a basis for feasibility studies of instruments and search programs. In this paper, we present a method for exocomet transit light curve calculations using arbitrary dust distributions in transit.

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Wu, Zixiao, Bo Shen, and Dawei Lv. "Study on the Transit Network Evaluation Method Based on the Transit Ridership Model." Procedia - Social and Behavioral Sciences 43 (2012): 428–34. http://dx.doi.org/10.1016/j.sbspro.2012.04.116.

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Xie, Wenbin, Costantino Sigismondi, Xiaofan Wang, and Paolo Tanga. "Venus transit, aureole and solar diameter." Proceedings of the International Astronomical Union 8, S294 (2012): 485–86. http://dx.doi.org/10.1017/s1743921313002986.

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AbstractThe possibility to measure the solar diameter using the transits of Mercury has been exploited to investigate the past three centuries of its evolution and to calibrate these measurements made with satellites. This measurement basically consists to compare the ephemerides of the internal contact timings with the observed timings. The transits of Venus of 2004 and 2012 gave the possibility to apply this method, involving a planet with atmosphere, with the refraction of solar light through it creating a luminous arc all around the disk of the planet. The observations of the 2012 transit

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Nikolov, N., J. Koppenhoefer, M. Lendl, T. Henning, and J. Greiner. "Multiband Transit Light Curve Modeling of WASP-4." Proceedings of the International Astronomical Union 7, S282 (2011): 141–42. http://dx.doi.org/10.1017/s1743921311027220.

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AbstractWe report on the simultaneous g′,r′,i′,z′ multiband, high time sampling (18-24s) ground-based photometric observations, which we use to measure the planetary radius and orbital inclination of the extrasolar transiting hot Jupiter WASP-4b. We recorded 987 images during three complete transits with the GROND instrument, mounted on the MPG/ESO-2.2m telescope at La Silla Observatory. Assuming a quadratic law for the stellar limb darkening we derive system parameters by fitting a composite transit light curve over all bandpasses simultaneously. To compute uncertainties of the fitted paramet

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Ma, Xi Qin, Chang Qi Yang, and Guang Sheng Ren. "A Novel Evaluation Method for Overall Performance Testing of Rail Transit Brake System." Advanced Materials Research 156-157 (October 2010): 113–16. http://dx.doi.org/10.4028/www.scientific.net/amr.156-157.113.

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A system is developed to detect output pressure of rail transit brake system and the principle of the system design is expatiated. The function and the implement method of each block in the system are also discussed. According to the problems existed in detection of rail transit brake system, we propose a new evaluation index to detect overall performance of rail transit brake system.

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Chen, Rui, Tunan Zhang, and Bolin Lin. "A Search for Transiting Doppler-Detected Exoplanets." Theoretical and Natural Science 107, no. 1 (2025): 252–69. https://doi.org/10.54254/2753-8818/2025.22740.

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There have been indefatigable pursuits of exoplanets and their host stars, spanning from the first ever discovery of exoplanets in 1992 to today. Many researchers have analysed data in hope of detecting new planets, or to obtain more information regarding the host stars. Here, we present a search for transits of exoplanets in samples of stars with the following criteria: near Earth - within 50 parsecs, and has a planet/planets confirmed via methods other than the transit method. Using recent data from NASA's Transiting Exoplanet Survey Satellite (TESS), we were able to conduct analysis on data

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Xin, Xin, Yao Wu, Yan Yong Guo, and Ti Song. "Study on the Reasonable Scale of the Urban Rail Transit Network: A Case of Xi'an City." Applied Mechanics and Materials 253-255 (December 2012): 1829–32. http://dx.doi.org/10.4028/www.scientific.net/amm.253-255.1829.

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In order to determine a reasonable scale of rail transit network in Xi'an, four influencing factors are analyzed. Based on the introduction of three indicators of rail transit network scale and the network density index, a method of rail transit network scale is proposed. Also, the determination method of parameters is given. The method is used to forecast the rail transit network scale with the actual situation of Xi'an. The result shows that the scale of Xi'an rail transit network is about 550km.

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Kovacs, Geza. "More planetary candidates from K2 Campaign 5 using TRAN_K2." Astronomy & Astrophysics 643 (November 2020): A169. http://dx.doi.org/10.1051/0004-6361/202038726.

