SettingsLast update:
| Time UTC | DSCOVR | ACE | ||||
|---|---|---|---|---|---|---|
| Solar Wind | GSM | Solar Wind | GSM | |||
| Proton Density | Bulk Speed | Bz | Proton Density | Bulk Speed | Bz | |
| 20:04 | - | - | - | - | - | - |
| 20:03 | - | - | - | - | - | - |
| 20:02 | - | - | - | - | - | - |
| 20:01 | 20.52 | 477.4 | - | - | - | - |
| 20:00 | 19.35 | 478.1 | 1.00 | - | - | - |
| 19:59 | 13.57 | 463.6 | 1.10 | - | - | - |
| 19:58 | 10.80 | 440.1 | 0.92 | - | - | - |
| 19:57 | 23.52 | 477.0 | 0.85 | - | - | - |
| 19:56 | 18.59 | 481.1 | 1.08 | - | - | - |
| 19:55 | 16.61 | 476.8 | 1.33 | - | - | - |
| 19:54 | 5.81 | 440.2 | 1.11 | - | - | - |
| 19:53 | 17.05 | 466.3 | 1.08 | - | - | - |
| 19:52 | 16.69 | 462.2 | 1.31 | - | - | - |
| 19:51 | 16.64 | 461.8 | 1.83 | - | - | - |
| 19:50 | - | - | 0.20 | - | - | - |
| 19:49 | - | - | -2.83 | - | - | - |
| 19:48 | 11.00 | 468.1 | -2.75 | - | - | - |
| 19:47 | 14.93 | 473.1 | -2.71 | 14.9 | 473.1 | -2.7 |
| 19:46 | 16.26 | 481.4 | -2.72 | 16.3 | 481.4 | -2.7 |
| 19:45 | 9.77 | 469.5 | -3.25 | 9.8 | 469.5 | -3.2 |
| 19:44 | 2.17 | 449.3 | -3.33 | 7.9 | 460.5 | -3.3 |
| 19:43 | 15.08 | 478.4 | -3.33 | 15.1 | 478.4 | -3.3 |
| 19:42 | 14.51 | 480.0 | -3.11 | 14.5 | 480.0 | -3.1 |
| 19:41 | 10.90 | 477.5 | -2.61 | 10.9 | 477.5 | -2.6 |
| 19:40 | 6.33 | 449.6 | -2.28 | 6.3 | 449.6 | -2.3 |
| 19:39 | 13.05 | 476.8 | -2.69 | 13.0 | 476.8 | -2.7 |
| 19:38 | 12.95 | 472.0 | -2.72 | 13.0 | 472.0 | -2.7 |
| 19:37 | 12.07 | 496.4 | -2.75 | 12.1 | 496.4 | -2.8 |
| 19:36 | 6.79 | 436.9 | -2.37 | 6.8 | 436.9 | -2.4 |
| 19:35 | 13.13 | 471.3 | -2.48 | 13.1 | 471.3 | -2.5 |
| 19:34 | 13.49 | 467.8 | -2.52 | 13.5 | 467.8 | -2.5 |
| 19:33 | 12.84 | 470.9 | -2.16 | 12.8 | 470.9 | -2.2 |
| 19:32 | 6.69 | 451.4 | -1.98 | 6.7 | 451.4 | -2.0 |
| 19:31 | 9.00 | 458.2 | -1.45 | 9.0 | 458.2 | -1.5 |
| 19:30 | 15.90 | 473.4 | -1.68 | 15.9 | 473.4 | -1.7 |
| 19:29 | 17.81 | 475.5 | -2.10 | 17.8 | 475.5 | -2.1 |
| 19:28 | 13.21 | 466.6 | -2.21 | 13.2 | 466.6 | -2.2 |
| 19:27 | 5.13 | 451.5 | -2.06 | 10.1 | 457.5 | -2.1 |
| 19:26 | 14.83 | 468.4 | -1.70 | 14.8 | 468.4 | -1.7 |
| 19:25 | 13.80 | 465.8 | -1.26 | 13.8 | 465.8 | -1.3 |
| 19:24 | 19.03 | 477.6 | -0.61 | 19.0 | 477.6 | -0.6 |
