• 제목/요약/키워드: visible wave

검색결과 141건 처리시간 0.025초

Illumination Control in Visible Light Communication Using Manchester Code with Sync-Mark Signal

  • Lee, Seong-Ho
    • 센서학회지
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    • 제29권3호
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    • pp.149-155
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    • 2020
  • In this study, we employed Manchester code for illumination control and flicker prevention of the light-emitting diode (LED) used in a visible light communication (VLC) system. In the VLC transmitter, the duty factor of the Manchester code was utilized for illumination control; in the VLC receiver, the spike signal from an RC-high pass filter was utilized to recover the transmitted signal whilst suppressing the 120-Hz noise arising from adjacent lighting lamps. Instead of the clock being transmitted in a separate channel, a syncmark signal was transmitted in front of each data byte and used as the reference time for transforming the Manchester code to non-return-to-zero (NRZ) data in the receiver. In experiments, the LED illumination was controlled in the range of approximately 12-84% of the constant wave (CW) light via changing of the duty factor from 10% to 90%. This scheme is useful for constructing indoor wireless sensor networks using LED light that is flicker-free and presents capability for illumination control.

맨체스터 코드의 부반송파 변조를 이용한 가시광통신의 조명제어 (Dimming Control in Visible Light Communication Using Subcarrier Modulation of Manchester Code)

  • 이성호
    • 센서학회지
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    • 제28권3호
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    • pp.191-197
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    • 2019
  • In this study, we propose a dimming control method for a visible light communication (VLC) system, in which the subcarrier on-off keying (OOK) modulation of Manchester code is used for data transmission. In the VLC transmitter, non-return-to-zero (NRZ) code data is transformed to Manchester code, which is OOK modulated with a subcarrier. Manchester code is used for flicker-free lighting; the duty factor is changed for dimming control, and the subcarrier is used for preventing the adjacent noise light interference. In the experiments, the dimming control was carried out from about 8%-92% of the continuous wave (CW) LED light. This configuration is simple and effective in constructing a VLC system for indoor wireless sensor networks with flicker-free illumination and dimming control capability without adjacent noise light interference.

천이주파수 변조를 이용한 가시광통신의 조명제어 (Illumination Control in Visible Light Communication Using Transition Frequency Modulation)

  • 이성호
    • 센서학회지
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    • 제30권2호
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    • pp.99-104
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    • 2021
  • In this study, we utilized the duty factor of the transition frequency modulation (TFM) for the illumination control of the light emitting diode (LED) light in visible light communication (VLC). The average optical power is linearly proportional to the duty factor in TFM waveforms. We used the transition frequencies of Na=5 and Nb=1 for the high and the low bits, respectively, of the non-return-to-zero (NRZ) data in the VLC transmitter. A resistor and capacitor high-pass filter (HPF) was used in the VLC receiver to eliminate the 120 Hz optical noise from adjacent lighting lamps and the spikes at the HPF output were used to recover NRZ data from the TFM waveform. In experiments, the illumination of the LED light was controlled in the range of 25-90% of the constant-wave optical power by changing the duty factor of the TFM waveforms.

TEST MODEL OF MILLIMETER-WAVE IMAGING RADIOMETER EQUIPMENT (MIRAE)

  • Lee, Ho-Jin;Kim, Won-Gyum;Seong, Jin-Taek;Kim, Dae-Suk;Na, Kyoung-Tae;Jung, Min-Kyoo;Chang, Yu-Shin;Kim, Soon-Tae;Kim, Yong-Hoon
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 2007년도 Proceedings of ISRS 2007
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    • pp.365-368
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    • 2007
  • Millimeter-wave (MMW) imaging radiometer systems have an attractive advantage to obtain an image through low visibility weather conditions such as fog, clouds and light rain compared with visible and infrared imaging systems. Many countries have developed a various kinds of MMW imaging radiometers for the aim of low cost and high performance. In Korea, Millimeter-wave Imaging RAdiometer Equipment (MIRAE) has been developed since the end of 2006. Recently the development of some modules was finished for the test model. This paper describes the design and development of the MIRAE. In addition, the test results of its manufactured modules are presented.

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Between Love and Hate: The New Korean Wave, Japanese Female Fans, and Anti-Korean Sentiment in Japan

  • Ahn, Ji-Hyun;Yoon, E Kyung
    • Journal of Contemporary Eastern Asia
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    • 제19권2호
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    • pp.179-196
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    • 2020
  • Despite the enormous success in Japan of Korean popular culture, including TV dramas and K-pop, over the past few decades, anti-Korean sentiment in the country has become increasingly visible and intense. In this article, we examine how young Japanese female fans of Korean popular culture engage with the Korean Wave discourse while also engaging with―or, rather, disengaging from―anti-Korean movements and hate speech. Whereas previous scholarship on the Korean Wave has emphasized the power of active fans' agency, this paper investigates how the fans who passionately and self-reflexively consume Korean popular culture understand and react to the growing anti-Korean sentiment in Japan. Through in-depth interviews with 15 of these fans in their 20s and 30s, we show how they have navigated the discursive space between appreciation for Korean culture and anti-Koreanism in Japan.

