주소 관련 미래 산업의 확장으로 새로운 주소체계에 대한 수요가 증가하였으며, 특정 사물에 주소를 부여하는 체계인 사물주소의 중요성이 강조되고 있다. 현행 사물주소는 행정안전부가 제작 및 배포하고 있으며 데이터베이스 제작 등 사물주소의 활성화를 위한 노력이 지속되고 있다. 하지만 현행 사물주소는 하향식 방법으로 부여되고 있기 때문에 수요자 응답형 정보제공 대응에 미흡한 현실이다. 이에 본 연구에서는 상향식 방법으로 운영 중인 포켓몬 고 DB와 사물주소 DB의 공간적 분포를 탐색함으로 써 사용자 참여형 주소정보 생성 및 적용 가능성을 제시하였다. 각 DB의 지점별 티센 폴리곤을 생성한 뒤 ANOVA 분석을 수행한 결과 두 DB간의 면적 차이가 있음을 확인하였다. 또한 지니 계수를 산출하여 분포 불평등성을 확인하여 DB를 통합하여 활용하는 방법을 제시하였다. 본 연구는 사물주소의 확산과 알기 쉬운 대국민 주소정보체계 확립에 정책적인 활용이 가능할 것이다.

현대형 소송이 증가함에 따라 전문가 증인의 역할의중요성이갈수록증대되고있다. 영미법계 를 따르는 미국은 특허 소송에서 전문가 증인 (Expert Witness)의 사용이 일반화되어 있으며, 전문가 증인은 소송 초기부터 배심원 재판까지 많은 절차에서 중요한 역할을 하고 있다. 배심원 은 1심 소송의 거의 마지막에 소송 절차에 참여 하기 때문에, 당사자를 위해 증언하는 전문가 증 인의 증언이 배심원 재판에서 허용되기 위해서는 기준이 필요했고, Frye, Dauert 판결 등에 의해 기준이 설정되다가 미국연방증거법 제702조에 법제화되었다. 우리나라는 대륙법 체계의 국가로, 소송의 사실판단에서 전문가의 도움을 받는 방법 으로 감정인 제도를 주로 이용해 왔으나, 부실한 감정, 감정인의 도덕성, 추상적 감정사항 기재로 인한 무용한 감정결과, 형식적인 감정인 신문등 이에 대한 문제점이 노출되면서, 전문심리위원제 도를 2007년 도입하였다. 하지만 전문심리위원제도 역시 역할 대비 복잡한 절차, 낮은 전문심리 위원 수당, 제도 자체에 대한 인식부족, 전문심리 위원의 의견에 대한 반박 절차의 부족 등으로 그 활용도가 낮아서 문제가 되었으며, 이의 개선을 위해 의료 및 건축분야에 한정하여 상임전문심리 위원제도를 도입하였다. 하지만 감정인의 문제점 은 해결이 어려운바, 법원의 공정한 판결을 위해, 프랑스에서 시행하고 있는 특임판사 제도와 유사 한 감정인의 업무를 총괄하는 전문심리관제와 전 문기술의 심리방안 연구와 전문심리위원 선정을 위한 각 기술 분야별 전문가 위원회를 법원산하 에서 운영하는 방안을 제안한다. 우리나라 특허 소송은 특허법원이 2020년 전문심리위원 추천위 원 위촉등을 시작으로 본격적인 전문위원제도 활 용을 시작했고, 특허심판원도 2021년 전문심리 위원제도 운영을 시작하는 등, 특허 소송에 전문 가 활용 제고를 위해 노력하고 있으나, 기존 감정 인과 전문심리위원의 문제는 여전히 안고 있는바, 특허법원 산하에 전문심리관과 전문가위원회를 두어 이에 대한 해결까지 같이 진행하는 방안을 제안하고자 한다. 미국 Dauert 판결의 전문가 증 언 허용 기준은 우리나라에서 증거력과 증명력의 기준으로 사용되고 있으나, 국민참여재판 제도가 확대된다면, 배심원 재판에서 제시허용 기준에대 한 명확한 기준이 제시되어야 할 것이다.

Republic of Korea has both criminal penalty and punitive damages as a remedy for willful infringement of patent rights after the revision of the Patent Act in 2018. The statutory sentence for willful patent infringement, especially imprisonment, has been enacted since 1961, and the sentence has increased, but statistics over the past 13 years show that the application from the prosecution stage to the judgment is extremely insignificant. Even in the one case in which the prison sentence was ordered, it was necessary to apply doctrine of equivalent, and it is difficult to show the clarity required by the principle of legality, which shows circumstantial evidence that raises doubts about the necessity and justification of the imprisonment against willful patent infringement. Punitive damages is a system that has a punitive function and a deterrent and preventive function of the infringer’s actions, and can perform the same function as the imprisonment against infringement. The United States, Taiwan, China, Canada, Australia and the Philippines, which have punitive damages, do not have criminal penalties for willful infringement. Republic of Korea is the only country that has both criminal penalties and punitive damages for willful patent infringement. For the development of science and technology and economic development, published patents must be used in various ways throughout society. Due to its nature, it is desirable for the regulation and coordination of the country in the field of science and technology to intervene only to the extent of supplementing it while respecting individual autonomy and creativity as much as possible. The purpose of the Patent Act lies in technological innovation and industrial development, and although it is a willful infringement, punishing patent infringers as imprisonment or threatening them can be an act of cutting off the buds of technological innovation in advance. It would be desirable to perform remedies for patent infringement as compensatory damages, and punishment and prevention for willful infringement through punitive damages.

