Multi-Spacecraft Observations of the September 05, 2022 CME

Combination of in situ data, remote sensing observations, and CME modeling for the ICME on 2022 September 05. (a) Running difference COR2 image from STEREO-A at 19:11 UT, where the location of PSP is represented by the white asterisk. (b) The combined WISPR FOV, overlaid on a grid of heliocentric longitude and latitude. (c) PSP orbital trajectory in HEEQ coordinates, with CME1 in blue and CME2 in red. The orbital location of Solar Orbiter (SOLO), STEREO-A (STA), and Earth are shown by black arrows. (d) In situ measurements observed by PSP. From top to bottom, the electron density from QTN (blue) and SPAN-E (red), solar wind velocity spectra from SPAN-I, RTN magnetic field vector with magnitude (black), and normalized ePADs measured at 433 eV. The vertical black line indicates the current time in the animation. An animation of this figure is also available in the online Journal, spanning from 22-09-05/16:00 to 22-09-07/12:00~UT, syncing the different cadence rates of the coronagraph imaging, in situ measurements, and CME modeling.