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Solar Cycle 25 Flagship Hub

Solar Cycle 25: The Awakening

Real-time NOAA telemetry, deep dives, and cutting-edge coverage of the electromagnetic frontier — the Sun's surge, Schumann resonance, interoceptive awareness, CME velocity trends, and X-class flare coverage.

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Live Space Weather

Real-time data from NOAA Space Weather Prediction Center · updated 06:09:59

Latest Flare
B-class
Current class
Solar Wind
393 km/s
2.2 p/cm³
Kp Index
Kp 2.7
Quiet
Geo Storm
Quiet
Stable
K-index
2.7
Quiet
Solar Wind
393 km/s
Density: 2.2 p/cm³
X-Ray Class
B
Flux: 5.2e-7 W/m²
Geo Storm
Quiet
Kp threshold: 3

Geomagnetic Activity Map

Kp 2.7392.58 km/s solar wind
☀N POLES POLEQuietUnsettledStormSevere

Auroral oval expands equatorward with increasing Kp. Current Kp 2.7 — aurora confined to polar regions.

SDO Live Solar Imagery

NASA SDO
Continuum (Sunspots)
SUNSPOTS

Continuum (Sunspots)

HMI Intensitygram — shows sunspot regions as dark magnetic flux concentrations on the photosphere.

Images update every ~15 min from NASA SDO

Aurora Forecast

NOAA 3-Day Kp Model
31/ 100

Low

Aurora Likelihood

Conditions are marginal. Kp 2.7 — auroras likely limited to higher latitudes (75°+). Monitor for rising Kp trends.

Current Kp

2.7

Solar Wind

393 km/s

Visible from

75°+

3-Day Kp Forecast

10-28
Kp 2
10-29
Kp 2
10-30
Kp 4

Solar Wind Speed (km/s)

06:2706:2506:2406:2306:2206:2106:2006:1906:1806:1806:1706:1606:1506:1406:1306:1206:1106:1006:0906:08375390405420435

Planetary K-index (Kp)

06:0012:0018:0000:0006:0012:0018:0000:0006:0012:0018:0003:000369Kp5

NOAA Active Alerts

2026-11-03 05:02:29.447

Space Weather Message Code: ALTEF3 Serial Number: 3765 Issue Time: 2026 Nov 03 0502 UTC CONTINUED ALERT: Electron 2MeV Integral Flux exceeded 1,000pfu Continuation of Serial Number: 3764 Begin Time: 2026 Nov 01 1302 UTC Yesterday Maximum 2MeV Flux: 4481 pfu Max time: 2026 Nov 02 1540 UTC

2026-11-02 12:03:53.987

Space Weather Message Code: ALTEF3 Serial Number: 3764 Issue Time: 2026 Nov 02 1203 UTC CONTINUED ALERT: Electron 2MeV Integral Flux exceeded 1,000pfu Continuation of Serial Number: 3763 Begin Time: 2026 Nov 01 1302 UTC Yesterday Maximum 2MeV Flux: 5350 pfu Max time: 2026 Nov 01 1550 UTC

2026-11-01 14:57:52.780

Space Weather Message Code: WARK04 Serial Number: 5446 Issue Time: 2026 Nov 01 1457 UTC EXTENDED WARNING: Geomagnetic K-index of 4 expected Extension to Serial Number: 5445 Valid From: 2026 Oct 31 1235 UTC Now Valid Until: 2026 Nov 01 2359 UTC Warning Condition: Persistence NOAA Space Weath

2026-11-01 13:02:29.493

Space Weather Message Code: ALTEF3 Serial Number: 3763 Issue Time: 2026 Nov 01 1302 UTC ALERT: Electron 2MeV Integral Flux exceeded 1,000pfu Threshold Reached: 2026 Nov 01 1302 UTC Station: GOES-19 Comment:

2026-11-01 01:17:17.120

Space Weather Message Code: ALTK05 Serial Number: 2060 Issue Time: 2026 Nov 01 0117 UTC ALERT: Geomagnetic K-index of 5 Threshold Reached: 2026 Nov 01 0117 UTC Synoptic Period: 0000-0300 Active Warning: YES Noaa Scale: G1 - Minor Comment: NOAA Scale: G1 - Minor NOAA Space Weather Scale

Solar Event Feed

No events detected in the 7-day window.
Open the Time Scrubber to enable jump-to-event.

