Solar X-rays: Geomagnetic Field:

From n3kl.org

Solar X-ray status monitor

Geomagnetic Field status monitor

Normal: Solar X-ray flux is quiet (< 1.00e-6 W/m^2)	Quiet: the Geomagnetic Field is quiet (Kp < 4)
Active: Solar X-ray flux is active (>= 1.00e-6 W/m^2)	Active: the Geomagnetic Field has been unsettled (Kp=4)
M Class Flare: An M Class flare has occurred (X-ray flux >= 1.00e-5 W/m^2)	Storm: A Geomagnetic Storm has occurred (Kp>4)
X Class Flare: An X Class flare has occurred (X-ray flux >= 1.00e-4 W/m^2)
Mega Flare: An unprecedented X-ray event has occurred (X-ray flux >= 1.00e-3 W/m^2) The designation "Mega Flare" was chosen by Kevin Loch when the status monitor was created on March 4, 1999. There is no "official" designation for flares in this range.

Real Time Images of the Sun

SOHO EIT 304

SOHO EIT 284

Mauna Loa Solar Image

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

Solar Cycle Progression Solar Cycle chart updated using the latest ISES predictions.

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 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 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

Southern Hemi Auroral 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.

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