Solar wind plasma and magnetic field observations from 5 November until 9 November 2013 observed by STB a) and STA b). The top panel shows 145−165 keV electrons observed by SEPT in its four viewing directions. The panel below plots the pitch angles of the four SEPT telescopes. Below the latitudinal and azimuthal angle of the magnetic field in RTN coordinates are shown the magnetic field magnitude, the plasma beta, the solar wind proton temperature, the proton density, and the solar wind speed. The red/green bar at the bottom represents the in situ polarity of the magnetic field with red (green) standing for negative (positive) polarity and yellow meaning uncertain periods. The shaded range in a) marks the duration of an ICME as listed in the ICME catalog by Lan Jian⁴ with a magnetic obstacle (identified as a magnetic-cloud-like structure, labeled MCL) between the second and third vertical lines. The red dashed line (labeled S) indicates the associated CME-driven shock listed in the Jian shock list. The shaded range in b) indicates a SIR as listed in the Jian SIR catalog. Two shocks (labeled S, from the Jian catalog) pass STA at the beginning of the SIR.