SettingsLast update:
| Time UTC | DSCOVR | ACE | ||||
|---|---|---|---|---|---|---|
| Solar Wind | GSM | Solar Wind | GSM | |||
| Proton Density | Bulk Speed | Bz | Proton Density | Bulk Speed | Bz | |
| 19:55 | - | - | - | - | - | - |
| 19:54 | - | - | - | - | - | - |
| 19:53 | - | - | - | - | - | - |
| 19:52 | 3.26 | 410.7 | -2.27 | - | - | - |
| 19:51 | 3.73 | 413.0 | -2.52 | - | - | - |
| 19:50 | 4.82 | 416.3 | -2.47 | - | - | - |
| 19:49 | 4.84 | 391.5 | -1.95 | - | - | - |
| 19:48 | 6.66 | 409.8 | -1.72 | - | - | - |
| 19:47 | 7.26 | 424.9 | -2.58 | 7.3 | 424.9 | -2.6 |
| 19:46 | 6.39 | 427.1 | -1.96 | 6.4 | 427.1 | -2.0 |
| 19:45 | 5.46 | 413.2 | -1.80 | 5.5 | 413.2 | -1.8 |
| 19:44 | 5.43 | 402.1 | - | 5.4 | 402.1 | - |
| 19:43 | 6.42 | 414.5 | -1.72 | 6.3 | 413.9 | -1.7 |
| 19:42 | 6.38 | 407.2 | -1.03 | 6.1 | 405.9 | -1.0 |
| 19:41 | 5.55 | 393.0 | -0.74 | 5.5 | 393.0 | -0.7 |
| 19:40 | 7.95 | 383.6 | -3.42 | 8.7 | 384.5 | -3.4 |
| 19:39 | 6.83 | 391.4 | -5.92 | 6.8 | 391.4 | -5.9 |
| 19:38 | 11.30 | 386.8 | -6.34 | 11.3 | 386.8 | -6.3 |
| 19:37 | 9.59 | 394.6 | -7.12 | 9.6 | 394.6 | -7.1 |
| 19:36 | 6.88 | 387.9 | -7.37 | 6.9 | 387.9 | -7.4 |
| 19:35 | 5.31 | 377.6 | -6.35 | 5.3 | 377.6 | -6.3 |
| 19:34 | 5.08 | 375.9 | - | 5.1 | 375.9 | - |
| 19:33 | 7.74 | 394.9 | - | 7.7 | 394.9 | - |
| 19:32 | 6.81 | 387.7 | -2.74 | 6.8 | 387.7 | -2.7 |
| 19:31 | 5.92 | 376.1 | -1.45 | 5.9 | 376.1 | -1.4 |
| 19:30 | 9.43 | 374.4 | -4.00 | 9.4 | 374.4 | -4.0 |
| 19:29 | 13.16 | 388.6 | -5.70 | 13.2 | 388.6 | -5.7 |
| 19:28 | 11.58 | 407.3 | -1.06 | 11.6 | 407.3 | -1.1 |
| 19:27 | 7.97 | 408.0 | 1.09 | 8.0 | 408.0 | 1.1 |
| 19:26 | 7.59 | 392.1 | 2.05 | 7.6 | 392.1 | 2.0 |
| 19:25 | 11.83 | 401.5 | -0.80 | 11.8 | 401.5 | -0.8 |
| 19:24 | 14.06 | 402.7 | -1.95 | 14.1 | 402.7 | -1.9 |
| 19:23 | 6.57 | 379.4 | -2.13 | 6.6 | 379.4 | -2.1 |
| 19:22 | 7.45 | 366.2 | -3.61 | 7.4 | 366.2 | -3.6 |
| 19:21 | 11.27 | 389.8 | -5.23 | 11.3 | 389.8 | -5.2 |
| 19:20 | 12.44 | 392.4 | -5.15 | 12.4 | 392.4 | -5.2 |
| 19:19 | 14.63 | 392.6 | -5.95 | 14.6 | 392.6 | -6.0 |
| 19:18 | 7.43 | 374.6 | -6.10 | 7.4 | 374.6 | -6.1 |
