An improved empirical model of electron and ion fluxes at geosynchronous orbit based on upstream solar wind conditions.

MLA

Denton, M. H., et al. “An Improved Empirical Model of Electron and Ion Fluxes at Geosynchronous Orbit Based on Upstream Solar Wind Conditions.” Space Weather: The International Journal of Research & Applications, vol. 14, no. 7, July 2016, pp. 511–23. EBSCOhost, https://doi.org/10.1002/2016SW001409.

APA

Denton, M. H., Henderson, M. G., Jordanova, V. K., Thomsen, M. F., Borovsky, J. E., Woodroffe, J., Hartley, D. P., & Pitchford, D. (2016). An improved empirical model of electron and ion fluxes at geosynchronous orbit based on upstream solar wind conditions. Space Weather: The International Journal of Research & Applications, 14(7), 511–523. https://doi.org/10.1002/2016SW001409

Chicago

Denton, M. H., M. G. Henderson, V. K. Jordanova, M. F. Thomsen, J. E. Borovsky, J. Woodroffe, D. P. Hartley, and D. Pitchford. 2016. “An Improved Empirical Model of Electron and Ion Fluxes at Geosynchronous Orbit Based on Upstream Solar Wind Conditions.” Space Weather: The International Journal of Research & Applications 14 (7): 511–23. doi:10.1002/2016SW001409.