The dawn–dusk confinement of magnetic reconnection site in the near-Earth magnetotail is established on the basis of Geotail observations. Geotail has made more than 50 encounters with magnetic reconnection in association with the onset of substorms in the near-Earth magnetotail at radial distances of 20–30 RE in the period of 1994–2019. Ground magnetic field observations are examined for these events, and geosynchronous spacecraft observations are investigated for a limited number of cases. The magnetic reconnection site is located in the upward (from the ionosphere to the tail) field-aligned current part of large-scale substorm current system derived from ground mid-latitude magnetic variations. The site is confined to the localized dawn–dusk extent of the 1-h local time, just west of the center of the large-scale substorm current system. The short dawn-dusk length of the X-line implies that magnetic reconnection inherently proceeds as the two-dimensional dynamics in the magnetotail meridional plane. Rapid dipolarization with upward field-aligned currents occurs at geosynchronous altitude near the meridian of the magnetic reconnection site. This study demonstrates that rapid dipolarization in the inner magnetosphere is produced with earthward outflows from magnetic reconnection and that intense upward field-aligned currents are a direct consequence of magnetic reconnection.