| 19:17 | 8.90 | 378.0 | -6.11 | 8.9 | 378.0 | -6.1 |
| 19:16 | 9.79 | 385.6 | -6.37 | 9.8 | 385.6 | -6.4 |
| 19:15 | 10.83 | 386.2 | -6.00 | 10.8 | 386.2 | -6.0 |
| 19:14 | 9.11 | 373.1 | -2.39 | 9.1 | 373.1 | -2.4 |
| 19:13 | 3.64 | 361.9 | -3.36 | 9.2 | 369.2 | -3.4 |
| 19:12 | 13.45 | 380.9 | -4.97 | 13.5 | 380.9 | -5.0 |
| 19:11 | 14.19 | 384.2 | -2.56 | 14.2 | 384.2 | -2.6 |
| 19:10 | 12.44 | 378.3 | -1.58 | 12.4 | 378.3 | -1.6 |
| 19:09 | 13.19 | 371.2 | -3.72 | 13.2 | 371.2 | -3.7 |
| 19:08 | 11.16 | 387.2 | -2.81 | 11.2 | 387.2 | -2.8 |
| 19:07 | 11.55 | 385.4 | -1.04 | 11.5 | 385.4 | -1.0 |
| 19:06 | 12.89 | 386.4 | -1.81 | 12.9 | 386.4 | -1.8 |
| 19:05 | 13.22 | 384.7 | -1.13 | 13.2 | 384.7 | -1.1 |
| 19:04 | 9.52 | 382.8 | -2.87 | 9.5 | 382.8 | -2.9 |
| 19:03 | 11.81 | 400.8 | 0.54 | 11.8 | 400.8 | 0.5 |
| 19:02 | 11.89 | 390.6 | 2.30 | 11.9 | 390.6 | 2.3 |
| 19:01 | 11.79 | 386.9 | -0.46 | 11.8 | 386.9 | -0.5 |
| 19:00 | 7.82 | 370.5 | - | 7.8 | 370.5 | - |
| 18:59 | 10.08 | 378.0 | - | 10.1 | 378.0 | - |
| 18:58 | 12.94 | 381.8 | -1.08 | 12.9 | 381.8 | -1.1 |
| 18:57 | 15.73 | 383.4 | -2.96 | 15.7 | 383.4 | -3.0 |
| 18:56 | 10.92 | 387.3 | -3.34 | 13.8 | 379.8 | -3.3 |
| 18:55 | 8.26 | 370.8 | -3.31 | 8.3 | 370.8 | -3.3 |
| 18:54 | 11.22 | 379.5 | -3.14 | 11.2 | 379.5 | -3.1 |
| 18:53 | 14.96 | 387.2 | -2.58 | 15.0 | 387.2 | -2.6 |
| 18:52 | 13.51 | 387.0 | -3.08 | 13.5 | 387.0 | -3.1 |
| 18:51 | 4.87 | 363.0 | -3.66 | 4.9 | 363.0 | -3.7 |
| 18:50 | 10.28 | 379.6 | -2.49 | 10.3 | 379.6 | -2.5 |
| 18:49 | 12.45 | 380.0 | -1.60 | 12.5 | 380.0 | -1.6 |
| 18:48 | 12.89 | 369.7 | -2.24 | 12.9 | 369.7 | -2.2 |
| 18:47 | 6.42 | 353.9 | -3.91 | 6.4 | 353.9 | -3.9 |
| 18:46 | 8.56 | 361.6 | -4.61 | 8.6 | 361.6 | -4.6 |
| 18:45 | 12.49 | 365.3 | -4.74 | 12.5 | 365.3 | -4.7 |
| 18:44 | 11.71 | 364.6 | - | 11.7 | 364.6 | - |
| 18:43 | 7.62 | 359.0 | -4.07 | 7.6 | 359.0 | -4.1 |
| 18:42 | 8.35 | 361.8 | -3.53 | 8.4 | 361.8 | -3.5 |
| 18:41 | 11.21 | 369.7 | -2.90 | 12.7 | 374.5 | -2.9 |
| 18:40 | 7.03 | 372.0 | -1.73 | 13.3 | 378.3 | -1.7 |
| 18:39 | 9.96 | 368.4 | -2.58 | 10.0 | 368.4 | -2.6 |
