☀ SolarEvidence

Live Space Weather & Solar Dashboard

Real-time space weather, live spacecraft views of the Sun, and Earth's magnetic shield status—updated every build (Sat Oct 31, 8:58 PM ET) and refreshed in your browser from NOAA SWPC, WDC Kyoto, and NASA SDO.

☀ LIVE SPACE WEATHER IN PLAIN ENGLISH

What the Sun and Earth's Magnetic Shield Are Doing Right Now

Updated Sat Oct 31, 8:58 PM ET from live NOAA satellites
1. NORTHERN LIGHTS TONIGHT
Kp 3.7 / 9

Minor storm level (G1) possible: an outside chance along the northern US border

24-hour peak forecast: Kp 4.7 (Kp 5+ is a storm). Good for high latitudes (Alaska, Canada, Iceland, Norway, Lapland) on clear nights.

Check My City → Full 24h forecast →

2. SOLAR WIND & EARTH'S SHIELD
525 km/s

Moderate Solar Wind (~1,174,394 mph)

Earth's magnetic shield is holding steady at 10.4 Earth radii (~41,215 miles) up on the sunlit side. Solar-wind magnetic direction (Bz): -2 nT (pointing south — helps aurora).

Live magnetic shield diagram →

3. SOLAR FLARES & GRID ALERTS
G0Geomagnetic
S0Radiation
R0Radio

Quiet Today (Level 0 out of 5)

NOAA rates storms from 0 (calm) to 5 (extreme). Latest bulletin: WARNING: Geomagnetic K-index of 5 expected…

How storms affect power grids →

The Sun Right Now (Live Spacecraft Views)

Left shows the cooler lower atmosphere and erupting filaments (GOES-19 SUVI 304 Å). Right shows the million-degree outer corona and dark coronal holes that send fast solar wind toward Earth (NASA SDO AIA 193 Å).

The Sun right now

The full Sun in extreme ultraviolet at 304 ångströms from the GOES-19 SUVI imager, showing the chromosphere, bright active regions and prominences on the limb, observed 2026-11-01 00:48 UTC
GOES-19 SUVI, 304 ÅSUVI 304 Å20:48 ETChromosphere and prominences, gas at about 50,000 to 80,000 K.NOAA/SWPC, public domainPD
The full Sun in extreme ultraviolet at 193 ångströms from NASA's Solar Dynamics Observatory, showing the corona, bright active regions and dark coronal holes, posted 2026-11-01 00:53 UTC
SDO AIA, 193 ÅSDO 193 Å20:53 ETCorona at about 1.2 million K; dark patches are coronal holes, sources of fast solar wind.NASA/SDO, public domainPD · credits

Raw Satellite Telemetry & Recent Solar Activity

L1 Solar Wind & IMF Telemetry

Solar wind speed525 km/s
Proton density3.1 protons/cm³
Total field strength (Bt)8 nT
North–South field (Bz GSM)-2 nT

Updated 2026-11-01T00:47:00Z (spacecraft: ACE). Data: NOAA SWPC.

Recent GOES X-Ray Flares & SWPC Bulletins

  • 2026-11-01 00:08 UTC WARNING: Geomagnetic K-index of 5 expected
  • 2026-10-31 19:14 UTC ALERT: Geomagnetic K-index of 6
  • 2026-10-31 19:08 UTC WARNING: Geomagnetic K-index of 6 expected
  • 2026-10-31 19:07 UTC ALERT: Geomagnetic K-index of 5

Strongest GOES X-ray flares (last 7 days)

  • 2026-10-31 20:51 UTC class B4.0
  • 2026-10-31 20:37 UTC class B3.6
  • 2026-10-31 19:55 UTC class B5.9
  • 2026-10-31 19:13 UTC class B4.1
  • 2026-10-31 15:42 UTC class B3.8

NASA DONKI CMEs (build snapshot 2026-10-18 to 2026-11-01, fetched 2026-11-01 00:58 UTC):

