회원 여러분께,

2024년 6월 23일부터 강원도 평창에서 열리는 AOGS2024에서 고분해능태양관측연구 세션(ST28)을 아래와 같이 진행합니다.

고분해능 지상-우주기반 태양관측자료를 활용한 연구를 진행하시는 회원 여러분의 많은 관심과 참여를 바랍니다.

초록등록은 1월 2일까지입니다. 발표와 관련하여 문의가 있으신 경우 (eklim@kasi.re.kr)로 연락주시기 바랍니다.

* Session Description:

ST28: Recent Scientific Discoveries from Goode Solar Telescope at Big Bear Solar Observatory

(https://www.asiaoceania.org/aogs2024/public.asp?page=sessions_and_conveners.asp ) .

The 1.6-meter clear aperture, off-axis Goode Solar Telescope (GST), is the first facility-class solar telescope built in the U.S. in a generation. As one of the highest-resolution solar telescopes in the world, GST with its state-of-the-art instruments, routinely collects diffraction-limited spatial resolution photometric, spectroscopic, and polarimetric data at Big Bear Solar Observatory. Since its regular operation began in 2010, GST has been providing the community with open access to observations of the photosphere and chromosphere with unprecedented resolution, significantly advancing our understanding of the origin of solar activity and space weather, and the fundamental nature of the solar atmosphere. Current GST users are distributed over 61 universities, institutes, and observatories in 21 countries. GST has actively supported campaign observations with NASA space, rocket, and balloon missions (PSP, IRIS, Hinode, SO, NuStar, CLASP-2, BITSE, and SUNRISE-III), and other large ground-based facilities (ALMA, DKIST, GREGOR, NVST). This session will highlight recent scientific discoveries based on GST data and campaign observations with space missions and ground-based facilities. In addition, presentations of high-resolution studies of the Sun using large ground-based telescopes are also invited. The session topics cover many subfields of solar physics and space weather, including small-scale reconnection and chromospheric flows, fine structure of the quiet Sun, coronal heating, solar flares, filaments and prominences, sunspot oscillations, structure of sunspots and pores, etc. The session will further enhance the international collaborations between solar and terrestrial science communities, therefore increasing scientific output of the operational facilities.

* Session conveners:

Prof Wenda Cao (Big Bear Solar Observatory, New Jersey Institute of Technology)
Prof Jongchul Chae (Seoul National University)
Mr Haisheng Ji (Chinese Academy of Sciences)
Dr Eun-Kyung Lim (Korea Astronomy and Space Science Institute)
Dr Vasyl Yurchyshyn (Big Bear Solar Observatory, New Jersey Institute of Technology)

감사합니다.

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