Active Solar Regions (ARs)

174 regions · NOAA SWPC
AR #
Location
Mag Class
C%
M%
X%
AR 4549N10E15BGD
55%
10%
1%
AR 4547N15W46B
20%
5%
1%
AR 4545N20E07BG
25%
5%
1%
AR 4548S12E38A
10%
1%
1%
AR 4547N15W59B
30%
5%
1%
AR 4549N10E01BGD
75%
35%
5%
AR 4545N19W06B
30%
10%
1%
AR 4548S12E25A
10%
1%
1%
AR 4548S12E13A
10%
1%
1%
AR 4549N10W13BGD
65%
30%
5%
AR 4545N18W19B
30%
10%
1%
AR 4550S15W22B
10%
1%
1%
AR 4547N15W73A
5%
1%
1%
AR 4549N10W29BGD
80%
55%
10%
AR 4545N17W33B
25%
5%
1%
AR 4548S13W01A
10%
1%
1%
AR 4548S13W14A
10%
1%
1%
AR 4552N22W21B
20%
5%
1%
AR 4545N18W46B
30%
5%
1%
AR 4549N10W41BGD
80%
50%
5%
AR 4551S13E71B
30%
5%
1%
AR 4552N22W34B
5%
1%
1%
AR 4548S13W26A
10%
1%
1%
AR 4551S14E61B
55%
15%
5%
AR 4545N17W60B
15%
1%
1%
AR 4549N09W54BGD
99%
65%
10%
AR 4548S13W39A
5%
1%
1%
AR 4545N16W73B
10%
1%
1%
AR 4553N07E60A
5%
1%
1%
AR 4551S15E47BG
55%
15%
1%
AR 4549N09W67BD
75%
50%
10%
AR 4554N07E61B
10%
1%
1%
AR 4555S08W17B
15%
1%
1%
AR 4549N09W81B
30%
5%
1%
AR 4548S13W53A
5%
1%
1%
AR 4551S15E34B
55%
15%
1%
AR 4553N07E47B
5%
1%
1%
AR 4555S06W30B
5%
1%
1%
AR 4551S15E21BG
50%
10%
1%
AR 4556N03E59B
10%
1%
1%
AR 4554N07E48B
15%
1%
1%
AR 4557N06E57B
15%
1%
1%
AR 4549N09W95B
25%
5%
1%
AR 4548S13W66A
10%
1%
1%
AR 4551S15E07BGD
75%
25%
10%
AR 4548S13W79A
5%
1%
1%
AR 4556N03E45B
10%
1%
1%
AR 4549N09W0*B
0%
0%
0%
AR 4553N06E20A
5%
1%
1%
AR 4557N07E43B
15%
5%
1%
AR 4554N07E33A
5%
1%
1%
AR 4558S08W34A
5%
1%
1%
AR 4555S07W43B
10%
1%
1%
AR 4555S07W56B
5%
1%
1%
AR 4553N06E06A
5%
1%
1%
AR 4551S15W06BGD
85%
25%
10%
AR 4557N07E29B
35%
5%
1%
AR 4548S13W93A
5%
1%
1%
AR 4555S08W70B
15%
1%
1%
AR 4548S13W0*A
0%
0%
0%
AR 4557N07E16B
35%
5%
1%
AR 4551S14W19BG
80%
20%
5%
AR 4551S15W32BG
70%
15%
5%
AR 4557N17E01B
50%
10%
1%
AR 4555S07W84A
5%
1%
1%
AR 4560N14E12B
15%
1%
1%
AR 4557N06W13B
60%
15%
5%
AR 4559S19W37B
10%
1%
1%
AR 4555S07W99A
0%
0%
0%
AR 4551S16W46BG
65%
20%
5%
AR 4560N14W01B
15%
5%
1%
AR 4557N06W28B
55%
10%
5%
AR 4551S15W59BG
70%
25%
5%
AR 4557N07W41BG
50%
10%
1%
AR 4560N13W14BG
50%
10%
1%
AR 4551S15W71BG
55%
15%
1%
AR 4557N07W55B
25%
5%
1%
AR 4560N13W28BG
50%
10%
1%
AR 4551S16W85BG
55%
15%
1%
AR 4560N13W42BG
60%
15%
5%
AR 4551S15W97BG
55%
15%
1%
AR 4557N07W68B
35%
5%
1%
AR 4557N07W82B
25%
5%
1%
AR 4560N13W58BG
60%
15%
1%
AR 4557N07W97B
0%
