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On 2018 November 5, about 24 hours before the first close perihelion passageof Parker Solar Probe (PSP), a coronal mass ejection (CME) entered the field ofview of the inner detector of the Wide-field Imager for Solar PRobe (WISPR)instrument onboard PSP, with the northward component of its trajectory carryingthe leading edge of the CME off the top edge of the detector about four hoursafter its first appearance. We connect this event to a very small jet-liketransient observed from 1 au by coronagraphs on both the SOlar and HeliosphericObservatory (SOHO) and the A component of the Solar TErrestrial RElationsObservatory mission (STEREO-A). This allows us to make the firstthree-dimensional reconstruction of a CME structure considering bothobservations made very close to the Sun and images from two observatories at 1au. The CME may be small and jet-like as viewed from 1 au, but the close-invantage point of PSP/WISPR demonstrates that it is not intrinsically jet-like,but instead has a structure consistent with a flux rope morphology. Based onits appearance in the SOHO and STEREO-A images, the event belongs in the"streamer blob" class of transients, but its kinematic behavior is veryunusual, with a more impulsive acceleration than previously studied blobs.

Morphological Reconstruction of a Small Transient Observed by Parker Solar Probe on 2018 November 5