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Statistical analysis of magnetopause crossings at lunar distances
<p><strong>Abstract.</strong> Different magnetopause models with a diverse level of complexity are in use. One thing that they have in common is that they are mainly based on near-earth observations; i.e. they use measurements at distances of about <span class="inline-formula">±10</span> Earth radii along the GSM <span class="inline-formula"><i>x</i></span> axis. Only very few observations of magnetopause crossings at larger distances are used for model fitting. In this study we comparedoi:10.5194/angeo-37-163-2019 fatcat:5u3wopmyzvajfkjaywpgnts7yy