Abstract: I will present a rapid sequence of near-relativistic solar electron events observed on November 9 to 15, 2022 by STEREO-A at 0.96 au, by near-Earth spacecraft such as ACE, Wind and SOHO at ∼0.99 au, and by Solar Orbiter at heliocentric distances ranging from 0.59 to 0.66 au. At least 23 electron intensity enhancements at energies >10 keV were clearly distinguishable in the particle data collected by the Energetic Particle Detector (EPD) suite of instruments on board Solar Orbiter, with 12 of these events occurring on 11 November 2022. Several of these electron events were accompanied by <10 MeV proton and <∼2 MeV/n heavy ion intensity enhancements. I will describe the origin of this rapid succession of particle events. A series of jet-like eruptions detected in extreme ultraviolet (EUV) observations occurred in association with Hard X-ray (HXR) flares and type III radio bursts in the decametric-hectometric range.  The events on 9 November and late on 14 November are particularly interesting in that they were just evident at electron energies below ∼40 keV, were rich in heavy ions with energies below ∼1 MeV/n, associated with type III radio bursts at frequencies below ∼1.0 MHz, and originated at EUV solar eruptions lacking a clear jet. By combining remote and in-situ data from the three viewpoints (Solar Orbiter and STEREO-A were ∼20 degrees and ∼15 degrees east of Earth, respectively), we analyze the origin of this sequence of events, determine the interplanetary context where they were observed, and investigate the interplanetary transport of electrons to the different spacecraft.