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Context. The exquisite precision of space-based photometric surveys and the unavoidable presence of instrumental systematics and intrinsic stellar variability call for the development of sophisticated methods that distinguish these signal components from those caused by planetary transits. Aims. Here, we introduce the standalone Fortran code TRAN_K2 to search for planetary transits under the colored noise of stellar variability and instrumental effects. We use this code to perform a survey to uncover new candidates. Methods. Stellar variability is represented by a Fourier series and, when nece

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Kolin, Aleksey V., Pavel V. Rybakov, Pavel A. Krasilnikov, and Liliya R. Aysina. "Calculation of self-cost of transportation work on ground urban transit using the unit expense rate method." International Journal of Advanced Studies 15, no. 1 (2025): 22–46. https://doi.org/10.12731/2227-930x-2025-15-1-326.

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The article describes possibility of using the method of unit expense rates to calculate the urban transit self-cost and evaluating the quality of economic operations at urban transit operators. Purpose. The article examines optimization possibilities of the amount of operating costs determining procedure and the self-cost of transportation at urban ground transit operators. Article proposes a methodology that allows increasing the veracity of calculations, while simplifying them. Also, the methodology allows quality evaluation of operation activities at urban transit operators. The proposed c

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Hermawan, Dedy, and Simon Sumanjoyo. "BUS RAPID TRANSIT POLICY IN MUNICIPAL CITY OF BANDAR LAMPUNG." Spirit Publik: Jurnal Administrasi Publik 10, no. 2 (2016): 17. http://dx.doi.org/10.20961/sp.v10i2.1262.

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<p>The aim of the research is to describe and discess the policy cycle of Bus Rapid Transit, the polemic in the policy of bus rapid transit, and the involvement of the stakeholder and their role in bus rapid transpit policy in Bandar Lampung. This research uses post positivistic paradigm with the approach of qualitative descriptive research method. This research resulted as: firstly, the bus rapid transit is an derivative regulation of Act No. 22 2009 regarding Traffic and Road Transport, aimed to reduce traffic jam in Bandar Lampung city. Secondly, the policy of bus rapid transit was ar

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Lee, Jinwoo, Amer Shalaby, John Greenough, Mike Bowie, and Stanley Hung. "Advanced Transit Signal Priority Control with Online Microsimulation-Based Transit Prediction Model." Transportation Research Record: Journal of the Transportation Research Board 1925, no. 1 (2005): 185–94. http://dx.doi.org/10.1177/0361198105192500119.

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An advanced transit signal priority (TSP) control method is presented: it provides priority operation in response to real-time traffic and transit conditions. A high-performance online microscopic simulation model was developed for the purpose of predicting transit travel time along an intersection approach. The proposed method was evaluated through application to a hypothetical intersection with a nearside bus stop. The performance of the proposed method was compared with that of normal signal operation without TSP and a conventional signal priority method. The experimental results indicated

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Afanasev, Dennis. "Detection of Exoplanets Using the Transit Method." George Washington University Undergraduate Review 1, Spring 2018 (2018): 10–14. http://dx.doi.org/10.4079/2578-9201.1(2018).03.

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Kolbe, Geoffrey. "A Test of the “Simultaneous Transit Method”." Journal for the History of Astronomy 39, no. 4 (2008): 515–17. http://dx.doi.org/10.1177/002182860803900406.

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Zolotorev, M. S., and A. A. Zholents. "Transit-time method of optical stochastic cooling." Physical Review E 50, no. 4 (1994): 3087–91. http://dx.doi.org/10.1103/physreve.50.3087.

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Cranford, C. A., D. Sutton, S. A. Sadek, N. Kennedy, and A. Cuschieri. "New physiological method of evaluating oesophageal transit." British Journal of Surgery 74, no. 5 (1987): 411–15. http://dx.doi.org/10.1002/bjs.1800740531.

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Ma, Changxi, and Dong Yang. "Public transit network planning in small cites considering safety and convenience." Advances in Mechanical Engineering 12, no. 1 (2020): 168781402090235. http://dx.doi.org/10.1177/1687814020902351.

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Scientific and rational public transit network planning, not only can effectively alleviate city traffic congestion, but also can reduce the risk of accidents. First, based on the data of residents’ travel survey, this article employs the multiple regression method to forecast the traffic generation and adopts the double-constrained gravity model to forecast the residents’ travel distribution of small cites. Second, by aiming at public transit planning objectives, the unsafe roads for public transit are screened, and the public transit trip-mode sharing rate is set as the interval value. Accor

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Lai, Xiongfei, Jing Teng, Paul Schonfeld, and Lu Ling. "Resilient Schedule Coordination for a Bus Transit Corridor." Journal of Advanced Transportation 2020 (June 15, 2020): 1–12. http://dx.doi.org/10.1155/2020/5398298.

