NTRS - NASA Technical Reports Server

As of October 27, 2023, NASA STI Services will no longer have an embargo for accepted manuscripts. For more information visit NTRS News.

Back to Results
Combining Stereo SECCHI COR2 and HI1 Images for Automatic CME Front Edge TrackingCOR2 coronagraph images are the most commonly used data for coronal mass ejection (CME) analysis among the various types of data provided by the STEREO (Solar Terrestrial Relations Observatory) SECCHI (Sun-Earth Connection Coronal and Heliospheric Investigation) suite of instruments. The field of view (FOV) in COR2 images covers 215 solar radii (Rs) that allow for tracking the front edge of a CME in its initial stage to forecast the lead-time of a CME and its chances of reaching the Earth. However, estimating the lead-time of a CME using COR2 images gives a larger lead-time, which may be associated with greater uncertainty. To reduce this uncertainty, CME front edge tracking should be continued beyond the FOV of COR2 images. Therefore, heliospheric imager (HI1) data that covers 1590 Rs FOV must be included. In this paper, we propose a novel automatic method that takes both COR2 and HI1 images into account and combine the results to track the front edges of a CME continuously. The method consists of two modules: pre-processing and tracking. The pre-processing module produces a set of segmented images, which contain the signature of a CME, for both COR2 and HI1 separately. In addition, the HI1 images are resized and padded, so that the center of the Sun is the central coordinate of the resized HI1 images. The resulting COR2 andHI1 image set is then fed into the tracking module to estimate the position angle (PA) and track the front edge of a CME. The detected front edge is then used to produce a height-time profile that is used to estimate the speed of a CME. The method was validated using 15 CME events observed in the period from January 1, 2008 to August 31, 2009. The results demonstrate that the proposed method is effective for CME front edge tracking in both COR2 and HI1 images. Using this method, the CME front edge can now be tracked automatically and continuously in a much larger range, i.e., from 2 to 90 Rs, for the first time. These improvement scan greatly help in making the quantitative CME analysis more accurate and have the potential to assist in space weather forecasting.
Document ID
Document Type
Reprint (Version printed in journal)
External Source(s)
Kirnosov, Vladimir
(Catholic Univ. of America Washington, DC, United States)
Chang, Lin-Ching
(Catholic Univ. of America Washington, DC, United States)
Pulkkinen, Antti
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Date Acquired
June 1, 2017
Publication Date
December 21, 2016
Publication Information
Publication: Journal of Space Weather and Space Climate
Publisher: EDP Sciences
Volume: 6
e-ISSN: 2115-7251
Subject Category
Space Sciences (General)
Instrumentation And Photography
Report/Patent Number
Distribution Limits

Available Downloads

There are no available downloads for this record.
No Preview Available