Accessibility navigation


Ion charge states and potential geoeffectiveness: the role of coronal spectroscopy for space-weather forecasting

Owens, M. J., Lockwood, M. and Barnard, L. A. (2018) Ion charge states and potential geoeffectiveness: the role of coronal spectroscopy for space-weather forecasting. Space Weather, 16 (6). pp. 694-703. ISSN 1542-7390

[img]
Preview
Text - Published Version
· Please see our End User Agreement before downloading.

1MB
[img] Text - Accepted Version
· Restricted to Repository staff only

3MB

It is advisable to refer to the publisher's version if you intend to cite from this work. See Guidance on citing.

To link to this item DOI: 10.1029/2018SW001855

Abstract/Summary

Severe space-weather is driven by interplanetary coronal mass ejections (ICMEs), episodic eruptions of solar plasma and magnetic flux that travel out through the heliosphere and can perturb the Earth’s magnetosphere, ionosphere and upper atmosphere. In order for space-weather forecasts to allow effective mitigating action, forecasts must be made as early as possible, necessitating identification of potentially “geoeffective” ICMEs close to the Sun. This presents two challenges. Firstly, geoeffectiveness is primarily determined by the magnetic field intensity and orientation, both of which are difficult to measure close to the Sun. Secondly, the magnetic field evolves in transit between the Sun and the Earth, sometimes in a highly non-linear way. Conversely, solar wind ion charge states, such as the ratio of O7+ to O6+, can be observed near the Sun through coronal spectroscopy and are fixed by the electron temperature at the coronal height where ion-electron collisions are last possible as the ICME erupts. After this point, they are said to be “frozen in” as they do not evolve further as the ICME propagates through the solar wind. In this study we show that ions charge states, while not geoeffective in and of themselves, act as strong markers for the geoeffectiveness of the ICME. The probability of severe space weather is around seven times higher in “hot” ICMEs than “cold” ICMEs, as defined by O7+/O6+. We suggest that coronal spectroscopy of ICMEs could complement current forecasting techniques, providing valuable additional information about potential geoeffectiveness.

Item Type:Article
Refereed:Yes
Divisions:Faculty of Science > School of Mathematical, Physical and Computational Sciences > Department of Meteorology
ID Code:77449
Publisher:American Geophysical Union

Downloads

Downloads per month over past year

University Staff: Request a correction | Centaur Editors: Update this record

Page navigation