| 18:38 | 8.57 | 364.7 | -3.17 | 8.6 | 364.7 | -3.2 |
| 18:37 | 11.40 | 372.0 | -3.18 | 11.4 | 372.0 | -3.2 |
| 18:36 | 12.35 | 369.2 | -3.32 | 12.3 | 369.2 | -3.3 |
| 18:35 | 13.39 | 372.0 | -3.78 | 13.4 | 372.0 | -3.8 |
| 18:34 | 10.85 | 367.5 | -3.94 | 10.9 | 367.5 | -3.9 |
| 18:33 | 10.41 | 366.9 | -4.82 | 10.4 | 366.9 | -4.8 |
| 18:32 | 11.28 | 375.2 | -5.10 | 11.3 | 375.2 | -5.1 |
| 18:31 | 12.64 | 377.6 | -4.19 | 12.6 | 377.6 | -4.2 |
| 18:30 | 11.25 | 376.7 | -4.64 | 11.3 | 376.7 | -4.6 |
| 18:29 | 7.55 | 366.9 | - | 7.5 | 366.9 | - |
| 18:28 | 6.26 | 363.1 | -4.61 | 6.3 | 363.1 | -4.6 |
| 18:27 | 10.32 | 372.2 | -3.52 | 10.3 | 372.2 | -3.5 |
| 18:26 | 12.47 | 379.0 | -3.29 | 12.5 | 379.0 | -3.3 |
| 18:25 | 9.75 | 377.4 | -3.39 | 9.7 | 377.4 | -3.4 |
| 18:24 | 2.45 | 367.6 | -3.20 | 6.2 | 372.7 | -3.2 |
| 18:23 | 9.50 | 379.9 | -3.02 | 9.5 | 379.9 | -3.0 |
| 18:22 | 9.77 | 380.9 | -3.11 | 9.8 | 380.9 | -3.1 |
| 18:21 | 10.25 | 384.5 | -2.58 | 10.2 | 384.5 | -2.6 |
| 18:20 | 4.39 | 361.2 | -2.29 | 4.4 | 361.2 | -2.3 |
| 18:19 | 10.55 | 379.2 | -2.70 | 10.6 | 379.2 | -2.7 |
| 18:18 | 11.91 | 378.1 | - | 11.9 | 378.1 | - |
| 18:17 | 13.20 | 389.1 | -2.70 | 13.2 | 389.1 | -2.7 |
| 18:16 | 7.63 | 366.5 | -2.99 | 7.6 | 366.5 | -3.0 |
| 18:15 | 9.50 | 378.4 | -3.04 | 9.5 | 378.4 | -3.0 |
| 18:14 | 10.47 | 379.9 | -3.07 | 10.5 | 379.9 | -3.1 |
| 18:13 | 11.69 | 386.7 | -3.20 | 11.6 | 386.3 | -3.2 |
| 18:12 | 7.32 | 371.9 | -3.35 | 7.3 | 371.9 | -3.3 |
| 18:11 | 7.93 | 372.7 | -3.41 | 7.9 | 372.7 | -3.4 |
| 18:10 | 9.91 | 379.3 | -3.23 | 10.1 | 379.6 | -3.2 |
| 18:09 | 9.91 | 379.4 | -3.17 | 10.1 | 379.7 | -3.2 |
| 18:08 | 9.65 | 377.7 | -3.69 | 9.0 | 375.9 | -3.7 |
| 18:07 | 8.68 | 373.6 | -3.81 | 7.7 | 370.9 | -3.8 |
| 18:06 | 9.57 | 376.0 | -3.30 | 9.6 | 376.0 | -3.3 |
| 18:05 | 10.96 | 378.9 | -2.86 | 11.0 | 378.9 | -2.9 |
| 18:04 | 10.45 | 377.3 | -3.54 | 10.5 | 377.3 | -3.5 |
| 18:03 | 10.40 | 372.0 | -3.29 | 10.4 | 372.0 | -3.3 |
| 18:02 | 10.64 | 374.9 | -3.88 | 10.6 | 374.9 | -3.9 |
| 18:01 | 12.42 | 378.4 | -3.56 | 12.4 | 378.4 | -3.6 |
| 18:00 | - | - | -3.51 | - | - | -3.5 |
| 17:59 | - | - | -3.46 | - | - | -3.5 |
