Solar Activity
Live solar imagery, recent flares, CMEs, active regions, and flare probability forecasts.
Solar Imagery

SUVI 094
Fe XVIII ~6.3 MK (hot flare plasma)

SUVI 131
Fe VIII/XXI ~0.4/10 MK

SUVI 171
Fe IX ~0.6 MK (quiet corona)

SUVI 195
Fe XII ~1.2 MK (active corona)

SUVI 284
Fe XV ~2.0 MK (warm corona)

SUVI 304
He II ~0.05 MK (chromosphere)

SOHO EIT 304
He II chromosphere (SOHO)

SOHO LASCO C2
Inner coronagraph (2-6 Rs)

SOHO LASCO C3
Outer coronagraph (3.7-30 Rs)
Flare Probabilities
Flare Probabilities
Recent Solar Flares
Recent Solar Flares
| Class | Peak Time | Source Location | Active Region |
|---|---|---|---|
| C4.1 | Mar 28, 2026, 11:35 AM UTC | N15E57 | 14404 |
| M1.3 | Mar 28, 2026, 4:18 AM UTC | S24E70 | 14405 |
| M3.9 | Mar 26, 2026, 6:23 AM UTC | N15E60 | 14403 |
| C2.9 | Mar 25, 2026, 12:12 AM UTC | S14W52 | 14400 |
| C7.2 | Mar 24, 2026, 5:54 PM UTC | N12E90 | N/A |
Coronal Mass Ejections
Mar 29, 2026, 11:12 AM UTC
- Source
- S35E55
- Speed
- 505 km/s
Very faint minor CME seen to the SE seen in SOHO LASCO C2, STEREO A COR2 and GOES CCOR-1. No clear source has been found for this very faint minor CME in EUV imagery, however there is a very minor dimming at ~(S35E55) seen in GOES SUVI 195 imagery, tentatively confirming the analysis based on the fit of the front of the CME in SOHO LASCO and STEREO A coronagraphs.
Mar 29, 2026, 5:12 AM UTC
- Source
- N/A
- Speed
- 515 km/s
Very faint and narrow blip to the SE seen in SOHO LASCO C2/C3 and in GOES CCOR-1 and STEREO A COR2. No clear source for it has been found in GOES SUVI imagery.
Mar 28, 2026, 11:48 PM UTC
- Source
- N/A
- Speed
- 511 km/s
Very faint jet to the NE seen best in SOHO LASCO C2 and also faintly seen in C3. It is not seen in GOES CCOR-1 and covered by the night time data gap in STEREO A COR2. Its source is possibly an eruption from AR 14403 (N30E28) starting ~2026-03-28T21:30Z, although this eruption seems to be deflecting N.
Mar 28, 2026, 11:45 PM UTC
- Source
- N/A
- Speed
- 455 km/s
Narrow CME first seen to the SE in GOES CCOR-1 starting around 2026-03-28T23:45Z. It is covered by real-time data gaps in SOHO LASCO C2/C3 and STEREO A COR2. This feature is very faint and is best seen in running difference imagery. There is not a good source candidate on the Earth-facing disk, so the source is possibly far-sided.
Mar 28, 2026, 8:24 PM UTC
- Source
- N/A
- Speed
- 358 km/s
Narrow CME first seen to the ESE in SOHO LASCO C2 starting at 2026-03-28T20:24Z. It is also seen to the ESE in SOHO LASCO C3 and GOES CCOR-1 but is covered by a real-time data gap in STEREO A COR2. This CME is very faint and is best seen in running difference imagery. There is no good source candidate on the Earth-facing disk, so that source is possibly far-sided.
Mar 28, 2026, 8:12 PM UTC
- Source
- N/A
- Speed
- 296 km/s
Narrow CME first seen to the SE in SOHO LASCO C2 starting at 2026-03-28T20:12Z. It is also seen to the SE in GOES CCOR-1 but is obscured by the pylon in SOHO LASCO C3. It is covered by a real-time data gap in STEREO A COR2. This CME is very faint and is best seen in running difference imagery. There is no good source candidate on the Earth-facing disk, so that source is possibly far-sided.
Mar 28, 2026, 5:09 PM UTC
- Source
- S25E56
- Active Region
- 14405
- Speed
- 300 km/s
Narrow CME first seen to the SE in STEREO A COR2 starting at 2026-03-28T17:09Z. It is also seen to the SE in GOES CCOR-1 but is covered by a real-time data gap in SOHO LASCO C2/C3. The source of this CME is most likely an eruption best seen in GOES SUVI 284 from AR 4405 (S25E56) starting at 2026-03-28T14:56Z with opening field lines. Likely due to its proximity to a coronal hole centered approximately around S15E35 at the CME start time, there is some deflection.
Mar 28, 2026, 12:23 PM UTC
- Source
- N15E55
- Active Region
- 14404
- Speed
- 926 km/s
CME visible to the NE in STEREO A COR2 and GOES CCOR-1. Not initially visible in SOHO LASCO C2/C3 imagery in real time due to a data gap. The potential source is a C4.1 flare starting at 2026-03-28T11:18Z from Active Region 14404 (approximately N15E55). The eruption can be best seen as brightening and opening field lines in GOES SUVI 195 imagery. Opening field lines are also visible in GOES SUVI 284 imagery. The eruption is visible beyond the NE limb in STEREO A EUV 195 imagery.
