A pair of relatively mild geomagnetic storms of February 3–4, 2022, resulted in the loss of 38 Starlink satellites. In this work we reconstruct a sequence of magnetospheric configurations during that event, based on the largest ever archive of historical data, a new magnetic field model, and the nearest‐neighbor method of mining the solar wind, magnetosphere, and ground activity data. The model is constructed as a combination of main modular framework, explicitly representing magnetic effects of principal current systems, and a high‐resolution superstructure, based on expanding the field of equatorial currents into a sum of quasi‐orthogonal harmonics, whose purpose is to correct residual inaccuracies of the modular component. In addition, the variable penetration of the interplanetary magnetic field (IMF) into the magnetosphere is taken into account in the form of a potential field, parameterized by the observed IMF components. Despite relatively modest intensity of the event in terms of Sym‐H peak values, surprisingly strong transient distortions of the global magnetic field are found. Whereas under quiet pre‐storm conditions the midnight segment of synchronous orbit and the dayside cusps mapped, respectively, to ∼67° and ∼77° of corrected latitude, at the peak of the storm their footpoints shifted equatorward to as low as ∼63° and ∼67°–68°, with formation of entangled flux‐rope‐like structures and magnetic neutral lines at distances R∼ 12–15 REon the nightside. At nearly the same time, a deep magnetic depression and, possibly, an island of reversed field polarity forms even closer, in the post‐dusk sector of geosynchronous orbit. In the beginning of February 2022, a relatively weak geomagnetic storm broke out, whose unexpected result was a premature demise of 38 Starlink satellites due to their abnormal drag in the upper atmosphere. This work analyses the concurrent distortions of the distant geomagnetic field, caused by the arrival of disturbed solar wind and interplanetary magnetic field. The storm‐time deformations of the Earth's magnetosphere are reconstructed by using an advanced magnetic field model, a huge database of past spacecraft and ground‐based observations covering the last 27 years, and novel methods of data mining. Strong distortions of the geomagnetic field during the storm culmination are revealed, that penetrated to unusually close distances up to the geosynchronous orbit. Dynamics of global geomagnetic connectivity during the ill‐famed storms of February 2022 is reconstructed via mining archived in situ dataA new hybrid model architecture is employed, combining flexible modular and high‐resolution components with added interplanetary magnetic field penetration effectDeep magnetic depression and possibly a neutral line formed in the post‐dusk sector around geosynchronous distance at the storm active phase Dynamics of global geomagnetic connectivity during the ill‐famed storms of February 2022 is reconstructed via mining archived in situ data A new hybrid model architecture is employed, combining flexible modular and high‐resolution components with added interplanetary magnetic field penetration effect Deep magnetic depression and possibly a neutral line formed in the post‐dusk sector around geosynchronous distance at the storm active phase