OPTICAL DESIGN OF THE VIGIL HELIOSPHERIC IMAGER
Dr. Grzegorz Dariusz Pekala
Leonardo S.p.A.
Day
Tuesday · 2026-10-13
Time
11:20 AM - 12:40 PM
Track
Track 1
Session
Image Processing, Image Design & Scanning
Venue
ICSO 2026 Conference Venue
Track indicates the session hall. Refer to the on-site programme board for the exact room number and any last-minute room changes.
In 30 seconds
The Vigil Heliospheric Imager is designed to detect faint coronal mass ejections from the L5 Lagrange point to support space weather monitoring. It utilizes a sophisticated baffling system, including diffractive rejection front baffles, to minimize straylight from the Sun and planetary sources. This precise optical bench configuration ensures high signal-to-noise detection of low-contrast solar phenomena.
Read the full paper
Access the complete technical paper via the official ICSO 2026 programme.
Topics & Subtopics
Source traceability
ID: icso26_108
Schedule facts reproduced from the published ICSO 2026 programme. Enrichment metadata is a discovery aid, not a scientific classification.