Mar 28, 2026, 7:48 AM UTC
- Source
- S30E55
- Speed
- 691 km/s
CME visible to the SE in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2. The CME is partially obscured by the pylon in SOHO LASCO C3. The source is an eruption with dimming starting around 2026-03-28T07:04Z as seen in GOES SUVI 195 imagery around S30E55, east of AR 4405.
Mar 28, 2026, 3:48 AM UTC
- Source
- S25E70
- Active Region
- 14405
- Speed
- 823 km/s
Wide CME visible to the SE in SOHO LASCO C2/C3 and STEREO A COR2. The CME is also visible in GOES CCOR-1 starting at 2026-03-28T06:45Z due to Earthshine. The source is a long duration M1.3 flare from AR 14405 (approximately S25E70) starting at 2026-03-28T02:16Z. Dimming and EUV wave are best seen in GOES SUVI 195. Moving field lines are also visible in GOES SUVI 171/195/284. The eruption can also be seen off the east limb in STEREO A EUV 195 imagery.
Mar 28, 2026, 1:26 AM UTC
- Source
- N15W55
- Speed
- 397 km/s
Narrow CME visible to the NW in SOHO LASCO C2/C3 and the NNE in STEREO A COR2. Not seen in GOES CCOR-1 due to Earthshine. The likely source is a partial filament eruption seen in GOES SUVI 304 starting at 2026-03-27T21:56Z around N15W55. There is possible deflection from the source location within the field of view.
Mar 27, 2026, 11:12 PM UTC
- Source
- S35E35
- Speed
- 417 km/s
Faint CME visible to the SE in SOHO LASCO C2/C3 and GOES CCOR-1. The CME is partially obscured by the pylon in SOHO LASCO C3. Not visible in STEREO A COR2 due to a data gap starting at 2026-03-27T16:53Z. The potential source is a filament eruption starting around 2026-03-27T20:36Z centered around S35E35 as seen in GOES SUVI 195/304.
Mar 27, 2026, 7:36 PM UTC
- Source
- N/A
- Speed
- 823 km/s
Faint CME visible to the SW in SOHO LASCO C2/C3 and GOES CCOR-1. There is a data gap in STEREO A COR2 for this event. The possible source of this CME is seen as moving/opening field lines along the W limb as seen in GOES SUVI 304 starting around 2026-03-27T18:56Z.
Mar 27, 2026, 8:24 AM UTC
- Source
- S22E80
- Speed
- 609 km/s
This CME is visible to the southeast in SOHO LASCO C2/C3 and GOES CCOR-1 imagery. This event is not observed in STEREO A COR2 imagery. The source is likely related to an eruption on the southeast limb (centered near S22E80) starting around 2026-03-27T07:00Z as seen in GOES SUVI 131/195/304 imagery.
Mar 27, 2026, 1:26 AM UTC
- Source
- N/A
- Speed
- 719 km/s
This CME is visible to the southeast in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2 imagery. The source is an eruption observed near the southeast limb starting around 2026-03-27T00:40Z as seen in GOES SUVI 131/171/195/294/304 imagery. An opening of field lines can be seen over the southeast limb at this time in GOES SUVI 171/195/284 imagery and post-eruptive arcades are visible on the southeast limb starting around 2026-03-27T01:00Z in GOES SUVI 131/171/195/304 imagery.
Mar 26, 2026, 11:12 PM UTC
- Source
- N/A
- Speed
- 320 km/s
This CME is visible to the northeast in SOHO LASCO C2/C3 and GOES CCOR-1 imagery. This event is not seen in STEREO A COR2 imagery due to a data gap from 2026-03-26T16:08Z to 2026-03-27T03:23Z. The source is likely far-sided and related to an opening of field lines observed over the northeast limb in GOES SUVI 171/195/284 imagery starting around 2026-03-26T22:30Z.
Mar 26, 2026, 9:24 PM UTC
- Source
- N20E90
- Speed
- 355 km/s
Jet CME seen to the northeast in SOHO C2 and SOHO C3, likely associated with a minor eruption with moving field lines seen near or just beyond the northeast limb in GOES SUVI 284 around 2026-03-26T21:00Z
Mar 26, 2026, 7:15 PM UTC
- Source
- N/A
- Speed
- 732 km/s
Bright CME seen to the southeast starting near 2026-03-26T19:15Z in GOES CCOR-1 and late in SOHO C2/C3 due to a data gap; the source is likely far-sided as determined from the lack of moving or opening field lines on the Earth-facing disk as seen in GOES coronagraph imagery between 17:00 and 19:00Z. The CME is comprised of a brighter central portion and an asymmetric shock portion which is fainter and overtakes the brighter portion in the imagery.
Mar 26, 2026, 6:48 AM UTC
- Source
- N15E60
- Active Region
- 14403
- Speed
- 440 km/s
Faint, wide CME observed to the NE in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2. The source is associated with an M3.9 flare from AR 14403 which peaked at 2026-03-26T06:23Z, as observed in GOES SUVI 131. Additional source observations include wide field line movement and an EUV wave in GOES SUVI 171/195/284/304 starting around 2026-03-26T06:12Z.
Mar 26, 2026, 12:48 AM UTC
- Source
- N/A
- Speed
- 333 km/s
Faint, thin CME observed to the SW in SOHO LASCO C2/C3 and GOES CCOR-1, not observed in STEREO A COR2 due to a data gap. The CME is barely a half width of 10 degrees, perhaps slightly smaller. The source is observed as field line movement over the SW limb beginning at 2026-03-26T23:40Z in GOES SUVI 171/195/284, likely originating from former AR 14392 which is around W100-W105 at this time, although direct observations of the source are not possible without STEREO A EUVI to confirm longitude.
