Abstract
The shape and location of the magnetopause current sheet in the near-cusp region is still a debated question. Over time, several observations led to contradictory conclusions regarding the presence of an indentation of the magnetopause in that region. As a result several empirical models consider the surface is indented in that region, while some others do not. To tackle this issue, we fit a total of 17,230 magnetopause crossings to various indented and non-indented analytical models. The results show that while all models describe the magnetopause position and shape equivalently far from the cusp region, the non-indented version over-estimate the radial position of the near-cusp magnetopause. Among indented models, we show that the one designed from non-linearmagneto hydrodynamic simulations fits well the near-cusp magnetopause location, while the other underestimate its position probably because their design was possibly based on magnetopause crossing catalogs that contain cusp inner boundary crossings.
| Original language | English |
|---|---|
| Article number | e2021JA029776 |
| Journal | Journal of Geophysical Research: Space Physics |
| Volume | 127 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 1 Jan 2022 |
Keywords
- magnetopause
- magnetosphere
- polar cusps
- solar wind
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