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Providing convenient transit services at reasonable cost is important for transit agencies. Timed transfers that schedule vehicles from various routes to arrive at some transfer stations simultaneously (or nearly so) can significantly reduce wait times in transit networks, while stochastic passenger flows and complex operating environments may reduce this improvement. Although transit priority methods have been applied in some high-density cities, operating delays may cause priority failures. This paper proposes a resilient schedule coordination method for a bus transit corridor, which analyze

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Zeng, Lu, Jun Liu, Yong Qin, Li Wang, and Jie Yang. "A Passenger Flow Control Method for Subway Network Based on Network Controllability." Discrete Dynamics in Nature and Society 2018 (September 4, 2018): 1–12. http://dx.doi.org/10.1155/2018/5961090.

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The volume of passenger flow in urban rail transit network operation continues to increase. Effective measures of passenger flow control can greatly alleviate the pressure of transportation and ensure the safe operation of urban rail transit systems. The controllability of an urban rail transit passenger flow network determines the equilibrium state of passenger flow density in time and space. First, a passenger flow network model of urban rail transit and an evaluation index of the alternative set of flow control stations are proposed. Then, the controllable determination model of the urban r

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Yang, Tianlin. "Transit and radial velocity method for exoplanet detection." Theoretical and Natural Science 10, no. 1 (2023): 137–42. http://dx.doi.org/10.54254/2753-8818/10/20230329.

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This article introduces some basic methods that human usually uses nowadays to detect exoplanets, including transits method, radial velocity method, direct imaging method, gravitational microlensing method, and astrometry method. As we all know, none of these methods are perfect, each of them has its advantages: some of them are good at detecting planets with great mass, some are good at detecting planets with great radius, and some of the methods are good at detecting planets far away from their host star. But at the same time, each method has its own disadvantages. That is the reason why som

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Ji, Yanjie, Bo Hu, Jing Han, and Dounan Tang. "An Improved Algebraic Method for Transit Signal Priority Scheme and Its Impact on Traffic Emission." Mathematical Problems in Engineering 2014 (2014): 1–11. http://dx.doi.org/10.1155/2014/412132.

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Transit signal priority has a positive effect on improving traffic congestion and reducing transit delay and also has an influence on traffic emission. In this paper, an optimal transit signal priority scheme based on an improved algebraic method was developed and its impact on vehicle emission was evaluated as well. The improved algebraic method was proposed on the basis of classical algebraic method and has improvements in three aspects. First, the calculation rules of split loss are more reasonable. Second, the delay caused by transit stations and queued vehicles can be considered. Third, m

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Iwanaga, Yuji, Jipu Wen, Mikael S. Thollander, et al. "Scintigraphic measurement of regional gastrointestinal transit in the dog." American Journal of Physiology-Gastrointestinal and Liver Physiology 275, no. 5 (1998): G904—G910. http://dx.doi.org/10.1152/ajpgi.1998.275.5.g904.

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Scintigraphic techniques can measure sequentially gastric emptying, small bowel transit, and colonic transit in humans, and comparable methods for experimental studies in animals would be useful. We developed such a method in dogs and examined the effects of prokinetic drugs on regional transit. Two isotopes were given to fasting dogs. Polystyrene pellets labeled with99mTc were mixed in a can of dog food and111In- labeled pellets were given in a gelatin capsule coated with a pH-sensitive polymer, designed to dissolve in the distal bowel. Gamma camera images were obtained for up to 24 h. Prokin

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Chen, Wan, and Kuan Min Chen. "Study on Connection of Rail Transit and Bicycle Traffic - A Case Study of Xi’an Metro Line2." Applied Mechanics and Materials 361-363 (August 2013): 1933–36. http://dx.doi.org/10.4028/www.scientific.net/amm.361-363.1933.

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The development of rail transit made travel convenient for urban residents, alleviated traffic pressure, but the long travel distance of the site and the surrounding areas affecting rail transit service level. In order to full play the rail transit large capacity, improve the appeal of the public transit, solve the problem of "last one kilometer", This paper summarized the importance of connection of rail transit and bicycle traffic with a case of xi 'an metro line 2, discussed the forecasting methods of rail transit and bicycle traffic transfer demand, then used vertical and horizontal analog

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