The EISCAT BLOB experiment has been designed to study structuring of t
he plasma in the auroral ionosphere on scales of tens of kilometres tr
ansverse to the magnetic field. Results are presented from the initial
observations that show three different types of field-aligned irregul
arities occurring within a time interval of about two hours. The first
type appears to be a long-lived boundary blob of cold plasma convecti
ng through the field of view. The others show evidence of in-situ form
ation. A narrow density enhancement, associated initially with high el
ectron temperatures, appears to originate and develop from a localised
particle precipitation event. In the third category the irregularity
takes the form of a narrow trough in electron density with high ion te
mperatures caused by ion-frictional heating in a fast convective flow.