# data[].attributes.body
Geomagnetic storms are the result of too many particles enter our geomagnetic field. This causes major problems with satellites and even our electrical grid. KP index is used to measure the strength of the storm, giving us vital time to brace for impact.

# data[].attributes.body
The magnetic field around Earth stretches far into space, at least 37,000 miles. The Bt value represents the strength while the Bz value represents the orientation of incoming magnetic fields.

# data[].attributes.body
Solar wind is a continuous outward stream of particles released from the sun's hot corona. Solar wind is measured by a few of NASA's satellites.

# data[].attributes.body
Solar Flares are short outbursts of energy stored in twisted magnetic fields. Solar Flares are monitored by various GOES satellites.

# data[].attributes.body
Coronal Holes are essentially openings in the sun's surface where tons of hot gases are shot from the sun. Measured by extreme ultraviolet in pictures.

# data[].attributes.body
A CME is an ejection of huge amounts of matter from the sun's corona. CME's are measured and recorded using a coronagraph.

# data[].attributes.body
Sunspots are regions of reduced surface temperature caused by concentrations of magnetic field flux. Sunspots are monitored by region of sun and number of spots.