0%
0%
AR 4560N13W72BG
60%
10%
1%
AR 4560N13W84B
50%
10%
1%
AR 4561S11W77B
50%
10%
1%
AR 4562S17E49A
5%
1%
1%
AR 4560N13W98B
0%
0%
0%
AR 4562S17E34A
5%
1%
1%
AR 4561S11W91B
50%
10%
1%
AR 4563S19W70B
10%
1%
1%
AR 4561S11W0*B
0%
0%
0%
AR 4563S18W81A
10%
1%
1%
AR 4564N05E68A
10%
1%
1%
AR 4563S19W94A
5%
1%
1%
AR 4564N04E56B
10%
1%
1%
AR 4565N12E75A
5%
1%
1%
AR 4564N04E44B
20%
1%
1%
AR 4565N13E63A
5%
1%
1%
AR 4563S19W0*A
0%
0%
0%
AR 4564N04E29B
20%
1%
1%
AR 4565N14E47A
5%
1%
1%
AR 4565N13E35A
10%
1%
1%
AR 4564N03E11A
10%
1%
1%
AR 4566S07E66B
15%
5%
1%
AR 4566S06E53BGD
40%
15%
5%
AR 4564N03W02A
10%
1%
1%
AR 4565N14E20A
15%
5%
1%
AR 4544S09W99—
0%
0%
0%
AR 4546S19W88—
0%
0%
0%
AR 4546S19W0*—
0%
0%
0%
AR 4550S16W37—
1%
1%
1%
AR 4547N15W87—
1%
1%
1%
AR 4547N15W0*—
0%
0%
0%
AR 4550S16W51—
1%
1%
1%
AR 4550S16W65—
1%
1%
1%
AR 4552N23W45—
1%
1%
1%
AR 4550S16W79—
1%
1%
1%
AR 4550S16W93—
0%
0%
0%
AR 4545N17W86—
1%
1%
1%
AR 4552N23W59—
1%
1%
1%
AR 4545N17W0*—
0%
0%
0%
AR 4552N23W73—
0%
0%
0%
AR 4553N07E47—
1%
1%
1%
AR 4552N23W87—
1%
1%
1%
AR 4552N23W0*—
0%
0%
0%
AR 4558S08W48—
1%
1%
1%
AR 4556N03E32—
1%
1%
1%
AR 4554N07E20—
1%
1%
1%
AR 4558S08W62—
0%
0%
0%
AR 4554N07E05—
0%
0%
0%
AR 4556N03E17—
0%
0%
0%
AR 4553N06W09—
0%
0%
0%
AR 4554N07W10—
0%
0%
0%
AR 4553N06W24—
0%
0%
0%
AR 4558S08W76—
0%
0%
0%
AR 4556N03E03—
0%
0%
0%
AR 4556N03W12—
0%
0%
0%
AR 4554N07W25—
0%
0%
0%
AR 4553N06W39—
0%
0%
0%
AR 4558S08W90—
0%
0%
0%
AR 4558S08W0*—
0%
0%
0%
AR 4556N03W27—
1%
1%
1%
AR 4559S19W51—
1%
1%
1%
AR 4554N07W40—
1%
1%
1%
AR 4553N06W54—
1%
1%
1%
AR 4554N07W54—
1%
1%
1%
AR 4559S20W64—
5%
1%
1%
AR 4553N06W68—
1%
1%
1%
AR 4556N03W41—
1%
1%
1%
AR 4556N03W55—
1%
1%
1%
AR 4559S20W78—
1%
1%
1%
AR 4553N06W82—
1%
1%
1%
AR 4554N07W68—
1%
1%
1%
AR 4559S20W92—
0%
0%
0%
AR 4553N06W97—
0%
0%
0%
AR 4556N03W69—
1%
1%
1%
AR 4554N07W82—
1%
1%
1%
AR 4556N03W84—
1%
1%
1%
AR 4554N07W97—
0%
0%
0%
AR 4556N03W99—
0%
0%
0%
AR 4562S17E20—
1%
1%
1%
AR 4562S17E13—
1%
1%
1%
AR 4562S17W01—
1%
1%
1%
AR 4562S17W15—
0%
0%
0%
AR 4562S17W29—
0%
0%
0%
AR 4562S17W43—
1%
1%
1%
AR 4562S17W57—
1%
1%
1%
AR 4562S17W71—
0%
0%
0%
AR 4564N02W16—
0%
0%
0%
AR 4566S03E47—
0%
0%
0%
AR 4565N17E07—
0%
0%
0%
Click any row to expand. Sort by column header. Probabilities are 24-hour forecasts.

