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I am looking for an individual that is proficient in website design and coding that would be willing to assist in bringing SolarHam up to the latest standards to display real time space weather data. If interested, please E-Mail me at kevin@solarcycle24.com. Thank You.

Space Weather for July 2, 2026 UTC Time  
Indices:
(7/2 @ 00:35 UTC)
SFI
201
2
SSN
146
7
AREA
2310
370

HMI Intensity
Latest | Movie | HARP

HMI Magnetogram
Latest | Movie

Coronal Holes
Analysis | Movie

AIA 131 (Latest)
Movie

SUVI 304 (Latest)
Movies
Imagery: SDO | AIA | GOES | GONG | STEREO | CORONAGRAPH
Video: SDO | GSFC | SUVI | SOHO | STEREO | Helioviewer | YouTube
     

3 Day Geomagnetic Forecast
July 2
July 3
July 4
2-3 (G0)
5-6 (G2)
5-6 (G2)

Max Kp

M-Lat   10%
H-Lat   20%
M-Lat   20%
H-Lat   45%
M-Lat   20%
H-Lat   20%

Probabilities

Latest SWPC Forecast (@ 00:30 + 12:30 UTC)

Current Moon Phase:
96% Illumination
Waning Gibbous

Noteworthy Flare Events (Past 72h)

M4.2
AR 4479
7/2/26 @ 01:56 UTC
M8.5
AR 4478
7/1/26 @ 23:09 UTC
M3.5
AR 4479
7/1/26 @ 19:43 UTC
M2.6
AR 4479
7/1/26 @ 14:55 UTC
M2.5
AR 4479
7/1/26 @ 08:17 UTC
X1.1
AR 4479
6/30/26 @ 20:50 UTC
Type II RE   (1496 km/s)   IV    DIM
10cm Radio Burst   (9m, 409 sfu)
M5.8
AR 4475
6/30/26 @ 12:57 UTC

   


Visible Sunspot Regions

   
AR 4480
BG
S16W43
Growing
AR 4479
BGD
N17W38
Stable
AR 4478
BGD
S05W20
Stable

Updated @ 13:30 UTC (July 2)

CME Tracking

1 Event(s) Logged

Cactus  |  SEEDS (GMU)
CCOR-1 Realtime RD

Farside Watch

Updated @ 13:20 UTC (July 2)
Latest Image  |  JSOC  |  STEREO

AIA Composite

Filaments + Coronal Holes

Latest AIA Composite

Solar Oribiter PHI Continuum (ESA)

Latest Available

STIX Light Curves | More Imagery

           

Real Time Solar Wind  |  Expand Data  | SOLAR-1

Updated every minute.


X-Rays

Current

Global D-LAYER Absorption
Current Solar Flare Threat
C-Flare: 90%
M-Flare: 70%
X-Flare: 20%
Proton: 20%

Geomagnetic Field and Aurora
Past 24 Hours
Unsettled

Auroral Oval Forecast | South Pole
Kp-Index | A-Indices | Magnetometers

Latest Space Weather News
Moderate (G2) Storm Watch Issued
July 1, 2026 @ 13:10 UTC
A moderate (G2) geomagnetic storm watch has been issued by NOAA/SWPC beginning July 3rd. A coronal mass ejection (CME) that left the Sun on Tuesday following an X1.1 solar flare around AR 4479 is predicted to sweep past Earth. More updates in the days ahead.

X-Flare, Partial Halo CME
June 30, 2026 @ 21:20 UTC (UPDATED)
Earth facing sunspot region 4479 just erupted with an X1.1 solar flare at 20:50 UTC (June 30). The event is associated with a type II radio emission with an estimated velocity of 1496 km/s, along with a 10cm Radio Burst (TenFlare) measuring 409 solar flux units (sfu) and lasting 9 minutes. Coronal dimming is now evident meaning the chances for an Earth directed coronal mass ejection (CME) will be at an increased level. More details to follow.

