View in EDS HTML Full Text PDF Full Text

Whistler wave mode generation via large amplitude steepened magnetic structures propagating through the Martian ionosphere.

Saved in:
Bibliographic Details
Title: Whistler wave mode generation via large amplitude steepened magnetic structures propagating through the Martian ionosphere.
Authors: Fowler, C. M.1 (AUTHOR) christopher.fowler@mail.wvu.edu, Hanley, K. G.2 (AUTHOR), Halekas, J.3 (AUTHOR), Regan, C. E.1 (AUTHOR), McFadden, J.2 (AUTHOR), Mitchell, D.2 (AUTHOR), Andersson, L.4 (AUTHOR), Bark, D.4 (AUTHOR), Harada, Y.5 (AUTHOR), Ma, Y.6 (AUTHOR), Chaston, C.2 (AUTHOR), Sanchez-Cano, B.7 (AUTHOR), Lester, M.7 (AUTHOR), Brain, D.4 (AUTHOR), Mazelle, C.8 (AUTHOR), Espley, J.9 (AUTHOR), Benna, M.9 (AUTHOR), Jolitz, R.2 (AUTHOR), Curry, S.4 (AUTHOR)
Source: Frontiers in Astronomy & Space Sciences. 2026, p1-16. 16p.
Database: Academic Search Ultimate
Full text is not displayed to guests.
Description
ISSN:2296987X
DOI:10.3389/fspas.2025.1688155