STEREO-B/SECCHI/HI-1 FITS data

The Heliospheric Imager-1 (HI-1) telescope is part of the Sun Earth Connection Coronal and Heliospheric Investigations (SECCHI) instrument suite on the NASA STEREO mission. The SECCHI on the two STEREO spacecraft are identical suites of remote sensing instruments designed to observe coronal mass ejections (CMEs) at the Sun and in transit outwards to 1 AU. The HI-1 telescope observes the inner heliosphere from 12 to 84 solar radii with the band-pass wavelength of 450-750 nm.

Data and Resources

This dataset has no data

Additional Info

Field	Value
Maintainer	NASA Space Physics Data Facility
Last Updated	March 30, 2026, 21:47 (UTC)
Created	April 8, 2025, 14:32 (UTC)
accessLevel	public
bureauCode	{026:00}
catalog_conformsTo	https://project-open-data.cio.gov/v1.1/schema
harvest_object_id	dcf4aeb4-91f9-4b0c-9743-dbab3943dc88
harvest_source_id	b99e41c6-fe79-4c19-bbc3-9b6c8111bfac
harvest_source_title	Science Discovery Engine
identifier	https://doi.org/10.48322/zstc-3d34
landingPage	https://doi.org/10.48322/zstc-3d34
license	https://www.usa.gov/government-works
modified	2026-03-23T22:16:01Z
programCode	{026:000}
publisher	STEREO Science Center;SSC;Solar Data Analysis Center (SDAC)
resource-type	Dataset
source_datajson_identifier	true
source_hash	aef6938d812d5c168b0cbdb03cc54175a8bdfa58c698786ecdbb77f22994246b
source_schema_version	1.1
theme	{Heliophysics}