| 17:58 | 13.17 | 376.7 | -2.64 | 13.2 | 376.7 | -2.6 |
| 17:57 | 14.33 | 382.6 | -1.20 | 14.3 | 382.6 | -1.2 |
| 17:56 | 13.30 | 383.3 | -0.90 | 13.3 | 383.3 | -0.9 |
Built 2026-04-25 19:56 from source
| Solar wind parameters of the latest hour by NOAA | |||
|---|---|---|---|
| parameter | min | max | mean |
| IMF Bz [nT] | -7.4 | 2.3 | -3.1 |
| velocity [km/s] | 353.9 | 408.0 | 383.2 |
| density [cm-3] | 3.6 | 15.7 | 10.1 |
| Geomagnetic activity (RX [nT]) | ||
|---|---|---|
| site | latest hour | next hour (RXmin, RXmax) |
| Kevo (KEV) | 261 | 35 | 410 |
| Maasi (MAS) | 236 | 27 | 372 |
| Kilpisjärvi (KIL) | 195 | 31 | 394 |
| Ivalo (IVA) | 190 | 21 | 400 |
| Muonio (MUO) | 145 | 20 | 414 |
| Sodankylä (SOD) | 104 | 16 | 392 |
| Pello (PEL) | 103 | 13 | 398 |
| Oulujärvi (OUJ) | 38 | 10 | 238 |
| Mekrijärvi (MEK) | 32 | 5 | 82 |
| Hankasalmi (HAN) | 47 | 7 | 71 |
| Nurmijärvi (NUR) | 28 | 7 | 57 |
| Tartu (TAR) | 27 | 5 | 37 |
| low | increased | moderate | high | very high |
Short explanation of the method
AurorasNow! (Finnish Meteorological Institute)Built 2026-04-25 19:47 from source
Issue Time: 2026-04-25 01:37 UTC
WARNING: Geomagnetic K-index of 4 expected
Valid From: 2026-04-25 01:37 UTC
Valid To: 2026-04-25 23:59 UTC
Warning Condition: Onset
Induced Currents - Weak power grid fluctuations can occur.
Aurora - Aurora may be visible at high latitudes such as Canada and Alaska.
WARNING: Geomagnetic K-index of 4 expected
Valid From: 2026-04-25 01:37 UTC
Valid To: 2026-04-25 23:59 UTC
Warning Condition: Onset
Induced Currents - Weak power grid fluctuations can occur.
Aurora - Aurora may be visible at high latitudes such as Canada and Alaska.
Issue Time: 2026-04-24 23:50 UTC
WATCH: Geomagnetic Storm Category G1 Predicted
Highest Storm Level Predicted by Day
Apr 25: G1 (Minor) Apr 26: G1 (Minor) Apr 27: None (Below G1)
THIS SUPERSEDES ANY/ALL PRIOR WATCHES IN EFFECT
Induced Currents - Weak power grid fluctuations can occur.
Spacecraft - Minor impact on satellite operations possible.
Aurora - Aurora may be visible at high latitudes, i.e., northern tier of the U.S. such as northern Michigan and Maine.
