Columns Description 2-5 Type of event and satellites involved. An occultation (``O'') can either be partial (``P''), total (``T'') or annular (``A''). An eclipse (``E'') can either be penumbral (``P''), umbral (``U''), total (``T'') or annular (``A''). Grazing (``G'') events are allowable given the ephemeris uncertainties. Satellite identification is as follows: Ariel (1), Umbriel (2), Titania (3), Oberon (4), Miranda (5). 8-11 Year (YYYY) 13-15 Month (MMM) 17-18 Day (DD). Note that date corresponds to event start. 21-28 Penumbra ingress time (eclipses only). Note that all times are given in UTC with deltaT fixed at 64.184 sec. 31-38 Umbra Ingress (eclipses) or Partial event start (occultations). 41-48 Start of Totality or Annularity. 51-58 Middle of event 61-68 End of Totality or Annularity. 71-78 Umbra Egress (eclipses) or Partial event end (occultations). 81-88 Penumbra egress time (eclipses only). 93-96 Time between penumbra ingress and egress (eclipses only). 100-103 Time between umbra ingress and egress (eclipses) or partial phase start and end (occultations). 107-110 Duration of totality/annularity. 113-117 Impact parameter in units of the eclipsed/occulted satellite's apparent radius. 120-124 Fractional drop in light flux of eclipsed satellite. 127-131 Fractional drop in cumulative flux of satellites involved in event (occultations and eclipses). 134-136 Distance from uranian limb at onset of event in units of the apparent planetary radius.