• Title/Summary/Keyword: observational study

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Constraining non-Gaussianity with Minkowski Functionals

  • Chingangbam, Pravabati;Park, Chang-Bom
    • The Bulletin of The Korean Astronomical Society
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    • v.35 no.2
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    • pp.42.2-42.2
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    • 2010
  • The possibility of detection of deviation from Gaussian distribution of primordial perturbations in the Cosmic Microwave Background (CMB) Radiation is very important because it can shed light on how the perturbations were created in the very early universe. We study the effect of the primordal non-Gaussianity on topological observables called Minkowski Functionals, which are functions of the temperature fluctuation field, and show that they carry distinct signatures of different types of non-Gaussianities. Then, we constrain the non-Gaussianity parameters by comparing the theoretical predictions of the Minkowski Functionals with measurements from observational data from WMAP.

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A Retrospective Observational Study on the Emotional Characteristics of Hwa-Byung Inpatients in a Korean Medicine Hospital Using the Core Seven-Emotions Inventory-Short Form (한방병원에 입원한 화병 환자의 정서적 특성에 대한 핵심칠정척도 단축형을 활용한 후향적 관찰연구)

  • Kim, Ju Yeon;Kang, Dong Hoon;Kang, Hyung-Won;Jung, In Chul
    • Journal of Oriental Neuropsychiatry
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    • v.33 no.1
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    • pp.1-19
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    • 2022
  • Objectives: The objective of this study was to confirm the Chiljeong (七情) characteristics of Hwa-byung patients using the core seven-emotions inventory-short form. Methods: We conducted a retrospective observational study based on the electronic medical records from a Korean medicine hospital. We included patients who were diagnosed with Hwa-byung and examined with Core Seven-Emotions Inventory-short Form (CSEI-S) during hospitalization periods. We presented the characteristics of Hwa-byung by demographic information, CSEI-S, Hwa-byung scale, and Korean Symptom Checklist 95. A correlation analysis was performed between CSEI-S and other clinical and psychological characteristics. Results: The Chiljeong characteristics of Hwa-byung were high in the order of Sorrow (悲), Thought (思), Fear (恐), Fright (驚), Depression (憂), Joy (喜), and Anger (怒). There was no significant difference between each emotion. After combined Korean medical treatment, Sorrow (悲) and Thought (思) significantly decreased. There were static correlations between sorrow (悲) and fright (驚), thought (思) and sorrow (悲), depression (憂) and sorrow (悲), depression (憂) and fright (驚), thought (思) and depression (憂), fear (恐) and fright (驚), anger (怒) and thought (思), thought (思) and fright (驚), sorrow (悲) and fear (恐). Sorrow (悲) and Hwa-byung characteristics scale showed static correlation. Joy (喜) showed a static correlation with disharmony between the heart and kidney scores of the Hwa-byung pattern identification. Between KSCL-95 and CSEI-S, static correlation appeared in depression (憂) with depression, anxiety, and sleep problem scale, sorrow (悲) with depression and anxiety, fright (驚) with depression and obsessive symptoms. Conclusions: Despite several limitations due to the study design and small sample size, this research successfully used CSEI-S to study the Chiljeong (七情) characteristics of Hwa-byung for the first time.

The Effect of Korean Medical Combination Treatment on 72 Cases of Herniated Intervertebral Lumbar Disc Patients: An Observational Study (요추 추간판탈출증 입원환자 72례에 대한 한의학적 복합치료 효과의 관찰 연구)

  • Kim, Sang Min;Lee, Sun Ho;Shin, You Bin;Choi, Ji Hoon;Koo, Ja Sung;Yoo, Hyung Jin;Lee, Dong Hyun
    • Journal of Acupuncture Research
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    • v.32 no.2
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    • pp.23-33
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    • 2015
  • Objectives : This study was designed to assess the general distribution and clinical effectiveness of Korean medical treatment on lumbar disc herniation. Methods : This is an observational study. 72 patients admitted to Daejeon Jaseng Hospital of Korean Medicine with a diagnosis of herniated intervertebral disc(HIVD) by lumbar-CT of lumbar-MRI were observed from July, 2014 to April, 2015. They were analyzed according to sex, age, the period of disease, causal factors, symptoms on admission, admission day, disc herniation type and treatment efficacy. All patients received a combination of treatments during hospitalization, including acupuncture, Chuna, herbal medicines and physical therapy. A zero to ten numerating rating scale(NRS) assessing pain, Oswestry disability index(ODI) and EuroQol-5 dimension(EQ-5D) was used before and after treatments. Results : Average admission duration was $28.00{\pm}12.85$ days in lumbar disc patients. For lumbar patients, lower back pain NRS decreased from $5.89{\pm}2.00$ to $3.42{\pm}1.87$(p<0.001) and radiating pain from $5.96{\pm}2.12$ to $3.38{\pm}1.83$(p<0.001). ODI decreased from $46.69{\pm}19.25$ to $35.69{\pm}16.67$(p<0.001), and EQ-5D index increased from $0.63{\pm}0.26$ to $0.71{\pm}0.20$(p<0.05) after treatment in lumbar disc patients. Conclusions : Korean medical combination treatment might be effective in reducing pain and improving quality of life for patients with lumbar disc herniation. This study further confirmed the efficacy of Korean medical treatment on HIVD.

