LAUSR

The efficacy of coronal mass ejection (CME) observations as a key input to space weather forecasting is explored by comparing on and off Sun‐Earth line observations from the ESA/NASA SOHO and NASA STEREO spacecraft. A comparison is made of CME catalogs based on L1 coronagraph imagery and off Sun‐Earth line coronagraph and heliospheric imager observations, for the year 2011. Analysis reveals inconsistencies in the identification of a number of potentially Earth‐directed CMEs. The catalogs reflect our ability to identify and characterize CMEs, so any discrepancies can impact our prediction of Earth‐directed CMEs. We show that 15 CMEs, which were observed by STEREO, that had estimated directions compatible with Earth‐directed events, had no identified halo/partial halo counterpart listed in the L1 coronagraph CME catalog. In situ data confirms that for 9 of these there was a consistent L1 Interplanetary CME (ICME). The number of such “discrepant” events is significant compared to the number of ICMEs recorded at L1 in 2011, stressing the need to address space weather monitoring capabilities, particularly with the inclusion of off Sun‐Earth line observation. While the study provides evidence that some halo CMEs are simply not visible in near‐Earth coronagraph imagery, there is evidence that some halo CMEs viewed from L1 are compromised by preceding CME remnants or the presence of multiple‐CMEs. This underlines (a) the value of multiple vantage point CME observation, and (b) the benefit of off Sun‐Earth line platform heliospheric imaging, and coronagraph imaging, for the efficient identification and tracking of Earth‐directed events.