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Table 1.

Eruption features observed in the EUV and white-light coronagraph data by SDO/AIA, STEREO A/SECCHI EUVI and COR2, and SOHO/LASCO instruments.

Eruption Observational features and observation times

SDO AIA STEREO A STEREO A COR 2 SOHO LASCO C2
193 Å EUVI 195 Å (ϕ = 134°) (ϕ = 0°)
(ϕ = 0°) (ϕ = 134°)
EUV loop expansion 08:40 UT 08:50 UT COR Blob 1 09:54 UT (PA ∼ 94°) CME 09:48 UT (PA ∼ 261°)
and disappearance COR Blob 2 10:24 UT (PA ∼ 68°) CME 11:12 UT (PA ∼ 328°)
between western
sunspot and bipole

Expulsion of 09:07 UT 09:20 UT COR Blob 3 10:39 UT (PA ∼ 109°)
chromospheric/low-coronal
material between western
sunspot and bipole

M1.0 flare at 10:22 UT Possibly related COR Blob 4 11:24 UT (PA ∼ 53°) CME 11:12 UT (PA ∼ 328°)
the eastern end weak dimming
of the AR 10:30 UT →

Flare and an EUV N/A 08:50 UT COR Blob 1 09:54 UT (PA ∼ 94°) CME 09:48 UT (PA ∼ 261°)
eruption at the
center of STEREO A
solar disk

Notes. The first column lists the low-coronal eruption features as observed by SDO/AIA (second column) or STEREO A SECCHI EUVI (third column), whereas the final two columns show the possibly associated eruption features and their detection times in STEREO A COR 2 and SOHO/LASCO C2 data. The Stonyhurst heliographic longitudes ϕ for each instrument are listed in the second row. The initial detection of each observational feature is written in bold in the column of the observing instrument. The first three rows show the eruption features possibly related to activity at AR11726, and the final row shows the features possibly related to the eruption that occurred at the center of STEREO A solar disk. We note that since we could not make unique connections between all low-coronal EUV and white-light coronagraph features, some of the latter are listed several times.

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