Abstract
[1] In the paper “Magnetospheric cavity modes driven by solar wind dynamic pressure fluctuations” by S. G. Claudepierre et al. (Geophysical Research Letters, 36, L13101, doi:10.1029/2009GL039045) the acknowledgments should appear as follows. The authors are grateful for thoughtful discussions with R. E. Denton and J. G. Lyon. This work was supported by the New Hampshire NASA Space grant NNG05GG76H and by the Center for Integrated Space Weather Modeling funded by the NSF STC program under cooperative agreement ATM-0120950.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