WATCH: Geomagnetic Storm Category G1 Predicted
Highest Storm Level Predicted by Day
Apr 25: G1 (Minor) Apr 26: G1 (Minor) Apr 27: None (Below G1)
THIS SUPERSEDES ANY/ALL PRIOR WATCHES IN EFFECT
Induced Currents - Weak power grid fluctuations can occur.
Spacecraft - Minor impact on satellite operations possible.
Aurora - Aurora may be visible at high latitudes, i.e., northern tier of the U.S. such as northern Michigan and Maine.
Issue Time: 2026-04-24 18:35 UTC
SUMMARY: X-ray Event exceeded M5
Begin Time: 2026-04-24 17:54 UTC
Maximum Time: 2026-04-24 18:15 UTC
End Time: 2026-04-24 18:30 UTC
X-ray Class: M6.4
Location: N19W90
NOAA Scale: R2 - Moderate
Radio - Limited blackout of HF (high frequency) radio communication for tens of minutes.
SUMMARY: X-ray Event exceeded M5
Begin Time: 2026-04-24 17:54 UTC
Maximum Time: 2026-04-24 18:15 UTC
End Time: 2026-04-24 18:30 UTC
X-ray Class: M6.4
Location: N19W90
NOAA Scale: R2 - Moderate
Radio - Limited blackout of HF (high frequency) radio communication for tens of minutes.
Issue Time: 2026-04-24 18:12 UTC
ALERT: X-Ray Flux exceeded M5
Threshold Reached: 2026-04-24 18:12 UTC
NOAA Scale: R2 - Moderate
ALERT: X-Ray Flux exceeded M5
Threshold Reached: 2026-04-24 18:12 UTC
NOAA Scale: R2 - Moderate
Issue Time: 2026-04-24 10:41 UTC
ALERT: Type IV Radio Emission
Begin Time: 2026-04-24 08:40 UTC
Description: Type IV emissions occur in association with major eruptions on the sun and are typically associated with strong coronal mass ejections and solar radiation storms.
ALERT: Type IV Radio Emission
Begin Time: 2026-04-24 08:40 UTC
Description: Type IV emissions occur in association with major eruptions on the sun and are typically associated with strong coronal mass ejections and solar radiation storms.
Issue Time: 2026-04-24 09:28 UTC
ALERT: Type II Radio Emission
Begin Time: 2026-04-24 08:15 UTC
Estimated Velocity: 1293 km/s
Comment: Reissued with adjusted shock speed.
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.
ALERT: Type II Radio Emission
Begin Time: 2026-04-24 08:15 UTC
Estimated Velocity: 1293 km/s
Comment: Reissued with adjusted shock speed.
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.
Issue Time: 2026-04-24 09:27 UTC
CANCEL ALERT: Type II Radio Emission
Cancel Serial Number: 1477
Original Issue Time: 2026-04-24 08:57 UTC
Comment: Reissuing with corrected shock speed.
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.
CANCEL ALERT: Type II Radio Emission
Cancel Serial Number: 1477
Original Issue Time: 2026-04-24 08:57 UTC
Comment: Reissuing with corrected shock speed.
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.
Issue Time: 2026-04-24 08:57 UTC
ALERT: Type II Radio Emission
Begin Time: 2026-04-24 08:15 UTC
Estimated Velocity: 1869 km/s
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.
ALERT: Type II Radio Emission
Begin Time: 2026-04-24 08:15 UTC
Estimated Velocity: 1869 km/s
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.
Issue Time: 2026-04-24 08:38 UTC
SUMMARY: 10cm Radio Burst
Begin Time: 2026-04-24 08:09 UTC
Maximum Time: 2026-04-24 08:11 UTC
End Time: 2026-04-24 08:15 UTC
Duration: 6 minutes
Peak Flux: 570 sfu
Latest Penticton Noon Flux: 128 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
SUMMARY: 10cm Radio Burst
Begin Time: 2026-04-24 08:09 UTC
Maximum Time: 2026-04-24 08:11 UTC
End Time: 2026-04-24 08:15 UTC
Duration: 6 minutes
Peak Flux: 570 sfu
Latest Penticton Noon Flux: 128 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
Issue Time: 2026-04-24 08:26 UTC
SUMMARY: X-ray Event exceeded X1
Begin Time: 2026-04-24 08:01 UTC
Maximum Time: 2026-04-24 08:13 UTC
End Time: 2026-04-24 08:18 UTC
X-ray Class: X2.5
Optical Class: 2b
Location: N20W90
NOAA Scale: R3 - Strong
Radio - Wide area blackout of HF (high frequency) radio communication for about an hour.
