Artists impression of the twin STEREO satellites

The Heliospheric Imager for the NASA STEREO Mission

Part of the SECCHI Consortium

An analysis of inconsistent visible-light imaging observations

Coronal Mass Ejections (CMEs) can impact human activities and technological assets and are continuously monitored by dedicated space weather operations centers. A study by Harrison et al. 2023, Space Weather 21, 10.1029/2022SW003358 identifies inconsistencies between the identification of potentially Earth-directed CMEs in observations made from a near-Earth vantage point and those made from off the Sun-Earth line. Almost a third of a set of potentially Earth-directed CMEs that were identified in an off Sun-Earth line heliospheric imager catalog from 2011, which were subsequently evidenced as Interplanetary CMEs (ICMEs) in in-situ data near Earth, were not cataloged as halo or partial halo events in near Earth coronagraph imagery. Given the number of such discrepant events, compared to the total number of ICMEs recorded near Earth in 2011, it is important to understand the inconsistencies and to ensure that future space weather monitoring strategies cater for them.

HI and COR images of CMEs
HI-1A (left), HI-1B (middle) and COR-2A (right) difference images for the events first observed in HI data on 3 July (CME 9; top), 26 October (CME 12; middle) and 29 November (CME 13; bottom), 2011.

The first comprehensive catalogue of CMEs in the heliosphere

Harrison et al. 2018, Solar Phys. 293, 77, 10.1007/s11207-018-1297-2 present, and analyse, the first catalogue of heliospheric CMEs based on STEREO/HI-1 imagery. The authors present distributions of the basic observational CME parameters – namely occurrence frequency, central PA and PA span – from over 2000 CME detections over the majority of solar cycle 24 (April 2007 to August 2017). These distributions are compared to those of CMEs at coronal altitudes, and sunspot number, providing valuable insights to the launch and propagation of CMEs.

Analysis was based on the HICAT catalogue, which was generated within the EU FP7 HELCATS project.

hicat cmes
Histogram of daily-average rates of HICAT CMEs detected by (a) STEREO/HI-1A and (b) STEREO/HI-1B compared to coronal CME rates from (c) STEREO/COR-2A and (d) STEREO/COR-2B and (e) SOHO/LASCO. Panel (f) shows the monthly sunspot count over the same period. HI CME catalogue

Using heliospheric imaging for space weather application

A landmark paper Harrison et al. 2017, Space Weather 15, 985, 10.1002/2017SW001633 considers lessons learnt from published studies of heliospheric imagery in the context of its application to space weather. This work reviews a cross section of scientific analyses that have exploited STEREO/HI imagery, in particular, and discusses their relevance to operational predictions of CME arrivals at Earth and elsewhere.

The authors assert that the potential benefit of heliospheric images to the provision of accurate CME arrival predictions on an operational basis, although as yet not fully realized, is significant and assert that heliospheric imagery is central to any credible space weather mission, particularly one located at a vantage point off the Sun-Earth line.

CME Images from STEREO
A sequence of six images from February 2011 illustrating the passage of a CME through the combined STEREO-A COR2, HI-1 and HI-2 field-of-view. The white near horizontal line denotes the position angle of Earth; the location of Earth corresponds to the white dot at the intersection of that line with the near-vertical curve. HI SpaceWeather