A recent flurry of eruptions on the sun did more than spark pretty auroras around the poles. NASA-funded researchers say the solar storms of March 8th through 10th dumped enough energy in Earths upper atmosphere to power every residence in New York City for two years.
This was the biggest dose of heat weve received from a solar storm since 2005, says Martin Mlynczak of NASA Langley Research Center. It was a big event, and shows how solar activity can directly affect our planet.
Mlynczak is the associate principal investigator for the SABER instrument onboard NASAs TIMED satellite. SABER monitors infrared emissions from Earths upper atmosphere, in particular from carbon dioxide (CO2) and nitric oxide (NO), two substances that play a key role in the energy balance of air hundreds of km above our planets surface.
Carbon dioxide and nitric oxide are natural thermostats, explains James Russell of Hampton University, SABERs principal investigator. When the upper atmosphere (or thermosphere) heats up, these molecules try as hard as they can to shed that heat back into space.
Thats what happened on March 8th when a coronal mass ejection (CME) propelled in our direction by an X5-class solar flare hit Earths magnetic field. (On the Richter Scale of Solar Flares, X-class flares are the most powerful kind.) Energetic particles rained down on the upper atmosphere, depositing their energy where they hit. The action produced spectacular auroras around the poles and significant1 upper atmospheric heating all around the globe.
The thermosphere lit up like a Christmas tree, says Russell. It began to glow intensely at infrared wavelengths as the thermostat effect kicked in.
For the three day period, March 8th through 10th, the thermosphere absorbed 26 billion kWh of energy. Infrared radiation from CO2 and NO, the two most efficient coolants in the thermosphere, re-radiated 95% of that total back into space.
In human terms, this is a lot of energy. According to the New York City mayors office, an average NY household consumes just under 4700 kWh annually. This means the geomagnetic storm dumped enough energy into the atmosphere to power every home in the Big Apple for two years.
Unfortunately, theres no practical way to harness this kind of energy, says Mlynczak. Its so diffuse and out of reach high above Earths surface. Plus, the majority of it has been sent back into space by the action of CO2 and NO.
During the heating impulse, the thermosphere puffed up like a marshmallow held over a campfire, temporarily increasing the drag on low-orbiting satellites. This is both good and bad. On the one hand, extra drag helps clear space junk out of Earth orbit. On the other hand, it decreases the lifetime of useful satellites by bringing them closer to the day of re-entry.
The storm is over now, but Russell and Mlynczak expect more to come.
Were just emerging from a deep solar minimum, says Russell. The solar cycle is gaining strength with a maximum expected in 2013.
More sunspots flinging more CMEs toward Earth adds up to more opportunities for SABER to study the heating effect of solar storms.
This is a new frontier in the sun-Earth connection, says Mlynczak, and the data were collecting are unprecedented.
Stay tuned for updates from the top of the atmosphere.
Explore further: Flying through a geomagnetic storm