Space Weather
Solar X-rays:
Status
Geomagnetic Field:
Status
Solar Flares, Sun spots There's something on the wing  Space Weather Observations, Alerts, and Forecast

 3-day Solar-Geophysical Forecast
  3-day Report of Solar and Geophysical Activity

Issued May 17 22:00 UTC

Solar Activity Forecast:
Solar activity is expected to be at predominantly low levels with a slight chance for M-class activity for all three days of the period (18 - 20 May).

Geophysical Activity Forecast:
The geomagnetic field is expected to be mostly quiet during the first half of day 1 (18 May). Around mid to late on day 1, a shock arrival is expected from the partial halo CME associated with the 17 May M5 flare. Active to minor storm conditions are expected. Early on day 2 (19 May), unsettled to active conditions are expected, returning to quiet to unsettled levels by the end of the day. Quiet to unsettled conditions are expected on day 3 (20 May).




Today’s Space Weather

Updated 2012 May 17 22:16 UTC



Latest GOES Solar X-ray Image, link to large image

Latest GOES Solar X-ray Image Image

SWPC GOES SXI Web Page

See Solar Image References for other solar image sites.

HF Propagation

May 17 2105 UTC

Solar flux: 136 increasing
A Index: 6 decreasing
K Index: 1 no change
Sunspots: 122
Forecast: Disturbed
Conditions
< 10MHz: Normal
10-20MHz: Good
20-30MHz: Good

Solar data from WWV.
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NOAA Scales Activity
Range 1 (minor) to 5 (extreme)
NOAA Scale Past 24 hrs Current
Geomagnetic Storms Highest Geomagnetic Storm level past 24 hrs Current Geomagnetic Storm level
Solar Radiation Storms Highest Radiation Storm level past 24 hrs Current Radiation Storm level
Radio Blackouts Highest Radio Blackout level past 24 hrs Current Radio Blackout level
Updated: 2012 May 17 22:16 UTC
SOHO MDI Sun Spots
Click to enlarge image of SOHO MDI Sun Spots



Real Time Images of the Sun


SOHO EIT 304
Click for time-lapse image of the sun
SOHO EIT 284
SOHO EIT 284 image of the sun
Mauna Loa Solar Image
Latest Mauna Loa image of the Sun

The sun is constantly monitored for sun spots and coronal mass ejections. EIT (Extreme ultraviolet Imaging Telescope) images the solar atmosphere at several wavelengths, and therefore, shows solar material at different temperatures. In the images taken at 304 Angstrom the bright material is at 60,000 to 80,000 degrees Kelvin. In those taken at 171 Angstrom, at 1 million degrees. 195 Angstrom images correspond to about 1.5 million Kelvin, 284 Angstrom to 2 million degrees. The hotter the temperature, the higher you look in the solar atmosphere.

Real Time Solar X-ray and Solar Wind

CURRENT TIME
(based on your computer's time):   UTC..
Local
Solar Cycle Progression
Graph showing current solar cycle progression (click to enlarge)
Solar Cycle chart updated using the latest ISES predictions.
Graph showing Real-Time Solar Wind
Real-Time Solar Wind data broadcast from NASA's ACE satellite.

The Solar Cycle is observed by counting the frequency and placement of sunspots visible on the Sun. Solar minimum occurred in December, 2008. Solar maximum is expected to occur in May, 2013.


Solar X-ray Flux
Graph showing Real-Time Solar X-ray Flux (click to enlarge)
This plot shows 3-days of 5-minute solar x-ray flux values measured on the SWPC primary and secondary GOES satellites.
Satellite Environment Plot
Graph showing Real-Time Satellite Environment Plot (click to enlarge)
The Satellite Environment Plot combines satellite and ground-based data to provide an overview of the current geosynchronous satellite environment.


Auroral Activity Extrapolated from NOAA POES


Northern Hemi Auroral Map
Current Northern hemispheric power input map
Southern Hemi Auroral Map
Current Southern hemispheric power input map

Instruments on board the NOAA Polar-orbiting Operational Environmental Satellite (POES) continually monitor the power flux carried by the protons and electrons that produce aurora in the atmosphere. SWPC has developed a technique that uses the power flux observations obtained during a single pass of the satellite over a polar region (which takes about 25 minutes) to estimate the total power deposited in an entire polar region by these auroral particles. The power input estimate is converted to an auroral activity index that ranges from 1 to 10.







NASA Image of the Day
NASA Image of the Day
The latest NASA "Image of the Day" image.
  • Composite of a Series of Images Taken From Space Aboard the Space Station

    Thu, 17 May 2012 00:00:00 EDT


    This is a composite of a series of images photographed from a mounted camera on the Earth-orbiting International Space Station, from approximately 240 miles above Earth. Expedition 31 Flight Engineer Don Pettit said of the about photographic techniques used to achieve the images: "My star trail images are made by taking a time exposure of about 10 to 15 minutes. However, with modern digital cameras, 30 seconds is about the longest exposure possible, due to electronic detector noise effectively snowing out the image. To achieve the longer exposures I do what many amateur astronomers do. I take multiple 30-second exposures, then ‘stack’ them using imaging software, thus producing the longer exposure." A total of 18 images photographed by the astronaut-monitored stationary camera were combined to create this composite. Image Credit: NASA





A Closer Look at the Sun in Real time


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