CME Update: A partial halo CME is associated with the X1.1 solar flare around AR 4479 on Tuesday. The main bulk of plasma is heading to the north, however with a partial halo signature present, an Earth impact is expected by July 3rd according to a new model released by NASA. I would expect a minor (G1) geomagnetic storm watch to be put in place with a chance for moderate (G2) storming as well. More updates to follow once an updated CME tracking model and forecast is released by NOAA/SWPC.

M5.8 Solar Flare
June 30, 2026 @ 13:30 UTC
A solar flare measuring M5.8 was observed around AR 4475 peaking at 12:57 UTC (June 30). So far it does not appear to be the source of a noteworthy coronal mass ejection (CME).

Incoming CME Detected
June 30, 2026 @ 11:50 UTC (UPDATED)
The edge of a slow moving CME observed leaving the Sun on June 26th has finally been detected. A passage past our planet should be expected within the next hour or so. The solar wind speed only increased to around 440 km/s, although there was a noticeable increase in plasma density and strength (Bt). More to follow whenever necessary.

UPDATE: Magnetometers are showing an impact to Earth's geomagnetic field at 11:53 UTC (June 30). Although not a strong impact, we will wait to see what happens, especially with the Bz component of the interplanetary magnetic field (IMF).

Space Weather Update
June 29, 2026 @ 12:40 UTC
Below is an updated look at the two big sunspot regions facing Earth on Monday. Of the two, AR 4479 appears to be more magnetically complex and has been the main source of minor C-Flares so far today. There will remain a chance for a moderate M-Flare during the next 24 hours.

Speaking of M-Flares, the ESA solar orbiter did detect an M4 flare off the farside of the Sun today and the source may have been another large sunspot forming that is visible in their latest imagery.

A minor (G1) geomagnetic storm watch is now in effect for the next 24 hours due to the expected arrival of a slow moving CME that left the Sun on June 26th. More updates will be provided whenever necessary.

CME Alert
June 27, 2026 @ 03:10 UTC (UPDATED)
This event is a little sneaky, however a slow moving coronal mass ejection (CME) was observed leaving the Sun following an event beginning around 20:15 UTC (June 26). At first it would seem that the eruption originated from either the farside of the Sun or the southern pole region, however STEREO-Ahead imagery shows it to be more of an Earth facing event. Coronal dimming is evident using the Solar Demon website in the vicinity of AR 4475 in the southern hemisphere. While the majority of plasma is heading south of the Sun-Earth line, the northern edge may be Earth directed. If so, a passage may be possible within 72-96 hours due to the slow moving nature of this event. More details to follow whenever necessary.

UPDATE: As per the latest NOAA/SWPC update, the slow moving CME is expected to pass mostly south of the Sun-Earth line with a glancing blow possible by June 30th. More updates in the days ahead whenever necessary.

Space Weather Update
June 26, 2026 @ 12:55 UTC
Below is an updated look at AR 4478 on Friday as seen by SDO/HMI. The sunspot cluster only manged low to mid level C-Flares so far today, but will remain an ongoing threat for an M-Class solar flare (50%). Elsewhere, AR 4475 located near center disk chipped in with a few minor C-Flares as well. Overall, there is about a 10% chance for a strong X-Class flare according to the latest NOAA/SWPC update.


Site Information

SolarHam.com launched on March 15, 2006 with the purpose of providing real time Space Weather news and data from various sources, all in one location for easy navigation. The site was created and is still maintained solely by amateur (HAM) radio station Kevin VE3EN.

Data Sources

This website relays data and imagery from the following sources.

- NOAA Space Weather Prediction Center (SWPC)
- Solar Dynamics Observatory (SDO)
- Atmospheric Imaging Assembly (AIA)
- Solar Terrestrial Relations Observatory (STEREO)
- Deep Space Climate Observatory (DSCOVR)
- Large Angle and Spectrometric Coronagraph Experiment (LASCO)
- Solar and Heliospheric Observatory (SOHO)
- Lockheed Martin Solar & Astrophysics Laboratory (LMSAL)
- Global Oscillation Network Group (GONG)
- Space Weather Canada
- Australia Space Weather Services (SWS)

Contact Information

Any comments or questions regarding this website can be sent via E-Mail by clicking HERE.

Now go work some DX!