| 19:23 | 11.84 | 455.4 | 0.13 | 11.8 | 455.4 | 0.1 |
| 19:22 | 14.31 | 465.8 | 0.81 | 14.3 | 465.8 | 0.8 |
| 19:21 | 15.75 | 467.6 | 1.14 | 15.8 | 467.6 | 1.1 |
| 19:20 | 19.41 | 470.6 | -0.13 | 19.4 | 470.6 | -0.1 |
| 19:19 | 17.76 | 471.6 | 1.04 | 17.8 | 471.6 | 1.0 |
| 19:18 | 6.59 | 441.4 | 1.38 | 6.6 | 441.4 | 1.4 |
| 19:17 | 19.12 | 462.8 | 2.28 | 19.1 | 462.8 | 2.3 |
| 19:16 | 25.25 | 474.6 | 2.45 | 25.3 | 474.6 | 2.5 |
| 19:15 | 7.48 | 448.9 | 2.43 | 7.5 | 448.9 | 2.4 |
| 19:14 | 6.13 | 438.6 | - | 6.1 | 438.6 | - |
| 19:13 | 12.24 | 447.6 | 2.65 | 12.2 | 447.6 | 2.6 |
| 19:12 | 19.90 | 471.0 | 2.10 | 19.9 | 471.0 | 2.1 |
| 19:11 | 16.93 | 473.5 | 1.50 | 16.9 | 473.5 | 1.5 |
| 19:10 | 12.34 | 464.9 | 3.15 | 12.3 | 464.9 | 3.1 |
| 19:09 | 2.95 | 428.2 | 2.91 | 6.4 | 436.1 | 2.9 |
| 19:08 | 18.82 | 471.2 | 2.09 | 18.8 | 471.2 | 2.1 |
| 19:07 | 17.31 | 470.8 | 2.27 | 17.3 | 470.8 | 2.3 |
| 19:06 | 13.91 | 462.1 | 1.97 | 13.9 | 462.1 | 2.0 |
| 19:05 | 4.71 | 429.7 | 1.66 | 4.7 | 429.7 | 1.7 |
| 19:04 | 14.56 | 469.7 | 1.19 | 14.6 | 469.7 | 1.2 |
| 19:03 | 16.91 | 469.9 | 0.66 | 16.9 | 469.9 | 0.7 |
| 19:02 | 13.96 | 463.2 | 0.64 | 14.0 | 463.2 | 0.6 |
| 19:01 | 7.44 | 438.6 | 0.44 | 7.4 | 438.6 | 0.4 |
| 19:00 | 9.24 | 452.7 | 1.03 | 9.2 | 452.7 | 1.0 |
| 18:59 | 11.41 | 465.1 | -0.84 | 11.4 | 465.1 | -0.8 |
| 18:58 | 15.55 | 473.6 | 1.49 | 15.6 | 473.6 | 1.5 |
| 18:57 | 10.08 | 460.2 | 2.17 | 10.1 | 460.2 | 2.2 |
| 18:56 | 7.29 | 448.4 | 1.43 | 7.3 | 448.4 | 1.4 |
| 18:55 | 11.24 | 461.1 | 1.74 | 11.2 | 461.1 | 1.7 |
| 18:54 | 12.82 | 463.8 | 1.82 | 12.8 | 463.8 | 1.8 |
| 18:53 | 14.60 | 467.3 | 1.61 | 14.6 | 467.3 | 1.6 |
| 18:52 | 15.73 | 469.5 | 1.44 | 15.7 | 469.5 | 1.4 |
| 18:51 | 8.04 | 454.7 | 1.75 | 8.0 | 454.7 | 1.7 |
| 18:50 | 11.60 | 459.5 | 1.84 | 11.6 | 459.5 | 1.8 |
| 18:49 | 18.07 | 472.1 | 1.79 | 18.1 | 472.1 | 1.8 |
| 18:48 | 16.89 | 471.7 | 1.57 | 16.9 | 471.7 | 1.6 |
| 18:47 | 5.49 | 446.7 | 1.61 | 5.5 | 446.7 | 1.6 |
| 18:46 | 10.63 | 460.7 | 1.80 | 10.6 | 460.7 | 1.8 |
| 18:45 | - | - | 1.58 | - | - | 1.6 |
| 18:44 | - | - | 1.85 | - | - | 1.9 |
| 18:43 | - | - | 1.97 | - | - | 2.0 |
| 18:42 | 10.72 | 459.1 | 2.13 | 10.7 | 459.1 | 2.1 |