Development of a Period Analysis Algorithm for Detecting Variable Stars in Time-Series Observational Data

  • Kim, Dong-Heun;Kim, Yonggi;Yoon, Joh-Na;Im, Hong-Seo
    • Journal of Astronomy and Space Sciences
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    • v.36 no.4
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    • pp.283-292
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    • 2019
  • The purpose of this study was to develop a period analysis algorithm for detecting new variable stars in the time-series data observed by charge coupled device (CCD). We used the data from a variable star monitoring program of the CBNUO. The R filter data of some magnetic cataclysmic variables observed for more than 20 days were chosen to achieve good statistical results. World Coordinate System (WCS) Tools was used to correct the rotation of the observed images and assign the same IDs to the stars included in the analyzed areas. The developed algorithm was applied to the data of DO Dra, TT Ari, RXSJ1803, and MU Cam. In these fields, we found 13 variable stars, five of which were new variable stars not previously reported. Our period analysis algorithm were tested in the case of observation data mixed with various fields of view because the observations were carried with 2K CCD as well as 4K CCD at the CBNUO. Our results show that variable stars can be detected using our algorithm even with observational data for which the field of view has changed. Our algorithm is useful to detect new variable stars and analyze them based on existing time-series data. The developed algorithm can play an important role as a recycling technique for used data

A Multi-wavelength Observational Study of Eruption Processes of Two Prominences in the Solar Active Region NOAA 11261

  • Park, Sung-Hong;Cho, Kyung-Suk
    • The Bulletin of The Korean Astronomical Society
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    • v.38 no.2
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    • pp.90.1-90.1
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    • 2013
  • To better understand the physics underlying the eruption of prominences in solar active regions, we studied eruption processes of two active prominences located in the active region NOAA 11261 using multi-wavelength observational data with high temporal and spatial resolution. Specifically, we examined (1) the temporal variation of morphology and plasma properties of the two active prominences, (2) magnetic fields and their evolution on the photospheric surface underneath the prominences, and (3) the time profiles and locations of radio, EUV, and soft/hard X-ray emissions produced by the M9.3 flare related to the prominence eruption. As a result, we found that: (1) a prominence F1 began to erupt and expand as the abrupt and intense EUV brightening occurred in the localized region underneath the western part of F1 at 03:45 UT prior to the peak time of the M9.3 flare, (2) F1 split into two parts: i.e., the western part asymmetrically erupted by producing the M9.3 flare with microwave source motions along the magnetic polarity inversion line between the two flare ribbons, while the eastern part coalesced into a pre-existing prominence F2, (3) F2 became unstable due to the coalescence with the eastern part of F1, and then it partially erupted with clockwise untwisting motions.

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Effects of asymmetric plasmasphere on MHD waves in a three-dimensional dipolar magnetosphere

  • Roh, Sang-Il;Lee, Dong-Hun;R. E. Denton;K. Takahashi;J. Goldstein;A. Keiling;R. A. King;K. Yumoto
    • Bulletin of the Korean Space Science Society
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    • 2003.10a
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    • pp.39-39
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    • 2003
  • The plasmaspheric region shows relatively strong longitudinal asymmetry in the sense that the location of the plasmapause and the density distribution significantly vary with respect to local time, and this asymmetry effect has been neglected in previous magnetospheric ULF wave studies. In this study, we numerically examine the MHD wave properties of field line resonances (FLRs) and Pi2 pulsations when the inner magnetosphere is assumed to be asymmetric. We use the dipole magnetic field model, but our density model is based on. observational data from the IMAGE satellite. We assume an impulsive input in the magnetotail, which can be associated with a substorm onset. Our results suggest that local FLRs appear in both the radial and azimuthal oscillations owing to the asymmetry. Plasmaspheric Pi2 signals appear in the compressional component, but they are more strongly affected by ambient plasmaspheric structure than the FLRs. We compare our results with the observational data of Pi2 events.

