Table 1.
Summary table.
Event no. | CME1.1 | CME1.2 | CME1.3 | CME1.4 | CME2.1 | CME2.2 | CME2.3 | CME2.4+5 |
---|---|---|---|---|---|---|---|---|
Date | Nov.-01 | Nov.-02 | Nov.-03 | Nov.-03 | Nov.-27 | Nov.-28 | Nov.-28 | Nov.-29 |
SR locationi | S30E20 | N25E25 | S20W30 | N15W30 | W30S30 | N20E10 | N25E40 | S15W00 |
Flare class | – | – | M1.7/C2.8 | C3.2 | – | C6.7 | C5.6 | M3.4+M9.8 |
FR chirality | Right | Left | – | Left | Right | Left | Left | Right |
Filament relation | Yes | Yes | No | Yes (huge) | Yes | No | Yes | No |
CME PA in WL | 160–200 | 0–70 | 260–280 | Partial halo | 150–250 | Partial halo | 0–90 | Full halo |
CME GCS speed [km/s] | 650±30 | 630±30 | 350±20 | 1190±60 | 550±30 | 520±30 | 1020±50 | 640±30 |
CH area [×1010 km2] | 8.5 | 8.5 | 8.5 | 8.5 | 10.1 | 10.1 | 10.1 | 10.1 |
CH B-signed [G] | −5.2 | −5.2 | −5.2 | −5.2 | −3.5 | −3.5 | −3.5 | −3.5 |
CHIP (apex) [G] | 1.77 | 1.77 | 0.68 | 0.76 | 0.27+ | 0.46 | 0.70 | 0.81 |
3D DBM hit/miss | Miss | Clear miss | Likely miss | Likely hit | Likely miss | Likely hit | Clear miss | Clear hit |
3D DBM FR arrival [UT] | – | – | – | Nov.-05 23:00 | – | Dec.-02 00:44 | – | Dec.-02 00:44 |
3D DBM shock [km/s] | – | – | – | Nov.-05 13:00 | – | Dec.-01 14:44 | – | Dec.-01 14:44 |
Shock arrival [UT] | – | – | Nov.-05 09:15 | Nov.-05 12:30 | – | Dec.-01 00:22 | – | Dec.-01 09:38 |
FR arrival [UT] | – | – | – | – | – | Dec.-01 07:28 | – | Dec.-01 20:45 |
FR speed [km/s] | – | – | – | – | – | 460 | – | 430 |
FR chirality | – | – | – | – | – | – | – | Right |
Notes. The date is for the year 2023. Block 1: CME source region (SR) characteristics with i: to the nearest 5° at the launch time of CME (FR: flux rope; PA in WL: projected position angle of the CME as seen in white-light LASCO data). 3D speed and error for each CME as derived from GCS reconstructions (rounded; see details in Table A.1). Block 2: Derived CATCH parameters related to the CH and CHIP results (the CH area given is corrected for projection effects; B-signed refers to the signed mean magnetic field strength; +: the calculated value corresponds to instances when the source region is visible during CH CATCH time, yet part of the CME apex lies on the opposite side of the Sun due to the longitudinal separation between the SR and the CH). Block 3: Hit or miss likelihood of each CME derived from CME cone projections with GCS parameters and errors. 3D DBM results for the FR and shock (see Table A.1 for details of 3D DBM input parameters). Block 4: In situ measured FR and shock arrival times, and characteristics of the observed magnetic structure.
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