SUMMARY: X-ray Event exceeded X1
Begin Time: 2026-04-24 08:01 UTC
Maximum Time: 2026-04-24 08:13 UTC
End Time: 2026-04-24 08:18 UTC
X-ray Class: X2.5
Optical Class: 2b
Location: N20W90
NOAA Scale: R3 - Strong
Radio - Wide area blackout of HF (high frequency) radio communication for about an hour.
Issue Time: 2026-04-24 08:12 UTC
ALERT: X-Ray Flux exceeded M5
Threshold Reached: 2026-04-24 08:12 UTC
NOAA Scale: R2 - Moderate
ALERT: X-Ray Flux exceeded M5
Threshold Reached: 2026-04-24 08:12 UTC
NOAA Scale: R2 - Moderate
Issue Time: 2026-04-24 05:05 UTC
CONTINUED ALERT: Electron 2MeV Integral Flux exceeded 1000pfu
Continuation of Serial Number: 3683
Begin Time: 2026-04-19 19:20 UTC
Yesterday Maximum 2MeV Flux: 3446 pfu
CONTINUED ALERT: Electron 2MeV Integral Flux exceeded 1000pfu
Continuation of Serial Number: 3683
Begin Time: 2026-04-19 19:20 UTC
Yesterday Maximum 2MeV Flux: 3446 pfu
Issue Time: 2026-04-24 01:31 UTC
SUMMARY: X-ray Event exceeded X1
Begin Time: 2026-04-24 00:51 UTC
Maximum Time: 2026-04-24 01:07 UTC
End Time: 2026-04-24 01:13 UTC
X-ray Class: X2.4
Location: N17W71
NOAA Scale: R3 - Strong
Comment: Accompanied by a tenflare with a castelli-U signature. No radio observations currently available.
Radio - Wide area blackout of HF (high frequency) radio communication for about an hour.
SUMMARY: X-ray Event exceeded X1
Begin Time: 2026-04-24 00:51 UTC
Maximum Time: 2026-04-24 01:07 UTC
End Time: 2026-04-24 01:13 UTC
X-ray Class: X2.4
Location: N17W71
NOAA Scale: R3 - Strong
Comment: Accompanied by a tenflare with a castelli-U signature. No radio observations currently available.
Radio - Wide area blackout of HF (high frequency) radio communication for about an hour.