Mar 25, 2026, 3:48 PM UTC
- Source
- N/A
- Speed
- 295 km/s
Wide, faint, slow to evolve CME observed to the N/NW in SOHO LASCO C2/C3 and GOES CCOR-1, and less wide to the NE in STEREO A COR2. The CME begins very slow and faint, speeding up somewhat as it evolves. The source for this CME is not too clear, but may be associated with a very slow dimming region of the disk centered around N15W05 at 2026-03-25T15:00Z as part of a nearby coronal hole, slowly evolving and drifting with the coronal hole for almost a full 24 hours. This does match the slow, wide nature of this CME front, corroborating it as the potential source along with the swpc_cat triangulation to this general area of the disk.
Mar 25, 2026, 1:48 PM UTC
- Source
- N/A
- Speed
- 494 km/s
Faint CME to the NE in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2. The source of this CME appears to be moving/opening field lines visible beyond the NE limb in GOES SUVI 284 starting as early as 09:00Z, responsible for several other overlapping CMEs around this time.
Mar 25, 2026, 12:48 PM UTC
- Source
- N/A
- Speed
- 484 km/s
Faint CME to the NE in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2. The source of this CME appears to be moving/opening field lines visible beyond the NE limb in GOES SUVI 284 starting as early as 09:00Z, responsible for several other overlapping CMEs around this time.
Mar 25, 2026, 12:36 PM UTC
- Source
- N/A
- Speed
- 322 km/s
Bright and slow CME visible to the SE in GOES CCOR-1, and for a frame in SOHO LASCO C2 before a data gap starting at 2026-03-25T12:36Z. It is also visible due S in STEREO A COR2 imagery. The source is a filament eruption visible along/just beyond the SE limb in GOES SUVI 304 with associated moving/opening field lines in GOES SUVI 284 starting around 2026-03-25T07:00Z.
Mar 25, 2026, 11:12 AM UTC
- Source
- N/A
- Speed
- 394 km/s
Faint and narrow CME visible to the NE in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2 imagery. This CME appears to overlap the CME first seen in SOHO LASCO C2 at 2026-03-25T09:36Z. The source of this CME appears to be moving/opening field lines visible beyond the NE limb in GOES SUVI 284 starting around 09:00Z, overlaps source movement from CME: 2026-03-25T09:36Z.
Mar 25, 2026, 9:36 AM UTC
- Source
- N/A
- Speed
- 429 km/s
Faint and narrow CME visible to the NE in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2 imagery. The source appears to be moving/opening field lines just beyond the NE limb in GOES SUVI 284 starting around 2026-03-25T07:16Z.
Mar 25, 2026, 6:48 AM UTC
- Source
- N/A
- Speed
- 267 km/s
Faint CME visible to the NE in SOHO LASCO C2/C3, STEREO A, and possibly in GOES CCOR-1 following the Earth-shine event. This CME follows in the same path of the CMEs: 2026-03-24T20:15Z (CCOR-1) and 2026-03-25T03:36Z (C2). No clear source but appears to be within the outflow of the aforementioned CMEs.
Mar 25, 2026, 3:36 AM UTC
- Source
- N/A
- Speed
- 400 km/s
Faint CME visible to the NE in SOHO LASCO C2/C3 and STEREO A COR2 imagery. Blocked in CCOR-1 by Earth-shine. No clear source but appears to be within the outflow of the CME: 2026-03-24T20:15Z (CCOR-1).
Mar 25, 2026, 12:45 AM UTC
- Source
- S14W52
- Active Region
- 14400
- Speed
- 1208 km/s
CME visible to the southwest in GOES CCOR-1 and in limited available SOHO LASCO C3 imagery in real-time during a data downlink period. Not visible in STEREO A COR2 imagery due to a data gap starting at 2026-03-24T13:53Z. The source is a C2.9 flare and associated eruption from AR 14400 (approximately S14W52) starting at 2026-03-24T23:52Z as seen in GOES SUVI 195/284 with rapidly opening field lines and possible EUV wave.
Mar 24, 2026, 8:15 PM UTC
- Source
- N/A
- Speed
- 427 km/s
CME seen to the NE in GOES CCOR-1 and SOHO LASCO C2/C3. The CME is not visible in STEREO A COR2 in real-time due to a data gap starting at 2026-03-24T13:53Z. The source is a C7.2 flare starting at 2026-03-24T17:18Z as seen in GOES SUVI 131 imagery. Opening field lines and post-eruptive arcades are also visible near the NE limb in GOES SUVI 171/195/284/304 imagery.
Mar 24, 2026, 12:12 PM UTC
- Source
- S40W35
- Speed
- 398 km/s
Narrow, faint CME first seen to the SW by SOHO LASCO C2 beginning at 2026-03-24T12:12Z, as well as by SOHO LASCO C3, STEREO A COR2 and GOES CCOR-1 in later frames. The source of this event is a very small eruption seen beginning at approx. 2026-03-24T11:12Z located at approx. S40W35 as seen in GOES SUVI 195.
Mar 24, 2026, 3:53 AM UTC
- Source
- N/A
- Speed
- 317 km/s
CME first seen to the West by STEREO A COR2 beginning at 2026-03-24T03:53 following the end of a data gap which began at 2026-03-23T20:23Z. This CME is not visible in SOHO LASCO C2/C3 or GOES CCOR-1, as it is likely completely far sided with respect to the Sun-Earth line. This event is also quite faint in STERO A COR2 and is therefore only visible for a few frames. Due to the data gap in STEREO A and the far sided nature of the CME, no clear source is seen for this event.
