Articles | Volume 26, issue 8
https://doi.org/10.5194/angeo-26-2383-2008
© Author(s) 2008. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-26-2383-2008
© Author(s) 2008. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
05 Aug 2008
What is the best method to calculate the solar wind propagation delay?
B. Mailyan
Yerevan State University, Armenia
C. Munteanu
Alexandru Ioan Cuza, University Iasi, Romania
S. Haaland
University of Bergen, Norway
also at: Max-Planck Institute for Solar Systems, Germany
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- Statistical study on ultralow‐frequency waves in the magnetotail lobe observed by Cluster G. Wang et al. https://doi.org/10.1002/2016JA022533
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- On magnetopause inflation under radial IMF A. Suvorova & A. Dmitriev https://doi.org/10.1016/j.asr.2015.07.044
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- Forecasting Kp from solar wind data: input parameter study using 3-hour averages and 3-hour range values P. Wintoft et al. https://doi.org/10.1051/swsc/2017027
- Global Energy Dynamics During Substorms on 9 March 2008 and 26 February 2008 Using Satellite Observations and the WINDMI Model E. Spencer et al. https://doi.org/10.1029/2018JA025582
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Latest update: 02 Jul 2026
