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Sunquakes (SQs) have been routinely observed in the solar photosphere, but itis only recently that signatures of these events have been detected in thechromosphere. We investigate whether signatures of SQs are common inUltraviolet (UV) continua, which sample the solar plasma several hundred kmabove where SQs are typically detected. We analyse observations from the SolarDynamics Observatory's Atmospheric Imaging Assembly (SDO/AIA) 1600 {\AA} and1700 {\AA} passbands, for SQ signatures induced by the flares of Solar Cycle24. We base our analysis on the 62 SQs detected in the recent statistical studypresented by Sharykin & Zosovichev (2020). We find that 9 out of 62 SQcandidates produced a response that is clearly detected in running differenceimages from the AIA 1600 {\AA} and 1700 {\AA} channels. A binary frequencyfilter with a width of 2 mHz, centred on 6 mHz, was applied to the data. Thefirst signature of each SQ was detected at distances between 5.2 Mm to 25.7 Mmfrom the associated flare ribbon. Time-distance and regression analysis allowedus to calculate the apparent transverse velocities of the SQs in the UVdatasets and found maximum velocities as high as 41 km s-1, 87 Mm away from theSQ source. Our analysis shows that flare induced SQ signatures can be detectedin the SDO/AIA 1600 {\AA} and 1700 {\AA} passbands, hinting at their presencein the lower chromosphere. There was no apparent correlation between GOES flareclassification, and the appearance of the SQ at these heights.

Flare Induced Sunquake Signatures in the Ultraviolet as Observed by the Atmospheric Imaging Assembly