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Rotational and Observational Properties of NEA and Asteroid Family

  • Kim, Myung-Jin
    • The Bulletin of The Korean Astronomical Society
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    • v.39 no.2
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    • pp.96.1-96.1
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    • 2014
  • The rotation of asteroids can help reveal not only the fundamental characteristics of asteroids but also the origin and evolution of our Solar System. From the photometric observations for NEA 162173 (1999 JU3) and Maria family asteroids using 0.5 m- to 2 m- class telescopes at 10 observatories in the northern hemisphere, I obtained a total of 260 lightcurves for 97 asteroids and derived synodic rotational periods for 51 objects, including newly obtained periods of 34 asteroids. For the sake of efficiency, I developed an observation scheduler, SMART (Scheduler for Measuring Asteroid RoTation) and a photometric analysis software subsystem, ASAP (Asteroid Spin Analysis Package). Based on the lightcurve analysis of NEA 162173 (1999 JU3) and Maria family asteroids, 1) I present the rotational and observational characteristics of 1999 JU3 and provided the Hayabusa-2 Science team with the information on pole orientations, 2) I investigated correlations among rotational periods, amplitudes of lightcurves, and sizes, and conclude that the rotational properties of old-type family asteroids have been changed considerably by the YORP effect. 3) Finally, I found the Yarkovsky footprints on the Maria asteroid family and estimated that approximately 37 to 75 Maria family asteroids larger than 1 km have entered the near-Earth space every 100 Myr. This study should reveal the collisional history and transport route of the members from the resonance region to the near Earth space, for the first time.

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Evaluation of damage probability matrices from observational seismic damage data

  • Eleftheriadou, Anastasia K.;Karabinis, Athanasios I.
    • Earthquakes and Structures
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    • v.4 no.3
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    • pp.299-324
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    • 2013
  • The current research focuses on the seismic vulnerability assessment of typical Southern Europe buildings, based on processing of a large set of observational damage data. The presented study constitutes a sequel of a previous research. The damage statistics have been enriched and a wider damage database (178578 buildings) is created compared to the one of the first presented paper (73468 buildings) with Damage Probability Matrices (DPMs) after the elaboration of the results from post-earthquake surveys carried out in the area struck by the 7-9-1999 near field Athens earthquake. The dataset comprises buildings which developed damage in several degree, type and extent. Two different parameters are estimated for the description of the seismic demand. After the classification of damaged buildings into structural types they are further categorized according to the level of damage and macroseismic intensity. The relative and the cumulative frequencies of the different damage states, for each structural type and each intensity level, are computed and presented, in terms of damage ratio. Damage Probability Matrices (DPMs) are obtained for typical structural types and they are compared to existing matrices derived from regions with similar building stock and soil conditions. A procedure is presented for the classification of those buildings which initially could not be discriminated into structural types due to restricted information and hence they had been disregarded. New proportional DPMs are developed and a correlation analysis is fulfilled with the existing vulnerability relations.

Breastfeeding and the Risk of Childhood Hodgkin Lymphoma: A Systematic Review and Meta-analysis

  • Wang, Ke-Lai;Liu, Chun-Lan;Zhuang, Yan;Qu, Hong-Yi
    • Asian Pacific Journal of Cancer Prevention
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    • v.14 no.8
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    • pp.4733-4737
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    • 2013
  • Purpose: Numerous observational epidemiological studies have evaluated associations between breastfeeding and the risk of childhood Hodgkin lymphoma; however, the existing results are inconsistent. We therefore conducted a systematic review and meta-analysis. Methods: Medical literature was searched in the Pubmed and Embase databases to identify all English-language relevant studies up to April 10, 2013. Reference lists were thereafter hand-searched for additional articles. Studies that reported relative risk ratios (RRs) or odds ratios (ORs) with 95% confidence intervals (CIs) were included. This meta-analysis was conducted in accordance with the guidelines for the meta-analysis of observational studies in epidemiology. Results: We finally included 10 case-control studies in our meta-analysis, involving 1,618 childhood Hodgkin lymphoma cases and 8,181 controls. Overall, we did found a borderline significant association between breastfeeding and reduced risk of childhood Hodgkin lymphoma comparing ever breastfed children to never breastfed children (pooled OR =0.79; 95%CI, 0.58-1.08; P=0.13), with limited evidence for between-study heterogeneity (P =0.12, $I^2$ = 35.70%). Conclusion: There is limited evidence for an inverse association between breastfeeding and risk of childhood Hodgkin lymphoma.

Characteristics of Efficient Radius of Meteorological Observation Data to Estimate Regional Wind Energy (국지규모 풍력에너지 평가를 위한 기상 관측 자료의 영향 반경 특성)

  • Lee, Soon-Hwan;Kim, Min-Jung;Lee, Hwa-Woon
    • Journal of Korean Society for Atmospheric Environment
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    • v.23 no.5
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    • pp.585-595
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    • 2007
  • Representative impacts and effectiveness of surface meteorological observation data assimilation were examined in order to use wind resources estimation around southern coastal area of the Korean Peninsula. The data used in study are observational wind and temperature data at 5 and 41 sites of Regional Meteorological Offices and Automatical Weather Systems, respectively. Observation wind speed data tends to show small effective radius with limited area. Especially assimilation impacts of data observed at peninsula type sites like Yeosu play only around the inside of the peninsula. This limited effective radius for wind speed is caused by the strong correlation between topography and wind speed. And the efficient radius for surface air temperature is larger than that of wind. Data assimilation for observational air temperature is useful to increase the accuracy of wind energy estimation. However assimilation of wind data requires special care in its application due to high sensitivity of topographical complexity.