M, D., D, S., C, Z., Z, M., N, S., & H, B. (2026). Partially melted low velocity zones reveal an active upper mantle beneath Elysium Planitia, Mars. Nature communications, 17(1), . https://doi.org/10.1038/s41467-026-72209-x
Chicago Style (17th ed.) CitationM, Dai, Sun D, Zhao C, Mao Z, Sun N, and Bi H. "Partially Melted Low Velocity Zones Reveal an Active Upper Mantle Beneath Elysium Planitia, Mars." Nature Communications 17, no. 1 (2026). https://doi.org/10.1038/s41467-026-72209-x.
MLA (9th ed.) CitationM, Dai, et al. "Partially Melted Low Velocity Zones Reveal an Active Upper Mantle Beneath Elysium Planitia, Mars." Nature Communications, vol. 17, no. 1, 2026, https://doi.org/10.1038/s41467-026-72209-x.
Warning: These citations may not always be 100% accurate.