Japan Geoscience Union Meeting 2025

Presentation information

[E] Poster

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM10] Space Weather and Space Climate

Tue. May 27, 2025 5:15 PM - 7:15 PM Poster Hall (Exhibition Hall 7&8, Makuhari Messe)

convener:Ryuho Kataoka(National Institute of Polar Research), Antti Pulkkinen(NASA Goddard Space Flight Center), Mary Aronne(NASA GSFC/CUA), Yumi Bamba(National Institute of Information and Communications Technology)

5:15 PM - 7:15 PM

[PEM10-P07] Development of Compact magnetogram using polarized imaging sensor for space weather monitoring

*Park Inchun1, Kenichi Otsuji1, Satoshi Morita1, Daikou Shiota1, Yumi Bamba1, Tatsuki Tahara1 (1.National Institute of Information and Communications Technology)

Keywords:Solar magnetic field observation, Magnetogram

Observing the solar magnetic field is crucial for space weather forecasting, as solar flares result from intense magnetic energy release. Predicting flares in advance helps mitigate their impact on geospace, making continuous observation and analysis of the Sun’s magnetic field structure.

Currently, observations rely on NASA’s SDO and the ground-based GONG network. However, these programs may face observation gaps due to system failures or aging equipment. To address this, NICT is developing a compact solar magnetograph utilizing the 630 nm Fe I absorption line to enable efficient, cost-effective, and continuous observations.

This system incorporates Etalon filters, polarization image sensors, and liquid crystal retarders, allowing for rapid magnetic field measurements compared to conventional spectropolarimetry, which relies on scanning mechanisms. By reducing moving parts, we achieve a compact, low-maintenance design suited for long-term operation.

This study evaluates the performance of the newly developed instrument, presents solar magnetic field observation results, and explores future improvements for enhanced space weather forecasting.