Mar 23, 2026, 4:15 PM UTC
- Source
- N/A
- Speed
- 474 km/s
Faint CME observed to the SW only in GOES CCOR-1. SOHO LASCO is in a downlink gap, and the CME may be too faint or directed towards STEREO A COR2. No distinct source for this CME is observed, but based on its direction and recent eruptions it may be an outflow from AR 14392 following significant CMEs 2026-03-22T23:24Z and 2026-03-23T02:36Z.
Mar 23, 2026, 11:36 AM UTC
- Source
- N/A
- Speed
- 387 km/s
Narrow, faint, jet-like CME visible to the NW in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2 imagery. There is no clear source for this CME.
Mar 23, 2026, 2:36 AM UTC
- Source
- S17W65
- Active Region
- 14392
- Speed
- 551 km/s
CME observed to the SW in SOHO LASCO C2/C3 and GOES CCOR-1 and as a partial halo to the S/SW in STEREO A COR2. This CME immediately follows the larger CME 2026-03-22T23:24Z, and it is very likely outflow or a streamer blowout following that eruption from AR 14392 (S17W65), corroborated via coronagraph triangulation in the swpc_cat tool. The field line loops over AR 14392, which initially began to erupt around 2026-03-22T23:34Z in GOES SUVI 171/195/284, seen as a second movement of field lines starting around 2026-03-23T01:31Z. That first eruption is associated with a C1.5 flare as observed in GOES SUVI 131, which is not linked to this second CME.
Active Sunspot Regions
Active Sunspot Regions
| Region | Location | Spot Class | Mag Class | Area | C % | M % | X % |
|---|---|---|---|---|---|---|---|
| 4408 | N9 E50 | Hsx | A | 50 | 0% | 0% | 0% |
| 4407 | N18 E31 | Bxo | B | 10 | 0% | 0% | 0% |
| 4406 | N9 E24 | Hsx | A | 50 | 0% | 0% | 0% |
| 4405 | S27 E30 | Eao | BG | 180 | 0% | 0% | 0% |
| 4404 | N14 E19 | Hsx | A | 30 | 0% | 0% | 0% |
| 4403 | N16 E0 | Hsx | A | 70 | 0% | 0% | 0% |
| 4402 | N18 W32 | Cso | B | 30 | 0% | 0% | 0% |
| 4401 | N25 W41 | Eai | B | 150 | 0% | 0% | 0% |
| 4399 | S17 W40 | Hsx | A | 50 | 0% | 0% | 0% |
| 4398 | S16 W97 | N/A | N/A | 0% | 0% | 0% | |
| 4397 | N15 W95 | N/A | N/A | 0% | 0% | 0% | |
| 4404 | N14 E33 | Hsx | A | 30 | 10% | 1% | 1% |
| 4403 | N16 E14 | Hsx | A | 70 | 10% | 1% | 1% |
| 4402 | N18 W18 | Cso | B | 30 | 15% | 1% | 1% |
| 4401 | N25 W27 | Eai | B | 150 | 60% | 15% | 1% |
| 4399 | S17 W26 | Hsx | A | 50 | 10% | 1% | 1% |
| 4398 | S16 W83 | N/A | N/A | 0% | 0% | 0% | |
| 4397 | N15 W81 | N/A | N/A | 0% | 0% | 0% | |
| 4405 | S27 E44 | Eao | BG | 180 | 55% | 15% | 1% |
| 4406 | N9 E38 | Hsx | A | 50 | 10% | 1% | 1% |
| 4407 | N18 E45 | Bxo | B | 10 | 10% | 1% | 1% |
| 4408 | N9 E64 | Hsx | A | 50 | 10% | 1% | 1% |
| 4397 | N15 W67 | N/A | N/A | 0% | 0% | 0% | |
| 4398 | S16 W69 | N/A | N/A | 1% | 0% | 0% | |
| 4399 | S17 W13 | Hsx | A | 80 | 10% | 1% | 1% |
| 4400 | S12 W106 | Dai | B | 50 | 0% | 0% | 0% |
| 4401 | N25 W15 | Ekc | BG | 350 | 85% | 35% | 5% |
| 4402 | N19 W4 | Hsx | A | 50 | 10% | 1% | 1% |
| 4403 | N16 E27 | Hsx | A | 120 | 10% | 1% | 1% |
| 4404 | N14 E46 | Hsx | A | 50 | 10% | 1% | 1% |
| 4405 | S26 E55 | Ehi | BG | 330 | 65% | 20% | 5% |
| 4406 | N9 E52 | Hsx | A | 80 | 10% | 1% | 1% |