  • 2026-10-31 05:00 UTC 345 km/s · CME first seen to the West by SOHO LASCO C2 beginning at 2026-10-31T05:00Z, as well as by SOHO LASCO C3 and GOES CCOR-1 in later frames. Thi · DONKI
  • 2026-10-30 12:36 UTC 218 km/s · Very minor and faint CME seen to the W in SOHO LASCO C2/C3 and in GOES CCOR-1 coronagraphs and not seen in STEREO A COR2. Its source is a ve · DONKI
  • 2026-10-29 10:36 UTC 287 km/s · This CME is visible to the west in SOHO LASCO C2/C3 and GOES CCOR-1 and to the east in STEREO A COR2 imagery. The source is a filament erupt · DONKI
  • 2026-10-28 11:12 UTC 329 km/s · Faint CME observed to the SW in SOHO LASCO C2/C3 and GOES CCOR-1, also very faintly observed to the SW in STEREO A COR2 and difficult to res · DONKI

Live Space-Weather & Storm Event Brief G1 · Minor geomagnetic storm

Auto-updated Sat Oct 31, 8:58 PM ET

Timestamped summary card combining NOAA SWPC planetary Kp, L1 solar wind, Shue et al. (1998) magnetopause standoff distance, and estimated equatorward aurora horizon reach. Free to link, download or embed (CC0 public domain).

Solar Evidence Live Space-Weather Brief: G1 · Minor geomagnetic storm, Kp now 3.67, 24h max 4.67, solar wind 525 km/s, Bz -2.0 nT (south), magnetopause 10.4 RE
Download SVG card Check your city's Kp threshold → 38 vetted 3★+ aurora stays →

Geomagnetic field now unsettled to active

Field unsettled to active; magnetosphere near its usual size.

Schematic of Earth's magnetosphere now Earth with the dayside magnetopause drawn at the estimated standoff distance of 10.4 Earth radii, a schematic bow shock, field lines, the geostationary orbit and the current Bz direction. ← Sun · Solar wind 532 km/s, 3.67 p/cm³ Bz -1.3 nT southward 10.4 RE Magnetopause Bow shock(schematic) GOES orbit, 6.6 RE magnetotail → Schematic, not to scale except standoff distance (and the GOES ring). Original drawing, CC0.
Live schematic, redrawn at each hourly update (Sat Oct 31, 8:58 PM ET). The dayside boundary is drawn at the Shue et al. (1998) standoff distance; everything else is schematic. Original drawing, CC0.
Kp (latest 3 h)3.67: below storm level
interval from Sat Oct 31, 5:00 PM ET
Dst-32 nT: weak storm level (-30 to -50 nT)
Sat Oct 31, 7:00 PM ET
Solar wind532 km/s, 3.67 p/cm³
Sat Oct 31, 8:53 PM ET
IMF Bz / Bt-1.3 nT (southward) / 8.4 nT
Sat Oct 31, 8:52 PM ET
Magnetopause10.4 Earth radii (dynamic pressure 1.74 nPa)
GOES-19 Hp49.3 nT (6-h low 31.9 nT)
No sign of a magnetopause crossing in the last 6 h
Sat Oct 31, 8:56 PM ET

Data: NOAA SWPC planetary K-index; Kyoto WDC realtime (quicklook) Dst, via NOAA SWPC (provisional); NOAA SWPC real-time solar wind (spacecraft: ACE; 10-minute means); NOAA SWPC GOES magnetometer. NOAA data are U.S. government works in the public domain.

Solar Cycle 25 progression (NOAA SWPC / WDC-SILSO): smoothed sunspot peak so far is 160.9 (2024-10), compared with Cycle 24's peak of 116.4 (2014-04). Latest monthly sunspot number: 60.3 (2026-09, preliminary). Related: Aurora Tonight & 28 State/Region Guides · Free Embeddable Space Weather Widget · Geomagnetic Shield Model · Storm Log.

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