Forerunners: Outer rims of solar coronal transients

The large loop or blob-like transient events viewed in the white-light corona are rimmed by broad regions where the density is slightly enhanced above the pretransient corona. Every one of the Skylab events studied, for which sufficiently good Skylab coronagraph coverage is available, shows this effect. The upper boundaries of these forerunners blend gradually into the background corona 1 to greater than or equal to 2R[moonface] above the transients' leading edges. In any single event, the coronal mass enhancement represented by the forerunner is comprised of up to 25% of the total excess mass present in the field of view of the coronagraph, and includes a much larger volume of the corona than previously attributed to the underlying transient. A forerunner without an accompanying transient has not yet been seen. Clearly, forerunners must be reckoned with in any proposed models of discrete outward coronal mass motions because they indicate the presence of disturbed corona far ahead of the denser portions of the event.