| 18:41 | 13.16 | 464.7 | 2.18 | 13.2 | 464.7 | 2.2 |
| 18:40 | 12.93 | 465.4 | 2.66 | 12.9 | 465.4 | 2.7 |
| 18:39 | 7.02 | 449.8 | 2.62 | 7.0 | 449.8 | 2.6 |
| 18:38 | 7.43 | 444.4 | 2.14 | 7.4 | 444.4 | 2.1 |
| 18:37 | 13.90 | 471.0 | 2.86 | 13.9 | 471.0 | 2.9 |
| 18:36 | 15.34 | 492.0 | 3.02 | 15.3 | 492.0 | 3.0 |
| 18:35 | - | - | 2.89 | - | - | 2.9 |
| 18:34 | - | - | 3.87 | - | - | 3.9 |
| 18:33 | 6.28 | 465.0 | 5.12 | 6.3 | 465.0 | 5.1 |
| 18:32 | 6.86 | 463.8 | 4.87 | 6.9 | 463.8 | 4.9 |
| 18:31 | 6.78 | 463.5 | 4.80 | 6.8 | 463.5 | 4.8 |
| 18:30 | 6.71 | 464.5 | 4.90 | 6.7 | 464.5 | 4.9 |
| 18:29 | 6.70 | 464.8 | 4.35 | 6.7 | 464.8 | 4.3 |
| 18:28 | 7.36 | 465.7 | 4.75 | 7.4 | 465.7 | 4.7 |
| 18:27 | 7.45 | 465.9 | 4.63 | 7.5 | 465.9 | 4.6 |
| 18:26 | 7.96 | 468.7 | 4.55 | 8.0 | 468.7 | 4.6 |
| 18:25 | 9.05 | 467.8 | 4.33 | 9.1 | 467.8 | 4.3 |
| 18:24 | 9.21 | 464.5 | 4.62 | 9.2 | 464.5 | 4.6 |
| 18:23 | 8.62 | 465.6 | 5.01 | 8.6 | 465.6 | 5.0 |
| 18:22 | 9.16 | 464.5 | 4.97 | 9.2 | 464.5 | 5.0 |
| 18:21 | 8.97 | 464.3 | 4.64 | 9.0 | 464.3 | 4.6 |
| 18:20 | 8.35 | 463.1 | 4.28 | 8.3 | 463.1 | 4.3 |
| 18:19 | 8.05 | 461.4 | 4.06 | 8.1 | 461.4 | 4.1 |
| 18:18 | 7.47 | 459.3 | 5.63 | 7.5 | 459.3 | 5.6 |
| 18:17 | 7.35 | 461.8 | 5.52 | 7.4 | 461.8 | 5.5 |
| 18:16 | 7.33 | 465.6 | 5.37 | 7.3 | 465.6 | 5.4 |
| 18:15 | 7.32 | 465.9 | 5.55 | 7.3 | 465.9 | 5.5 |
| 18:14 | - | - | 5.32 | - | - | 5.3 |
| 18:13 | 6.75 | 462.7 | 5.51 | 6.7 | 462.7 | 5.5 |
| 18:12 | 6.89 | 462.6 | 5.15 | 6.9 | 462.6 | 5.1 |
| 18:11 | 6.11 | 457.3 | 5.02 | 6.1 | 457.3 | 5.0 |
| 18:10 | 5.50 | 453.4 | 5.38 | 5.5 | 453.4 | 5.4 |
| 18:09 | 5.11 | 457.0 | 5.86 | 5.1 | 457.0 | 5.9 |
| 18:08 | 5.18 | 455.4 | 5.68 | 5.2 | 455.4 | 5.7 |
| 18:07 | 4.91 | 453.9 | 5.27 | 4.9 | 453.9 | 5.3 |
| 18:06 | 4.43 | 456.9 | 5.26 | 4.4 | 456.9 | 5.3 |
| 18:05 | 5.21 | 458.4 | 5.30 | 5.2 | 458.4 | 5.3 |
Built 2026-04-26 20:05 from source
| Solar wind parameters of the latest hour by NOAA | |||
|---|---|---|---|
| parameter | min | max | mean |
| IMF Bz [nT] | -3.3 | 3.1 | -0.3 |
| velocity [km/s] | 428.2 | 496.4 | 464.0 |
| density [cm-3] | 2.2 | 25.2 | 13.1 |
| Geomagnetic activity (RX [nT]) | ||
|---|---|---|