OOK변조된 가시광 데이터전송에서 바이트반전을 이용한 플리커 방지 (Flicker Prevention Using Byte-Inversion in OOK Modulated Visible Light Data Transmission)

  • 이준호
    • 전기전자학회논문지
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    • 제24권2호
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    • pp.579-585
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    • 2020
  • 본 논문에서는 가시광을 사용하는 데이터 통신에서 광원의 플리커를 방지하기 위하여 On-off keying(OOK) 변조와 바이트반전 전송방식을 사용하였다. 송신부에서는 100 kHz의 구형파 전압을 부반송파로 사용하여 9.6 kbps의 기저대역 non-return-to-zero (NRZ) 입력데이터를 OOK 변조하고, 데이터의 비트열 형태에 관계없이 LED의 평균 광전력이 항상 일정하게 유지되도록 바이트반전 신호를 부가하여 전송하였다. 수신부에서는 대역통과 필터를 사용하여 주변의 120 Hz 잡음광의 간섭을 소거하고 OOK복조기를 사용하여 NRZ 형태의 원 신호를 복구하였다. 이러한 구조는 가시광 램프의 조명을 이용하여 근거리의 무선데이터 네트워크를 구축하는 데에 유용하다.

망막반응으로 본 각종파장가시광선조사하에서 발육한 과두(올챙이)의 식물신경계기능변조에 관하여 (Functional Disturbances Through the Retinal Pigment Reaction of the Automatic Nervous System of Tadpoles Developed under Various Visible Rays)

  • 주인호
    • 한국동물학회지
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    • 제1권2호
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    • pp.17-24
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    • 1958
  • Since Kesser first described in 1934 the functional change of the autonomic nervous system caused by certain visible rays many researchers have unanimously approved that animals flashed with a red visible ray develop parasympathicotony while those flashed with a blue visible ray develop sympathicotony. On the other hand through studies made by our colleagues it is now well known that the inner-movement of the retinal pigments of frogs is stimulated in sympathicotony and is in reverse inhibited in parasimpathicotony. It is almost evident that the mechanism by which the inner-movement of the retinal pigments is due to sympathicotony derived from the excessive secretion of adrenalin. In addition , through may recent experiments on the pharmacological action of various medicines on the retinal pigments reaction of tadpoles , ranging from the excessive secretion of adrenalin. In addition , through my recent experiments on the pharmacologtical action of various medicines on the retinal pigments reaction of tadploes, raging from every developmental stage , Ifound that the movement of the retinal pigments by adrenalin is predominant in the earlier developmental stages of taopoles around 11 mm of body length, whereas other medicines fail to give any responce to the retinal pigments in such an earlier stage. When tadpoles grown to body length of 15-16m the retinal pigments move to the complete light position while kept in adrenalin solution. Based on these facts it might be well to consider that if tadpoles were grown under the visible rays for a given period, they might show a functional change of the autonomic nervous system and thereby cause of certain change in the physciological phases of the retinal reaction. Experiments were undertaken to find this matter and also to discover the simultaneous effects of the visible radiations on the developmental process of tadpoles. The results summarized as follows ; 1. The longest wave of visible rav has an effective reaction on the growth of body length of taopoles, while the shortest wave of visible ray causes the same for the metamorphoric differentiation of tadpoles. 2. When keeping two groups of tadpoles the first group of 15 mm body length grown for the period of one week and the latter group of 20 mm body length grown for two weeks under the various visible rays. swimming in adrenalin solution, the inner-movement of the retinal pigment occurs in both groups. The movement of pigments of the first group is accelerated in a sequence of blue ray \ulcorner green ray > brown ray> red ray, and that of the latter group is also accelerated in a sequence of blue ray>green ray > brown ray and red ray. 3. When keeping tow groups of tadpoles, the first group of 20 mm body length grown for the period of two weeks, the latter group of 25 m body length grown for three wheeks, under the various visible rays in sunlight, the inner-movement of the retinal pigments occurs in both groups. The movement of pigments of the first group is accelerated in a sequence of blue ray> green ray>brown ray and red ray, and that of the latter group is also accelerated in a sequence of blue ray > brow ray>red ray. 4. In order words, there facts manifest that tadpoles grown under the various visible rays reveal functional disturbances of the autonomic nervous system, at the time of 15 mm body length by adrenalin solution, which is a unique indicator illustrating the status of sympathicotony, and at the time of 20 mm body length by sunlight. This means that the longest visible ray cause sympathicotony, while the shortest visible ray causes parasympathicotony.