| 4407 | N17 E56 | Hsx | A | 40 | 10% | 1% | 1% |
| 4397 | N15 W53 | N/A | N/A | 1% | 0% | 0% | |
| 4398 | S17 W55 | Axx | A | 10 | 5% | 1% | 1% |
| 4399 | S17 E2 | Cso | B | 120 | 15% | 1% | 1% |
| 4400 | S12 W92 | Dai | B | 50 | 50% | 10% | 1% |
| 4401 | N25 W2 | Ekc | BG | 370 | 85% | 40% | 5% |
| 4402 | N18 E8 | Cao | B | 70 | 20% | 5% | 1% |
| 4403 | N16 E40 | Hsx | A | 120 | 10% | 1% | 1% |
| 4405 | S25 E66 | Eho | B | 270 | 55% | 10% | 1% |
| 4404 | N15 E63 | Cso | B | 50 | 15% | 1% | 1% |
| 4406 | N9 E62 | Hsx | A | 70 | 10% | 1% | 1% |
| 4405 | S24 E82 | N/A | N/A | 0% | 0% | 0% | |
| 4403 | N15 E54 | Hsx | A | 110 | 50% | 25% | 1% |
| 4402 | N16 E18 | Cso | B | 120 | 15% | 5% | 1% |
| 4401 | N25 E11 | Ekc | B | 275 | 80% | 35% | 5% |
| 4400 | S12 W77 | Dai | B | 50 | 45% | 5% | 1% |
| 4399 | S17 E15 | Hax | A | 170 | 20% | 5% | 1% |
| 4398 | S17 W40 | Dro | B | 25 | 15% | 1% | 1% |
| 4397 | N15 W39 | Bxo | B | 10 | 1% | 1% | 1% |
| 4396 | N20 W99 | N/A | N/A | 0% | 0% | 0% | |
| 4403 | N16 E67 | Hsx | A | 110 | 55% | 10% | 1% |
| 4402 | N17 E32 | Dso | B | 140 | 20% | 5% | 1% |
| 4401 | N25 E24 | Eai | B | 230 | 60% | 15% | 1% |
| 4400 | S12 W65 | Dao | BG | 50 | 40% | 5% | 1% |
| 4399 | S17 E28 | Hax | A | 170 | 15% | 5% | 1% |
| 4398 | S17 W27 | Dro | B | 30 | 15% | 5% | 1% |
| 4397 | N15 W27 | Axx | A | 5 | 5% | 1% | 1% |
| 4396 | N20 W85 | N/A | N/A | 1% | 1% | 1% | |
| 4395 | S6 W102 | N/A | N/A | 0% | 0% | 0% | |
| 4392 | S17 W104 | Cao | B | 90 | 0% | 0% | 0% |
| 4403 | N16 E82 | N/A | N/A | 0% | 0% | 0% | |
| 4402 | N17 E45 | Dso | B | 150 | 35% | 5% | 1% |
| 4401 | N25 E38 | Eai | BG | 210 | 55% | 15% | 1% |
| 4400 | S14 W52 | Dao | B | 80 | 30% | 5% | 1% |
| 4399 | S18 E42 | Cao | B | 170 | 45% | 5% | 1% |
| 4398 | S17 W12 | Dao | B | 40 | 30% | 5% | 1% |
| 4397 | N15 W12 | Bxo | B | 10 | 5% | 1% | 1% |
| 4396 | N20 W71 | N/A | N/A | 1% | 1% | 1% | |
| 4395 | S6 W87 | N/A | N/A | 1% | 1% | 1% | |
| 4394 | S12 W94 | N/A | N/A | 0% | 0% | 0% | |
| 4392 | S17 W90 | Cao | B | 90 | 20% | 5% | 1% |
| 4402 | N17 E56 | Dao | B | 150 | 30% | 5% | 1% |
| 4401 | N24 E52 | Dao | B | 170 | 30% | 5% | 1% |
| 4400 | S12 W40 | Dao | BD | 70 | 30% | 5% | 1% |
| 4399 | S18 E54 | Cao | B | 170 | 20% | 5% | 1% |
| 4398 | S16 W1 | Csi | B | 30 | 40% | 10% | 1% |
| 4397 | N16 W1 | Cro | B | 20 | 15% | 1% | 1% |
| 4396 | N20 W57 | N/A | N/A | 0% | 0% | 0% | |
| 4395 | S6 W73 | N/A | N/A | 0% | 0% | 0% | |
| 4394 | S12 W80 | N/A | N/A | 0% | 0% | 0% | |
| 4392 | S17 W77 | Cao | B | 120 | 20% | 5% | 1% |
| 4400 | S12 W25 | Dai | BGD | 40 | 60% | 15% | 1% |
| 4401 | N24 E63 | Dao | B | 100 | 30% | 5% | 1% |
| 4399 | S17 E68 | Hax | A | 170 | 10% | 1% | 1% |
| 4398 | S15 E13 | Cro | B | 20 | 15% | 1% | 1% |
| 4397 | N16 E14 | Cro | B | 20 | 15% | 1% | 1% |
| 4396 | N20 W43 | N/A | N/A | 0% | 0% | 0% | |
| 4395 | S6 W58 | N/A | N/A | 0% | 0% | 0% | |
| 4394 | S12 W66 | N/A | N/A | 0% | 0% | 0% | |
| 4393 | N14 W101 | N/A | N/A | 0% | 0% | 0% | |
| 4392 | S18 W65 | Cso | B | 120 | 20% | 5% | 1% |
| 4402 | N14 E68 | Hax | A | 80 | 10% | 1% | 1% |