| site | latest hour | next hour (RXmin, RXmax) |
| Kevo (KEV) | 22 | 12 | 321 |
| Maasi (MAS) | 23 | 11 | 318 |
| Kilpisjärvi (KIL) | 10 | 10 | 321 |
| Ivalo (IVA) | 18 | 7 | 264 |
| Muonio (MUO) | 9 | 7 | 242 |
| Sodankylä (SOD) | 11 | 6 | 221 |
| Pello (PEL) | 19 | 6 | 217 |
| Oulujärvi (OUJ) | 28 | 5 | 87 |
| Mekrijärvi (MEK) | 25 | 3 | 35 |
| Hankasalmi (HAN) | 21 | 4 | 44 |
| Nurmijärvi (NUR) | 33 | 4 | 41 |
| Tartu (TAR) | 30 | 3 | 30 |
| low | increased | moderate | high | very high |
Short explanation of the method
AurorasNow! (Finnish Meteorological Institute)Built 2026-04-26 20:02 from source
Issue Time: 2026-04-26 11:47 UTC
EXTENDED WARNING: Geomagnetic K-index of 4 expected
Extension to Serial Number: 5328
Valid From: 2026-04-26 03:59 UTC
Now Valid Until: 2026-04-26 23:59 UTC
Warning Condition: Persistence
Induced Currents - Weak power grid fluctuations can occur.
Aurora - Aurora may be visible at high latitudes such as Canada and Alaska.
EXTENDED WARNING: Geomagnetic K-index of 4 expected
Extension to Serial Number: 5328
Valid From: 2026-04-26 03:59 UTC
Now Valid Until: 2026-04-26 23:59 UTC
Warning Condition: Persistence
Induced Currents - Weak power grid fluctuations can occur.
Aurora - Aurora may be visible at high latitudes such as Canada and Alaska.
Issue Time: 2026-04-26 06:01 UTC
WARNING: Geomagnetic K-index of 4 expected
Valid From: 2026-04-26 03:59 UTC
Valid To: 2026-04-26 12:00 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: 2026-04-26 03:59 UTC
Valid To: 2026-04-26 12:00 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: 2026-04-26 05:59 UTC
ALERT: Geomagnetic K-index of 4
Threshold Reached: 2026-04-26 05:59 UTC
Synoptic Period: 0300-0600 UTC
Active Warning: Yes
Induced Currents - Weak power grid fluctuations can occur.
Aurora - Aurora may be visible at high latitudes such as Canada and Alaska.
ALERT: Geomagnetic K-index of 4
Threshold Reached: 2026-04-26 05:59 UTC
Synoptic Period: 0300-0600 UTC
Active Warning: Yes
Induced Currents - Weak power grid fluctuations can occur.
Aurora - Aurora may be visible at high latitudes such as Canada and Alaska.
Issue Time: 2026-04-25 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.
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