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In-Ceram Alumina Core와 IPS Empress 2 core의 분광반사율 연구 (A study on reflective spectrum between In-Ceram alumina core and IPS Empress 2 core)

  • 박명자;김주원
    • 대한치과기공학회지
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    • 제23권2호
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    • pp.189-202
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    • 2002
  • A study on reflective spectrum between In-Ceram alumina plate(IAP) and IPS empress 2 plate were carried out in order to determine the difference of reflective spectrum rates between materials and between thicknesses of materials(0.8mm, 1.0mm, 1.2mm) by visible wave. The rates are measured by spectrophotometer(Top scan model TC-1800). And an analysis of ANOVA and paired sample t-test were carried out. The results are summarized as follows. 1. The reflective rates of IAP and IPS increased slowly as visible wave spectrum increased. 2. The difference of reflective rates of IAP between 0.8mm and 1.0mm is significant but a little(less than 1%). The differences of reflective rates of IAP between 0.8mm and l.2mm and between 1.0mm and l.2mm are significant(8%, 10% ). 3. The differences of reflective rates of IPS between 0.8mm and 1.0mm and between 0.8mm and 1.2mm and between 1.0mm and 1.2mm are significant(0.06 %, 0.01 %, 2 %). 4. The differences of reflective rates of 0.8mm, 1.0mm between IAP and IPS are significant but a little(less than 0.9%, 0.5%). The difference of reflective rates of l.2mm between IAP and IPS is significant and larger than the other thicknesses relatively(7 %).

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적외선 열화상 카메라용 캘리브레이션 타겟 개발 (Development of Calibration Target for Infrared Thermal Imaging Camera)

  • 김수언;최만용;박정학;신광용;이의철
    • 비파괴검사학회지
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    • 제34권3호
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    • pp.248-253
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    • 2014
  • 카메라 영상 캘리브레이션은 머신비전과 같은 비전검사기술분야에서 영상으로부터 기하학적 정보를 정확하게 추출하고자 할 때 정확성을 높이는데 필요한 매우 중요한 과정이다. 그러나 기존에 가시광 카메라에 사용되던 캘리브레이션 타겟은 중적외선, 원적외선 열화상 카메라에 적용하기 어렵다. 최근에 적외선 열화상카메라를 이용한 결함측정기술이 많이 사용되면서 적용할 수 있는 캘리브레이션 타겟 개발이 요구되고 있다. 따라서 본고에서는 유한요소 열전달 해석을 이용하여 가시광 카메라와 적외선 열화상카메라 모두에 적용 가능한 캘리브레이션 타겟을 제안하였다. 개발된 캘리브레이션 타겟을 열화상카메라와 가시광 카메라로 촬영하여 비교실험 하였으며, 실험결과 제안된 캘리브레이션 타겟의 효율성을 보여준다.

PROBABILITY DISTRIBUTION OF SURFACE WAVE SLOPE DERIVED USING SUN GLITTER IMAGES FROM GEOSTATIONARY METEROLOGICAL SATELLITE AND SURFACE VECTOR WINDS FROM SCATTEROMETERS

  • Ebuchi, Naoto;Kizu, Shoichi
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 2002년도 Proceedings of International Symposium on Remote Sensing
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    • pp.615-620
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    • 2002
  • Probability distribution of the sea surface slope is estimated using sun glitter images derived from visible radiometer on Geostationary Meteorological Satellite (GMS) and surface vector winds observed by spaceborne scatterometers. The brightness of the visible images is converted to the probability of wave surfaces which reflect the sunlight toward GMS in grids of 0.25 deg $\times$ 0.25 deg. Slope and azimuth angle required for the reflection of the sun's ray toward GMS are calculated for each grid from the geometry of GMS observation and location of the sun. The GMS images are then collocated with surface wind data observed by three scatterometers. Using the collocated data set of about 30 million points obtained in a period of 4 years from 1995 to 1999, probability distribution function of the surface slope is estimated as a function of wind speed and azimuth angle relative to the wind direction. Results are compared with those of Cox and Munk (1954a, b). Surface slope estimated by the present method shows narrower distribution and much less directivity relative to the wind direction than that reported by Cox and Munk. It is expected that their data were obtained under conditions of growing wind waves. In general, wind waves are not always developing, and slope distribution might differ from the results of Cox and Munk. Most of our data are obtained in the subtropical seas under clear-sky conditions. This difference of the conditions may be the reason for the difference of slope distribution.

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