loading page

Predicting the Time-of-Arrival of Coronal Mass Ejections at Earth Solely From Heliospheric Imaging Observations
  • +3
  • Carlos Roberto Braga,
  • Angelos Vourlidas,
  • Guillermo Stenborg,
  • Alisson Dal Lago,
  • Rafael R. S. Mendonca,
  • Ezequiel Echer
Carlos Roberto Braga
George Mason University

Corresponding Author:[email protected]

Author Profile
Angelos Vourlidas
Author Profile
Guillermo Stenborg
Author Profile
Alisson Dal Lago
National Institute for Space Research (INPE)
Author Profile
Rafael R. S. Mendonca
INPE - National Institute for Space Research
Author Profile
Ezequiel Echer
National Institute for Space Research (INPE)
Author Profile


The Time-of-Arrival (ToA) of coronal mass ejections (CME) at Earth is a key parameter due to the space weather phenomena associated with the CME arrival, such as intense geomagnetic storms. Several approaches to estimate the ToA based on kinematical parameters derived from single- and multi-viewpoint white-light coronagraph observations have been proposed and implemented, particularly in the last decade. Despite the incremental use of new instrumentation and the development of novel methodologies, ToA estimated errors remain above 10 hours on average. Here, we investigate the prediction of ToA of CMEs using observations solely from heliospheric imagers, i.e., from heliocentric distances higher than those covered by the existent coronagraphs. To that aim, we analyse 14 CMEs observed by the heliospheric imager HI-1 onboard the twin STEREO spacecraft to determine their front location and speed. Outside the field of view of the instruments, we assume that the dynamics of the CME evolution is controlled by the aerodynamic drag, a force that comes from the interaction with particles from the background solar wind. We found a CME ToA error mean value of 0.4+-7.3 hours ToA and a mean absolute error of 6.1+-3.6 hours in a set of 14 events. The results we found here illustrate that observations from HI-1 allow us to estimate the ToA with similar errors than observations from coronagraphs.
Sep 2020Published in Journal of Geophysical Research: Space Physics volume 125 issue 9. 10.1029/2020JA027885