| 4399 | S17 E82 | Hsx | A | 120 | 10% | 1% | 1% |
| 4398 | S14 E26 | Cro | B | 10 | 15% | 1% | 1% |
| 4397 | N16 E27 | Cro | B | 20 | 15% | 1% | 1% |
| 4396 | N20 W29 | N/A | N/A | 0% | 0% | 0% | |
| 4395 | S6 W43 | N/A | N/A | 0% | 0% | 0% | |
| 4394 | S12 W52 | N/A | N/A | 0% | 0% | 0% | |
| 4393 | N14 W87 | N/A | N/A | 0% | 0% | 0% | |
| 4392 | S17 W52 | Cso | B | 110 | 25% | 5% | 1% |
| 4391 | N7 W104 | N/A | N/A | 0% | 0% | 0% | |
| 4389 | N12 W99 | N/A | N/A | 0% | 0% | 0% | |
| 4397 | N18 E42 | Cao | B | 30 | 20% | 5% | 1% |
| 4396 | N20 W15 | N/A | N/A | 1% | 1% | 1% | |
| 4395 | S6 W28 | N/A | N/A | 1% | 1% | 1% | |
| 4394 | S12 W38 | N/A | N/A | 1% | 1% | 1% | |
| 4393 | N14 W73 | N/A | N/A | 1% | 1% | 1% | |
| 4392 | S16 W40 | Cso | B | 130 | 25% | 5% | 1% |
| 4391 | N7 W89 | N/A | N/A | 1% | 1% | 1% | |
| 4389 | N12 W85 | N/A | N/A | 1% | 1% | 1% | |
| 4387 | N8 W103 | N/A | N/A | 0% | 0% | 0% | |
| 4397 | N17 E55 | Cao | B | 30 | 20% | 5% | 1% |
| 4396 | N20 W1 | N/A | N/A | 1% | 1% | 1% | |
| 4395 | S6 W15 | N/A | N/A | 1% | 1% | 1% | |
| 4394 | S12 W24 | N/A | N/A | 1% | 1% | 1% | |
| 4393 | N14 W59 | N/A | N/A | 1% | 1% | 1% | |
| 4392 | S17 W26 | Csi | BG | 170 | 55% | 10% | 1% |
| 4391 | N7 W75 | N/A | N/A | 1% | 1% | 1% | |
| 4390 | N26 W96 | N/A | N/A | 0% | 0% | 0% | |
| 4389 | N12 W71 | N/A | N/A | 1% | 1% | 1% | |
| 4387 | N8 W89 | N/A | N/A | 1% | 1% | 1% | |
| 4397 | N17 E69 | Cro | B | 30 | 15% | 1% | 1% |
| 4392 | S17 W12 | Csi | BG | 170 | 55% | 20% | 5% |
| 4391 | N7 W61 | Axx | A | 10 | 5% | 1% | 1% |
| 4390 | N26 W82 | N/A | N/A | 1% | 1% | 1% | |
| 4389 | N12 W57 | N/A | N/A | 1% | 1% | 1% | |
| 4387 | N8 W75 | N/A | N/A | 1% | 1% | 1% | |
| 4396 | N20 E14 | N/A | N/A | 1% | 1% | 1% | |
| 4395 | S6 W1 | Bxo | B | 10 | 10% | 1% | 1% |
| 4394 | S12 W10 | N/A | N/A | 1% | 1% | 1% | |
| 4393 | N14 W45 | Cso | B | 20 | 15% | 1% | 1% |
| 4396 | N20 E27 | N/A | N/A | 5% | 1% | 1% | |
| 4395 | S6 E13 | Cro | B | 30 | 25% | 5% | 1% |
| 4394 | S12 E4 | N/A | N/A | 1% | 1% | 1% | |
| 4393 | N14 W31 | Cro | B | 30 | 25% | 5% | 1% |
| 4392 | S16 E1 | Csi | BG | 200 | 55% | 30% | 5% |
| 4391 | N7 W47 | Axx | A | 10 | 5% | 1% | 1% |
| 4390 | N26 W68 | N/A | N/A | 1% | 1% | 1% | |
| 4389 | N12 W43 | N/A | N/A | 1% | 1% | 1% | |
| 4387 | N8 W61 | N/A | N/A | 1% | 1% | 1% | |
| 4396 | N20 E38 | Axx | A | 10 | 5% | 1% | 1% |
| 4395 | S5 E27 | Dro | B | 30 | 15% | 5% | 1% |
| 4394 | S12 E17 | N/A | N/A | 1% | 0% | 0% | |
| 4393 | N14 W17 | Cro | B | 30 | 15% | 5% | 1% |
| 4392 | S16 E15 | Csi | BG | 160 | 55% | 20% | 5% |
| 4391 | N7 W34 | N/A | N/A | 5% | 1% | 1% | |
| 4390 | N26 W54 | N/A | N/A | 0% | 0% | 0% | |
| 4389 | N12 W29 | N/A | N/A | 0% | 0% | 0% | |
| 4387 | N8 W47 | N/A | N/A | 0% | 0% | 0% | |
| 4396 | N20 E55 | Bxo | B | 10 | 10% | 1% | 1% |
| 4395 | S5 E41 | Cro | B | 40 | 20% | 5% | 1% |
| 4394 | S12 E31 | Axx | A | 10 | 10% | 1% | 1% |
| 4393 | N14 W2 | Cro | B | 30 | 15% | 1% | 1% |
| 4392 | S16 E28 | Cso | B | 170 | 25% | 5% | 1% |
| 4391 | N7 W19 | Bxo | B | 10 | 10% | 1% | 1% |
