Calculating travel times and arrival speeds of CMEs to Earth: An analytic tool for space weather forecasting


Por: Corona-Romero, P., Gonzalez-Esparza, J. A., Perez-Alanis, C. A., Aguilar-Rodriguez, E., de-la-Luz, V., Mejia-Ambriz, J. C.

Publicada: 1 mar 2017
Categoría: Atmospheric science

Resumen:
Coronal mass ejections (CME) are one of the most important phenomena derived from solar activity that potentially perturb space weather of Earth. In this work we present a semiempirical arrival forecasting tool for Earth-directed halo CMEs. This tool combines the piston shock model and an empirical relationship to estimate in situ arrivals of halo CMEs. The empirical relationship uses the initial conditions of CMEs to calculate the value of free parameter of the piston shock model, a parameter which is closely related to the initial inertia of CMEs. Such a value will let the model to simultaneously approximate the travel time and arrival speed of CMEs (i.e., CME arrivals). We test the forecasting capabilities of our model and its empirical relationship by calculating the arrivals of 40 halo CMEs detected during the period of 1995-2015. Our results indicate that, together, the piston shock model and its empirical relationship approximate CME arrivals with average errors of 7h for travel times, and 100kms(-1) for arrival speeds. Our results show that our model is suitable for arrival forecasting of isolated events propagating through quiet interplanetary medium.

Filiaciones:
Corona-Romero, P.:
 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Space Weather Serv Mexico SCiESMEX, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, CONACYT, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Space Weather Natl Lab LANCE, Morelia, Michoacan, Mexico

Gonzalez-Esparza, J. A.:
 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Space Weather Serv Mexico SCiESMEX, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Space Weather Natl Lab LANCE, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Morelia, Michoacan, Mexico

Perez-Alanis, C. A.:
 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Posgrad Ciencias Tierra, Mexico City, DF, Mexico

Aguilar-Rodriguez, E.:
 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Space Weather Serv Mexico SCiESMEX, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Space Weather Natl Lab LANCE, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Morelia, Michoacan, Mexico

de-la-Luz, V.:
 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Space Weather Serv Mexico SCiESMEX, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, CONACYT, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Space Weather Natl Lab LANCE, Morelia, Michoacan, Mexico

Mejia-Ambriz, J. C.:
 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Space Weather Serv Mexico SCiESMEX, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, CONACYT, Morelia, Michoacan, Mexico

 Univ Nacl Autonoma Mexico, Inst Geofis, Unidad Michoacan, Space Weather Natl Lab LANCE, Morelia, Michoacan, Mexico
ISSN: 15427390
Editorial
AMER GEOPHYSICAL UNION, 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA, Estados Unidos America
Tipo de documento: Article
Volumen: 15 Número: 3
Páginas: 464-483
WOS Id: 000399447600001