Cite
Coexistence of Earth-origin O+ and solar wind-origin H+/He++ in the distant magnetotail.
MLA
Seki, K., et al. “Coexistence of Earth-Origin O+ and Solar Wind-Origin H+/He++ in the Distant Magnetotail.” Geophysical Research Letters, vol. 23, no. 9, May 1996, pp. 985–88. EBSCOhost, https://doi.org/10.1029/96GL00768.
APA
Seki, K., Hirahara, M., Terasawa, T., Shinohara, I., Mukai, T., Saito, Y., Machida, S., Yamamoto, T., & Kokubun, S. (1996). Coexistence of Earth-origin O+ and solar wind-origin H+/He++ in the distant magnetotail. Geophysical Research Letters, 23(9), 985–988. https://doi.org/10.1029/96GL00768
Chicago
Seki, K., M. Hirahara, T. Terasawa, I. Shinohara, T. Mukai, Y. Saito, S. Machida, T. Yamamoto, and S. Kokubun. 1996. “Coexistence of Earth-Origin O+ and Solar Wind-Origin H+/He++ in the Distant Magnetotail.” Geophysical Research Letters 23 (9): 985–88. doi:10.1029/96GL00768.