Issue Time: 2026-04-24 01:29 UTC
SUMMARY: 10cm Radio Burst
Begin Time: 2026-04-24 01:03 UTC
Maximum Time: 2026-04-24 01:04 UTC
End Time: 2026-04-24 01:09 UTC
Duration: 6 minutes
Peak Flux: 570 sfu
Latest Penticton Noon Flux: 128 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
SUMMARY: 10cm Radio Burst
Begin Time: 2026-04-24 01:03 UTC
Maximum Time: 2026-04-24 01:04 UTC
End Time: 2026-04-24 01:09 UTC
Duration: 6 minutes
Peak Flux: 570 sfu
Latest Penticton Noon Flux: 128 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
Issue Time: 2026-04-24 01:08 UTC
ALERT: X-Ray Flux exceeded M5
Threshold Reached: 2026-04-24 01:05 UTC
NOAA Scale: R2 - Moderate
ALERT: X-Ray Flux exceeded M5
Threshold Reached: 2026-04-24 01:05 UTC
NOAA Scale: R2 - Moderate
Issue Time: 2026-04-23 17:23 UTC
SUMMARY: 10cm Radio Burst
Begin Time: 2026-04-23 17:03 UTC
Maximum Time: 2026-04-23 17:05 UTC
End Time: 2026-04-23 17:07 UTC
Duration: 4 minutes
Peak Flux: 220 sfu
Latest Penticton Noon Flux: 116 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
SUMMARY: 10cm Radio Burst
Begin Time: 2026-04-23 17:03 UTC
Maximum Time: 2026-04-23 17:05 UTC
End Time: 2026-04-23 17:07 UTC
Duration: 4 minutes
Peak Flux: 220 sfu
Latest Penticton Noon Flux: 116 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
Issue Time: 2026-04-23 14:52 UTC
SUMMARY: 10cm Radio Burst
Begin Time: 2026-04-23 13:55 UTC
Maximum Time: 2026-04-23 13:56 UTC
End Time: 2026-04-23 13:57 UTC
Duration: 2 minutes
Peak Flux: 170 sfu
Latest Penticton Noon Flux: 116 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
SUMMARY: 10cm Radio Burst
Begin Time: 2026-04-23 13:55 UTC
Maximum Time: 2026-04-23 13:56 UTC
End Time: 2026-04-23 13:57 UTC
Duration: 2 minutes
Peak Flux: 170 sfu
Latest Penticton Noon Flux: 116 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
Issue Time: 2026-04-23 09:14 UTC
ALERT: Type II Radio Emission
Begin Time: 2026-04-23 08:59 UTC
Estimated Velocity: 722 km/s
Comment: Report from San Vito
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.
ALERT: Type II Radio Emission
Begin Time: 2026-04-23 08:59 UTC
Estimated Velocity: 722 km/s
Comment: Report from San Vito
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.
Issue Time: 2026-04-23 08:59 UTC
SUMMARY: 10cm Radio Burst
Begin Time: 2026-04-23 08:44 UTC
Maximum Time: 2026-04-23 08:44 UTC
End Time: 2026-04-23 08:44 UTC
Duration: 1 minutes
Peak Flux: 130 sfu
Latest Penticton Noon Flux: 116 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
SUMMARY: 10cm Radio Burst
Begin Time: 2026-04-23 08:44 UTC
Maximum Time: 2026-04-23 08:44 UTC
End Time: 2026-04-23 08:44 UTC
Duration: 1 minutes
Peak Flux: 130 sfu
Latest Penticton Noon Flux: 116 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
Issue Time: 2026-04-23 05:35 UTC
ALERT: Type IV Radio Emission
Begin Time: 2026-04-23 05:13 UTC
Comment: Report from San Vito
Description: Type IV emissions occur in association with major eruptions on the sun and are typically associated with strong coronal mass ejections and solar radiation storms.
ALERT: Type IV Radio Emission
Begin Time: 2026-04-23 05:13 UTC
Comment: Report from San Vito
Description: Type IV emissions occur in association with major eruptions on the sun and are typically associated with strong coronal mass ejections and solar radiation storms.
Issue Time: 2026-04-23 05:10 UTC
ALERT: Type II Radio Emission
Begin Time: 2026-04-23 04:50 UTC
Estimated Velocity: 1033 km/s
Comment: Report from San Vito
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.
ALERT: Type II Radio Emission
Begin Time: 2026-04-23 04:50 UTC
Estimated Velocity: 1033 km/s
Comment: Report from San Vito
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.
Issue Time: 2026-04-23 04:59 UTC
CONTINUED ALERT: Electron 2MeV Integral Flux exceeded 1000pfu
Continuation of Serial Number: 3682
Begin Time: 2026-04-19 19:20 UTC
Yesterday Maximum 2MeV Flux: 4922 pfu
CONTINUED ALERT: Electron 2MeV Integral Flux exceeded 1000pfu
Continuation of Serial Number: 3682
Begin Time: 2026-04-19 19:20 UTC
Yesterday Maximum 2MeV Flux: 4922 pfu
Built 2026-04-25 12:24 from source











