Fig. 1.

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In situ magnetic field measurements in local radial tangential normal (RTN) coordinates from Solar Orbiter (a/e), BepiColombo (b/f), and Wind (c/g) for the 2020 April 20 (left) and 2020 May 28 (right) event. The two bottom panels (d/h) show the in situ proton density number Np and the associated plasma beta coefficient, βp. The blue shaded area represents our estimated intervals for the unperturbed magnetic flux ropes (UMFR) which we subsequently use in our fitting approach.

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