| 4390 | N26 W40 | N/A | N/A | 0% | 0% | 0% | |
| 4389 | N10 W16 | N/A | N/A | 0% | 0% | 0% | |
| 4388 | S14 W99 | N/A | N/A | 0% | 0% | 0% | |
| 4387 | N8 W33 | N/A | N/A | 0% | 0% | 0% | |
| 4384 | N10 W108 | Dai | B | 230 | 0% | 0% | 0% |
| 4394 | S12 E44 | Axx | A | 10 | 5% | 1% | 0% |
| 4395 | S4 E53 | Bxo | B | 10 | 10% | 1% | 0% |
| 4393 | N13 E10 | Cro | B | 30 | 15% | 1% | 0% |
| 4392 | S15 E41 | Cso | B | 90 | 15% | 1% | 0% |
| 4391 | N6 W6 | Bxo | B | 10 | 10% | 1% | 0% |
| 4390 | N26 W26 | N/A | N/A | 0% | 0% | 0% | |
| 4389 | N10 W2 | N/A | N/A | 0% | 0% | 0% | |
| 4388 | S14 W85 | N/A | N/A | 0% | 0% | 0% | |
| 4387 | N8 W19 | N/A | N/A | 0% | 0% | 0% | |
| 4384 | N10 W94 | Dai | B | 230 | 55% | 10% | 0% |
| 4393 | N14 E23 | Cao | B | 30 | 20% | 5% | 1% |
| 4392 | S15 E54 | Cso | B | 120 | 15% | 5% | 1% |
| 4391 | N6 E7 | Cro | B | 30 | 20% | 5% | 1% |
| 4390 | N26 W12 | Bxo | B | 10 | 10% | 1% | 1% |
| 4389 | N12 E12 | Axx | A | 10 | 10% | 1% | 1% |
| 4388 | S14 W71 | Bxo | B | 10 | 10% | 1% | 1% |
| 4387 | N8 W5 | N/A | N/A | 1% | 1% | 1% | |
| 4385 | S9 W92 | N/A | N/A | 0% | 0% | 0% | |
| 4384 | N8 W81 | Dai | B | 230 | 55% | 15% | 1% |
| 4381 | N9 W110 | Hsx | A | 80 | 0% | 0% | 0% |
| 4393 | N13 E37 | Cso | B | 30 | 25% | 5% | 1% |
| 4392 | S16 E65 | Hsx | A | 80 | 10% | 1% | 1% |
| 4391 | N5 E21 | Dro | B | 30 | 20% | 1% | 1% |
| 4390 | N26 E1 | Bxo | B | 10 | 10% | 1% | 1% |
| 4389 | N12 E26 | Hrx | A | 10 | 10% | 1% | 1% |
| 4388 | S14 W60 | Bxo | B | 10 | 10% | 1% | 1% |
| 4387 | N8 E9 | Axx | A | 10 | 5% | 1% | 1% |
| 4385 | S9 W78 | N/A | N/A | 0% | 0% | 0% | |
| 4384 | N8 W68 | Dao | B | 210 | 25% | 5% | 1% |
| 4381 | N9 W96 | Hsx | A | 80 | 15% | 1% | 1% |
| 4391 | N6 E34 | Cro | B | 20 | 15% | 5% | 1% |
| 4392 | S15 E79 | Hsx | A | 80 | 10% | 1% | 1% |
| 4393 | N14 E49 | Cro | B | 40 | 25% | 5% | 1% |
| 4390 | N26 E15 | Dro | B | 20 | 15% | 5% | 1% |
| 4389 | N12 E39 | Hrx | A | 10 | 10% | 1% | 1% |
| 4388 | S15 W46 | Dri | B | 30 | 35% | 5% | 1% |
| 4387 | N8 E23 | Axx | A | 5 | 10% | 1% | 1% |
| 4385 | S9 W64 | N/A | N/A | 0% | 0% | 0% | |
| 4384 | N8 W57 | Cao | B | 200 | 20% | 5% | 1% |
| 4381 | N9 W82 | Hsx | A | 80 | 15% | 1% | 1% |
| 4380 | S21 W101 | N/A | N/A | 0% | 0% | 0% | |
| 4389 | N13 E60 | Ero | B | 60 | 60% | 10% | 1% |
| 4385 | S9 W50 | N/A | N/A | 0% | 0% | 0% | |
| 4384 | N9 W44 | Hsx | A | 190 | 20% | 5% | 1% |
| 4381 | N9 W68 | Cso | B | 110 | 55% | 10% | 1% |
| 4380 | S21 W87 | N/A | N/A | 0% | 0% | 0% | |
| 4379 | S19 W99 | N/A | N/A | 0% | 0% | 0% | |
| 4378 | N17 W99 | Hsx | A | 120 | 0% | 0% | 0% |
| 4388 | S15 W33 | Cri | B | 30 | 40% | 5% | 1% |
| 4387 | N9 E40 | Cro | B | 30 | 50% | 10% | 1% |
| 4388 | S15 W18 | Cri | B | 20 | 10% | 1% | 1% |
| 4387 | N9 E53 | Dro | B | 30 | 40% | 10% | 1% |
| 4386 | N17 W99 | N/A | N/A | 0% | 0% | 0% | |
| 4385 | S9 W37 | N/A | N/A | 10% | 1% | 1% | |
| 4384 | N9 W27 | Cso | B | 210 | 30% | 5% | 1% |
| 4381 | N9 W50 | Eso | B | 120 | 60% | 15% | 1% |
| 4380 | S21 W73 | N/A | N/A | 0% | 0% | 0% | |
| 4379 | S19 W85 | N/A | N/A | 0% | 0% | 0% | |
