Articles | Volume 38, issue 3
https://doi.org/10.5194/angeo-38-657-2020
https://doi.org/10.5194/angeo-38-657-2020
Regular paper
 | 
05 Jun 2020
Regular paper |  | 05 Jun 2020

Development of a formalism for computing in situ transits of Earth-directed CMEs – Part 2: Towards a forecasting tool

Pedro Corona-Romero and Pete Riley

Data sets

A catalog of white light coronal mass ejections observed by the SOHO spacecraft Yashiro, S., Gopalswamy, N., Michalek, G., St. Cyr, O. C., Plunkett, S. P., Rich, N. B., and Howard, R. A. https://doi.org/10.1029/2003JA010282

The SOHO/LASCO CME Catalog, Earth Moon and Planets Gopalswamy, N., Yashiro, S., Michalek, G., Stenborg, G., Vourlidas, A., Freeland, S., and Howard, R. https://doi.org/10.1007/s11038-008-9282-7

Near-Earth Interplanetary Coronal Mass Ejections During Solar Cycle 23 (1996 - 2009): Catalog and 925 Summary of Properties Richardson, I. G. and Cane, H. V. https://doi.org/10.1007/s11207-010-9568-6

Model code and software

High resolution OMNI (HRO) data NASA Goddard Space Flight Center https://spdf.gsfc.nasa.gov/pub/data/omni/high_res_omni/

Low resolution OMNI (HRO) data NASA Goddard Space Flight Center https://spdf.gsfc.nasa.gov/pub/data/omni/low_res_omni/

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Short summary
Solar storms are natural phenomena that affect technologies on which our societies are highly dependent. The understanding of solar storms and the capability to anticipate their effects on our technologies is of main interest to shield our societies. In this work we present a semi-empirical approach to increase our understanding of solar storms when they hit our planet. Additionally, we also preset a possible pathway to forecast the transits of solar storms by our planet's orbit.