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윤정환(Junghwan Yoon),서예지(Yezee Seo),김훈규(Hoonkyu Kim),권태경(Taekyoung Kwon) 한국정보보호학회 2018 정보보호학회논문지 Vol.28 No.2
FPGA (Field Programmable Gate Array) 는 개발자가 유연하게 프로그래밍 할 수 있다는 장점으로 인해 다양한 분야에서 사용되고 있다. 하지만 외부에서 구현된 시스템이 비트스트림 형태로 FPGA에 탑재 될 경우 오작동을 일으키거나 정보를 유출시키는 등의 하드웨어 악성 기능이 포함될 가능성이 있다. 이러한 이유로 비트스트림 역공학은 필수적이며, 따라서 이와 관련된 연구들이 진행되어 왔다. 본 논문에서는 FPGA 비트스트림 역공학 연구사례 중 가장 대표적인 역공학 알고리즘을 활용한 BIL 비트스트림 역공학 도구에 대한 분석 실험을 진행하여 성능 및 한계점을 확인하였다. Field Programmable Gate Array (FPGA) is widely used in a variety of fields because of its ability to be programmed as desired. However, when an externally implemented program is loaded on FPGA in the form of a bitstream, there is a possibility that hardware Trojans which cause malfunctions or leak information may be included. For this reason, bitstream reverse engineering is essential, and therefore related research has been conducted, such as BIL. In this paper, we analyze the BIL bitstream reverse engineering tool, which is the most representative algorithm, regarding its performance and limitations.
Ji-Hyeon Yoo,Dae-Young Lee,Eojin Kim,Hoonkyu Seo,Kwangsun Ryu,Kyung-Chan Kim,Kyoungwook Min,Jongdae Sohn,Junchan Lee,Jongho Seon,Kyung-In Kang,Seunguk Lee,Jaeheung Park,Goo-Hwan Shin,SungOg Park 한국우주과학회 2021 Journal of Astronomy and Space Sciences Vol.38 No.1
In this paper, we present observations of the Space Radiation Detectors (SRDs) onboard the Next Generation Small Satellite-1 (NEXTSat-1) satellite. The SRDs, which are a part of the Instruments for the study of Stable/Storm-time Space (ISSS), consist of the Medium-Energy Particle Detector (MEPD) and the High-Energy Particle Detector (HEPD). The MEPD can detect electrons, ions, and neutrals with energies ranging from 20 to 400 keV, and the HEPD can detect electrons over an energy range from 0.35 to 2 MeV. In this paper, we report an event where particle flux enhancements due to substorm injections are clearly identified in the MEPD A observations at energies of tens of keV. Additionally, we report a specific example observation of the electron distributions over a wide energy range in which we identify electron spatial distributions with energies of tens to hundreds of keV from the MEPD and with energy ranging up to a few MeV from the HEPD in the slot region and outer radiation belts. In addition, for an ~1.5-year period, we confirm that the HEPD successfully observed the well-known outer radiation belt electron flux distributions and their variations in time and L shell in a way consistent with the geomagnetic disturbance levels. Last, we find that the inner edge of the outer radiation belt is mostly coincident with the plasmapause locations in L, somewhat more consistent at subrelativistic energies than at relativistic energies. Based on these example events, we conclude that the SRD observations are of reliable quality, so they are useful for understanding the dynamics of the inner magnetosphere, including substorms and radiation belt variations.
Yoo, Ji-Hyeon,Lee, Dae-Young,Kim, Eojin,Seo, Hoonkyu,Ryu, Kwangsun,Kim, Kyung-Chan,Min, Kyoungwook,Sohn, Jongdae,Lee, Junchan,Seon, Jongho,Kang, Kyung-In,Lee, Seunguk,Park, Jaeheung,Shin, Goo-Hwan,Par The Korean Space Science Society 2021 Journal of astronomy and space sciences Vol.38 No.1
In this paper, we present observations of the Space Radiation Detectors (SRDs) onboard the Next Generation Small Satellite-1 (NEXTSat-1) satellite. The SRDs, which are a part of the Instruments for the study of Stable/Storm-time Space (ISSS), consist of the Medium-Energy Particle Detector (MEPD) and the High-Energy Particle Detector (HEPD). The MEPD can detect electrons, ions, and neutrals with energies ranging from 20 to 400 keV, and the HEPD can detect electrons over an energy range from 0.35 to 2 MeV. In this paper, we report an event where particle flux enhancements due to substorm injections are clearly identified in the MEPD A observations at energies of tens of keV. Additionally, we report a specific example observation of the electron distributions over a wide energy range in which we identify electron spatial distributions with energies of tens to hundreds of keV from the MEPD and with energy ranging up to a few MeV from the HEPD in the slot region and outer radiation belts. In addition, for an ~1.5-year period, we confirm that the HEPD successfully observed the well-known outer radiation belt electron flux distributions and their variations in time and L shell in a way consistent with the geomagnetic disturbance levels. Last, we find that the inner edge of the outer radiation belt is mostly coincident with the plasmapause locations in L, somewhat more consistent at subrelativistic energies than at relativistic energies. Based on these example events, we conclude that the SRD observations are of reliable quality, so they are useful for understanding the dynamics of the inner magnetosphere, including substorms and radiation belt variations.
Eojin Kim,Ji-Hyeon Yoo,Hee-Eun Kim,Hoonkyu Seo,Kwangsun Ryu,Jongdae Sohn,Junchan Lee,Jongho Seon,Ensang Lee,Dae-Young Lee,Kyoungwook Min,Kyung-In Kang,Sang-Yun Lee,Juneseok Kang 한국우주과학회 2020 Journal of Astronomy and Space Sciences Vol.37 No.3
This paper describes the initial operations and preliminary results of the Instrument for the study of Stable/Storm-time Space (ISSS) onboard the microsatellite Next Generation Small Satellite-1 (NEXTSat-1), which was launched on December 4, 2018 into a sun-synchronous orbit at an altitude of 575 km with an orbital inclination angle of 97.7°. The spacecraft and the instruments have been working normally, and the results from the observations are in agreement with those from other satellites. Nevertheless, improvement in both the spacecraft/instrument operation and the analysis is suggested to produce more fruitful scientific results from the satellite operations. It is expected that the ISSS observations will become the main mission of the NEXTSat-1 at the end of 2020, when the technological experiments and astronomical observations terminate after two years of operation.