| 4378 | N17 W85 | Hsx | A | 120 | 10% | 1% | 1% |
| 4387 | N9 E65 | Dao | B | 50 | 20% | 1% | 1% |
| 4386 | N17 W99 | N/A | N/A | 0% | 0% | 0% | |
| 4385 | S9 W25 | Axx | A | 10 | 5% | 1% | 1% |
| 4384 | N10 W14 | Dao | B | 240 | 40% | 5% | 1% |
| 4381 | N9 W39 | Eai | B | 200 | 60% | 15% | 1% |
| 4380 | S21 W59 | N/A | N/A | 0% | 0% | 0% | |
| 4379 | S19 W71 | N/A | N/A | 0% | 0% | 0% | |
| 4378 | N15 W73 | Cso | B | 170 | 20% | 1% | 1% |
| 4386 | N17 W90 | Axx | A | 40 | 15% | 1% | 1% |
| 4385 | S9 W12 | Axx | A | 10 | 5% | 1% | 1% |
| 4384 | N9 W1 | Eho | B | 270 | 50% | 10% | 1% |
| 4383 | N17 W92 | N/A | N/A | 0% | 0% | 0% | |
| 4381 | N8 W26 | Eai | B | 190 | 60% | 15% | 1% |
| 4380 | S21 W45 | N/A | N/A | 0% | 0% | 0% | |
| 4379 | S19 W57 | N/A | N/A | 0% | 0% | 0% | |
| 4378 | N16 W59 | Cso | B | 240 | 25% | 1% | 0% |
| 4386 | N15 W76 | Cao | B | 60 | 25% | 1% | 1% |
| 4385 | S9 E2 | Cro | B | 10 | 15% | 1% | 1% |
| 4384 | N10 E14 | Dho | B | 260 | 50% | 5% | 1% |
| 4383 | N17 W78 | N/A | N/A | 0% | 0% | 0% | |
| 4381 | N8 W11 | Eai | B | 200 | 60% | 10% | 1% |
| 4380 | S21 W31 | N/A | N/A | 0% | 0% | 0% | |
| 4379 | S19 W43 | N/A | N/A | 0% | 0% | 1% | |
| 4378 | N16 W44 | Cso | B | 240 | 25% | 1% | 1% |
| 4386 | N16 W63 | Bxo | B | 10 | 10% | 1% | 1% |
| 4385 | S8 E17 | Bxo | B | 10 | 10% | 1% | 1% |
| 4384 | N9 E26 | Eho | B | 260 | 50% | 10% | 1% |
| 4383 | N17 W64 | N/A | N/A | 0% | 0% | 0% | |
| 4382 | N22 W104 | N/A | N/A | 0% | 0% | 0% | |
| 4381 | N8 E2 | Dai | B | 170 | 50% | 10% | 1% |
| 4380 | S21 W17 | N/A | N/A | 0% | 0% | 0% | |
| 4379 | S19 W29 | N/A | N/A | 0% | 0% | 0% | |
| 4378 | N16 W29 | Cso | B | 230 | 15% | 1% | 1% |
| 4384 | N9 E40 | Eho | B | 290 | 55% | 10% | 1% |
| 4383 | N15 W55 | N/A | N/A | 0% | 0% | 0% | |
| 4382 | N22 W90 | N/A | N/A | 0% | 0% | 0% | |
| 4381 | N8 E16 | Cao | B | 170 | 35% | 5% | 1% |
| 4380 | S21 W3 | N/A | N/A | 0% | 0% | 0% | |
| 4379 | S19 W15 | N/A | N/A | 0% | 0% | 0% | |
| 4378 | N16 W15 | Cso | B | 230 | 25% | 5% | 1% |
| 4385 | S8 E31 | Bxo | B | 10 | 10% | 1% | 1% |
| 4384 | N10 E53 | Eho | B | 300 | 60% | 10% | 1% |
| 4383 | N15 W41 | Axx | A | 10 | 10% | 1% | 1% |
| 4382 | N22 W76 | N/A | N/A | 0% | 0% | 0% | |
| 4381 | N8 E30 | Eao | B | 220 | 40% | 10% | 1% |
| 4380 | S21 E11 | N/A | N/A | 10% | 1% | 1% | |
| 4379 | S19 W1 | N/A | N/A | 10% | 1% | 1% | |
| 4378 | N15 W2 | Cho | B | 250 | 30% | 5% | 1% |
| 4384 | N10 E67 | Ehi | B | 250 | 65% | 20% | 1% |
| 4383 | N15 W23 | Bxo | B | 10 | 10% | 1% | 1% |
| 4382 | N22 W62 | N/A | N/A | 0% | 0% | 0% | |
| 4381 | N8 E42 | Eao | B | 200 | 60% | 15% | 1% |
| 4380 | S21 E25 | Bxo | B | 30 | 15% | 1% | 1% |
| 4379 | S19 E14 | N/A | N/A | 0% | 0% | 0% | |
| 4378 | N15 E13 | Cho | B | 250 | 30% | 5% | 1% |
| 4384 | N10 E75 | Hsx | A | 220 | 55% | 10% | 1% |
| 4382 | N22 W48 | Bxo | B | 20 | 10% | 1% | 1% |
| 4381 | N8 E55 | Eao | B | 200 | 55% | 10% | 1% |
| 4380 | S21 E35 | Cao | B | 80 | 35% | 5% | 1% |
| 4379 | S19 E28 | N/A | N/A | 0% | 0% | 0% | |
| 4378 | N16 E21 | Hhx | A | 270 | 15% | 1% | 1% |
| 4383 | N15 W10 | Bxo | B | 20 | 10% | 1% | 1% |