천문학회오픈콜로퀴움
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저자 : 한국천문학회 | 등록일시 : 2022-12-05 11:07:17 | |||||||||
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안녕하십니까. 이번주 수요일(12월 7일) 오전 10:30에 아래와 같이 정규 콜로퀴움이 진행될 예정입니다. 많은 참여 부탁드립니다. 발표자 : 박진혜 (경희대학교 연구교수) 호스트 : 김수진 (우주과학본부) 장소 : 장영실홀 331-2 및 원격 연결 일시 : 12월 7일 (수) 오전 10:30 접속주소 : https://us02web.zoom.us/j/84597516884?pwd=OHVjOEQra1lSZ242K2tOZWY4T2Nzdz09 교육학점: 천문연 소속 현장참석자의 경우 필수 0.5 학점 부여 제목: Solar Energetic Particles Observed by
Multiple Spacecraft 초록: Solar
Energetic Particles (SEPs) are composed of protons, electrons, and heavy ions
with energies ranging from hundreds of keV to MeV. They are accelerated in
magnetic reconnection regions (impulsive events) and by Coronal Mass Ejection
(CME)-driven shocks (gradual events). Large-scale SEP events are one of the
most important phenomena in terms of space weather. They pose a risk of
radiation exposure to humans and equipment in space. In this presentation, I
will show the study of the large SEP sources using extreme-ultraviolet (EUV)
images and Potential Field Source Surface (PFSS) extrapolations from the
conventional magnetograms and AI-HMI magnetogram on a near real-time basis. The
features of SEPs strongly depend on physical quantities of CMEs and flares at
the connecting footpoints between the sources and the spacecraft. I will
present the temporal and spatial variations of SEP fluxes observed by in-situ
measurements and the relations between the fluxes and the quantities of the SEP
sources. 진행언어 : 한국어 슬라이드언어 : 영어 원격 접속 방법 : A. 웹 브라우저 : Chrome을 추천하며 아래 주소를 실행시 Zoom 구동을 위한 프로그램이 설치될 수 있음 2022년 하반기 KASI 콜로퀴움 일정 https://www.kasi.re.kr/kor/post/eng_colloquium (위 일정은 연사분의 상황에 따라서 변경될 수 있습니다.) 천문연 콜로퀴움 위원회 (홍성욱, 최지훈, 오희영) 드림 Dear all, KASI's regular colloquium is scheduled on this Wednesday,
December 7. Speaker : Dr. Jinhye Park (KHU) Host : Sujin Kim Place : Jang Yeong-sil Hall 331-2 & Online Time : Dec. 7 (Wed)
10:30 am Access: https://us02web.zoom.us/j/84597516884?pwd=OHVjOEQra1lSZ242K2tOZWY4T2Nzdz09 KASI Educational credits: 0.5 educational credits are awarded
to off-line attendees. Title: Solar Energetic Particles Observed by Multiple Spacecraft Abstract: Solar
Energetic Particles (SEPs) are composed of protons, electrons, and heavy ions
with energies ranging from hundreds of keV to MeV. They are accelerated in
magnetic reconnection regions (impulsive events) and by Coronal Mass Ejection
(CME)-driven shocks (gradual events). Large-scale SEP events are one of the
most important phenomena in terms of space weather. They pose a risk of
radiation exposure to humans and equipment in space. In this presentation, I
will show the study of the large SEP sources using extreme-ultraviolet (EUV)
images and Potential Field Source Surface (PFSS) extrapolations from the
conventional magnetograms and AI-HMI magnetogram on a near real-time basis. The
features of SEPs strongly depend on physical quantities of CMEs and flares at
the connecting footpoints between the sources and the spacecraft. I will
present the temporal and spatial variations of SEP fluxes observed by in-situ
measurements and the relations between the fluxes and the quantities of the SEP
sources. Language : Korean Slide Language : English Remote access procedure : A. Web browser : Chrome - When executing the address below, a
program for additional zoom operation can be installed. B. Access : Go to https://us02web.zoom.us/j/84597516884?pwd=OHVjOEQra1lSZ242K2tOZWY4T2Nzdz09 C. Notice : After join, Please mute your microphone. - The default
setting is microphone mute. 2022B KASI Colloquium Schedule https://www.kasi.re.kr/kor/post/eng_colloquium (This schedule may be changed according to the situation of the
speaker.) KASI Colloquium committee (Sungwook E. Hong, Jihoon
Choi, Heeyoung Oh) |
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이전글 | [KASI Colloquium] November 30 (Wed) 10:30 am - Youngdae Lee (CNU) / 이영대 (충남대학교) |
다음글 | [KASI Colloquium] December 14 (Wed) 10:30 am - Ross A. Burns (NAOJ) |