X-Ray Flux — Solar Flare Activity (log₁₀ W/m²)

Flare classes: A < -7 · B -7 · C -6 · M -5 · X ≥ -4

05:0705:1005:1305:1605:1905:2205:2505:2805:3105:3405:3705:4005:4305:4605:4905:5205:5505:5806:0106:06-9-7-5-3MX
Active Region 4551 Fires an M1.7 Flare as the Coronal Hole Stream Nears Earth
Space Weather & SolarCurrent

Active Region 4551 Fires an M1.7 Flare as the Coronal Hole Stream Nears Earth

The flare arrived at 09:03 UTC on October 19, delivering an R1 radio blackout. The region's delta signature has decayed, NOAA's X-class probability has eased to 5 percent, and the coronal hole stream remains on track for a G1 watch beginning October 20.

E. L. Corvin· 2026-10-19· 3 min
Active Region 4551: A Complex Sunspot Group Turns to Face Earth
Space Weather & SolarCurrent

Active Region 4551: A Complex Sunspot Group Turns to Face Earth

NOAA's own models give the Earth-facing Beta-Gamma-Delta region a 10% chance of an X-class flare in the next 24 hours. A coronal hole high-speed stream now adds a G1 geomagnetic storm forecast for October 19-20.

E. L. Corvin· 2026-10-18· 4 min
Solar Cycles 101: A Beginner's Guide to Solar Weather
Space Weather & SolarClassic

Solar Cycles 101: A Beginner's Guide to Solar Weather

Everything you need to know about Solar Cycle 25, solar flares, geomagnetic storms, and how to read the charts — your welcome center to Star-Field's solar coverage.

E. L. Corvin· 2026-09-23
Solar Cycle 25 Is Pressing Space Weather to Its Forecasting Limit
Space Weather & SolarCurrent

Solar Cycle 25 Is Pressing Space Weather to Its Forecasting Limit

The sunspot rhythm first recognized in the 19th century is now a live test of how well science can anticipate eruptions that affect technology on Earth.

E. L. Corvin· 2026-09-23· 5 min
Parker Solar Probe Traces How Alfvén Waves May Heat the Solar Corona
Space Weather & SolarCurrent

Parker Solar Probe Traces How Alfvén Waves May Heat the Solar Corona

Near the Sun, magnetic waves do more than carry energy outward: they appear to shed it into the corona through turbulence, reflection, and abrupt reversals.

E. L. Corvin· 2026-09-23· 4 min
The Solar Surge: Why Cycle 25 Is Defying Our Best Predictions
Space Weather & SolarCurrent

The Solar Surge: Why Cycle 25 Is Defying Our Best Predictions

As Solar Cycle 25 hits its peak, the Sun is unleashing a relentless barrage of X-class flares that far exceed initial scientific forecasts.

Kairos Research Desk· 2026-09-23· 5 min
Velocity and Violence: Decoding the High-Speed CMEs of Solar Cycle 25
Space Weather & SolarCurrent

Velocity and Violence: Decoding the High-Speed CMEs of Solar Cycle 25

As Solar Cycle 25 reaches its peak, the increasing frequency of high-velocity coronal mass ejections is challenging our predictive models and reshaping our understanding of space weather risks.

Kairos Research Desk· 2026-09-23· 5 min
Solar Cycle 25: The Growing Impact of the Suns Unpredictable Intensity
Space Weather & SolarDeep Dive

Solar Cycle 25: The Growing Impact of the Suns Unpredictable Intensity

How this solar maximum is reshaping space weather—and how the strongest solar activity in two decades, is exposing the limits of our forecasting models.

Kairos Research Desk· 2026-09-23· 6 min
How Eugene Parker Proved the Sun Was Blowing a Wind
Space Weather & SolarCurrent

How Eugene Parker Proved the Sun Was Blowing a Wind

A once-dismissed prediction became a cornerstone of space-weather science—and still shapes how we understand the Sun’s reach.

E. L. Corvin· 2026-09-16· 4 min
Where the Power Goes: Coronal Magnetic Reconnection and the Energy Budget of X‑Class Solar Flares
Space Weather & SolarCurrent

Where the Power Goes: Coronal Magnetic Reconnection and the Energy Budget of X‑Class Solar Flares

High-resolution observations and new diagnostics are finally constraining how reconnection in the corona partitions the colossal magnetic energy released in X‑class eruptions.

E. L. Corvin· 2026-09-03· 4 min
From Schwabe's Notebook to Power-Grid Alerts: How the Sun’s 11‑Year Pulse Shapes Modern Space Weather
Space Weather & SolarOverlooked

From Schwabe's Notebook to Power-Grid Alerts: How the Sun’s 11‑Year Pulse Shapes Modern Space Weather

An 1840s amateur discovery became the backbone—and the blind spot—of contemporary space‑weather forecasting.

E. L. Corvin· 2026-07-24· 3 min
How Coronal Magnetic Reconnection Powers X‑Class Solar Flares — Closing the Energy Budget
Space Weather & SolarCurrent

How Coronal Magnetic Reconnection Powers X‑Class Solar Flares — Closing the Energy Budget

New observations and global energetics analyses are converging on reconnection as the central engine for the largest flares, but key gaps in how magnetic energy is measured and partitioned remain.

E. L. Corvin· 2026-07-24· 4 min