The IGRINS is a near infrared high resolution spectrograph jointly developed by the Korea Astronomy and Space Science Institute and the University of Texas at Austin. We present design and fabrication of the optomechanical mount for the five mirrors, i.e., an input fold mirror, a slit mirror, a dichroic, and two camera fold mirrors. Based on the structure analysis and the thermal analysis of finite element methods, the optomechanical mount scheme satisfies the mechanical and the thermal design requirements given by the optical tolerance analysis. The performance of the fabricated mirror mounts has been verified through three IGRINS commissioning runs.

We present a method to improve the RV (radial velocity) measurements accuracy by using telluric lines. Telluric lines are used to estimate the wavelength scale drift over the detector of the spectrograph. In the case of BOES, the Echelle spectrograph at BOAO (Bohyunsan Optical Astronomical Observatory), the wavelength scale drift can be several hundreds m/s over 24 hours. Due to the wavelength scale drift, the RV measurements accuracy of BOES is limited to several hundreds m/s. By estimating the wavelength scale drift by telluric lines, we can remove its effect to improve the RV measurements accuracy to about 40 m/s.

Ni-GDC (gadolinia-doped ceria) composite powders, the anode material for the application of solid oxide fuel cells, were prepared by a solution reduction method using hydrazine. The distribution of Ni particles in the composite powders was homogeneous. The Ni-GDC powders were sintered at 1400˚C for 2 h and then reduced at 800˚C for 24 h in 3% H2. The percolation limit of Ni of the sintered composite was 20 vol%, which was significantly lower than these values in the literature (30-35 vol%). The marked decrease of percolation limit is attributed to the small size of the Ni particles and the high degree of dispersion. The hydrazine method suggests a facile chemical route to prepare well-dispersed Ni-GDC composite powders.

In this study we present basic principles and features of RVI2CELL, a precise RV (radial velocity) estimation program to process stellar spectra obtained through iodine cell. RVI2CELL is very robust and fast program. The instrument profile can be modeled as a sum of Gaussian functions or a non-parametric arbitrary shape. The RV accuracy estimated by observation of a RV standard star Tau Ceti indicates about 9 m/s.

We present the result of radial velocity observation of a W UMa type binary star EX Leo. We observed the star on February 16, 2003, using Long-Slit spectrograph of BOAO(Bohyunsan Optical Astronomical Observatory). Since the spectral lines are broad due to its fast rotation, it is difficult to distinguish two radial velocities from cross correlation function. Instead of cross correlation function, we used broadening function to develop our own code which estimate the radial velocity of the broadened line spectra. With our own code, radial velocities of primary and secondary stars are derived simultaneously. From the radial velocity curve fit, we obtained K1=50.24±8.29km/s and K2=254.05±20.984km/s respectively.

We developed a new program for automatic continuum normalization of Echelle spectrographic data. Using this algorithm, we have determined spectral continuum of almost BOES data. The first advantage of this algorithm is that we can save much time for continuum determination and normalization. The second advantage is that the result of this algorithm is very reliable for almost spectral type of spectrum. But this algorithm cannot be applied directly to the spectrum which has very strong and broad emission lines, for example Wolf-Rayet type spectrum. We implanted this algorithm to the program which was developed in the previous study. And we introduced more upgraded BOES data reduction program. This program has more convenient graphical user interface environment, so users can easily reduce BOES data. Lastly, we presented the result of study on line profile variation of magnetic Ap/Bp stars analyzed using this program.

We plan to install the polarimetric optics in the AGU(acqusition and guiding unit) of the 1.8 m telescope at the BOAO(Bohyunsan Optical Astronomy Observatory). With this, the spectropolarimetric observations with the resolution of 45,000 and 60,000 in 4,000 to 8,000＼AA ange could be done by the BOES(BOao Echelle Spectrograph). If we use the precision radial velocity measurement capability of the BOES, the accuracy of the magnetic field intensity measurements with this new BOES stokesmeter will be much increased. We present here the design concept of the BOES stokesmeter. Some details on the optics, mechanical parts, fiber parts and the lab test procedures of this stokesmeter are explained.

We developed a data reduction program (RX) to process BOES data automatically. It processes a whole set of data taken during one night automatically - preprocessing, extraction to one-dimensional spectra and wavelength calibration. The execution is very fast and the performance looks pretty good. We described the performance of this program, comparing its procedure with that of IRAF. RX does not have functions for continuum normalization yet. We will develop those functions in the next works.