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	Dr. Richard A. Harrison
Last Updated	July 9, 2025, 20:00 (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	e6df094b-de7b-4c57-8e1c-8670860d4282
harvest_source_id	b99e41c6-fe79-4c19-bbc3-9b6c8111bfac
harvest_source_title	Science Discovery Engine
identifier	https://doi.org/10.48322/zstc-3d34
modified	2025-07-09T19:35:24Z
programCode	{026:000}
publisher	STEREO Science Center;SSC;Solar Data Analysis Center (SDAC)
resource-type	Dataset
source_datajson_identifier	true
source_hash	4e98f19aaaaed13fb5fc0c2499a3d807e78466f1d16fe4d310c1980d4cbf4007
source_schema_version	1.1
temporal	2006-10-01/2014-09-27
theme	{Heliophysics}