Propagation Page (page reloads every 5 minutes)
| Geomagnetic Field | Solar X-ray status | |
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iSWA - Integrated Spaceweather Analysis system Current
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24 hours |
Current |
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Geomagnetic Storms |
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Solar Radiation Storms |
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Radio Blackouts |
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ACE Magnetic Field data 7d 3d 24h 6h 2h
Combined data F:136 A:6 K:2 SSN:114 2012-05-18 17:45:00Z
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Divide the number shown here by 100 to calculate the number of MHz that MUF is up or down compared to the last 60 days at the current time. Raw data can be found here for Wallops Island ionosonde. |
Recent SF, A and SSN
F5LEN solar forecast
X-ray plot (1min)
X-ray plot (5min)
Kp Index Plot
Space Weather Now (NWS)
eSSN (24hrs)
SSN smoothed
Space Weather
Space Weather Canada Penticton Solar Flux
Sun Nearside & FARSIDE images: 1 | 2 | 3 (SOHO/MDI, SOHO/SWAN, SOHO/SWAN)
Latest SOHO images
Forecast based on current data*
Active Region Monitor
STORM Ionospheric correction factors
Latest POES Aurora Data
Coronal Mass Ejection movie*
WARNINGS currently in effect
Current D layer Absorption
Real Time MUF
VRML (3D) view of Coronal fields* (VRML viewer required)
Mount Wilson Sunspot Count note this is drawn "backwards"
DXRobot (GoodDX)
The Lookers Blog
DXAnywhere Figures*
*Broadband required * Huge memory resources needed for Flash
Cycle 24 predictions: (I) (II) (III)
Did you know: The Sun is a big ball of plasma mostly made up of hydrogen, helium, oxygen, carbon, nitrogen, and neon.
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Nancay Not Real Time |
Nancay Not Real Time |
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These real-time images follow around the above graphic, except that: EIT 284Å is an additional image VHF/UHF images are not taken in real-time References: http://www.edpsciences.org/articles/aa/pdf/2001/42/aah2629.pdf?access=ok |
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Meudon Hα 6563Å |
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| GOES-15 X-ray Flux (5 minutes) | GOES-15 X-ray Flux (1 minute) |
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| GOES-13 & 15 Electron Flux (5 minutes) | GOES-13 Proton Flux (5 minutes) |
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| K Index (3 hours) | Combined (1 minute) |
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| GOES-13 and 15 Magnetometers (1 minute) | Boulder Magnetometer (1 minute) |
Click
on image for details 
POES data and OVATION Aurora Prediction
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| North Pole | South Pole |
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| NA | EU | AS |
From this vantage point Solar wind data can be detected about 45 to 60 minutes before reaching Earth.
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| Front Side | Far Side |
Key to solar history above
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| SoHO (straight-on view) [195Å] (SDO 193Å) | STEREO-B - to the East (looking around back of Sun) |
Browse
Latest Images  |
B: Separation angle with Earth 117.57° = 9.14 days = 219.46 hours A: Separation angle with Earth 114.96° = 8.94 days = 214.59 hours STEREO - receiving the data. Between April and June 2015 the datalink won't reach the Earth. Why? The angle B-Earth is gradually increasing, at the rate of about 0.3 degrees per month. When this gets too large, the signals will have to graze the Sun to reach Earth. If the satellites survive ecllipse and the increasing solar activity, then they will remain extraordinary solar sentinals. Antenna pointing is restricted, so signal recovery may be marginal. -90°/+90°
coverage was achieved in February 2011. With SoHO that should ensure
360° coverage until 2019 - or until instrument failure or
de-funding occurs.
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| SDO Magnetogram | SDO MDI - Sunspot indications |
Cycle 23: In the sun's northern hemisphere, all spots are S-N. In the southern hemisphere, all spots are N-S.
Cycle 24: Northern sunspots will become N-S while southern sunspots will become S-N.
This reversal occurs each time one cycle gives way to the next. It is called Hale's Law.
Data on
this page courtesy of: esa/SOHO,
NASA, Solar Terrestrial Dispatch,
Stanford University (Solar Oscillations Investigation group),
spaceweather.com, NW Research Associates, NOAA/SWPC (Space Weather
Prediction Center),
Lockheed Martin (Solar & Astrophysics Laboratory)
Raben Systems, Inc., n2yo.com, Deep Space Network and the hundreds of
ground
support team
personnel involved in these projects.