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Large Solar Flare (X-class)

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Large Solar Flare (X-class)

When the Sun has a tantrum and everyone on Earth pays attention/Events & Phenomena

An X-class solar flare is the most powerful category of solar explosion, releasing energy equivalent to billions of hydrogen bombs in minutes. The plasma eruption heats coronal material to tens of millions of kelvins and accelerates charged particles to nearly the speed of light. If the associated coronal mass ejection hits Earth, it can disrupt satellite communications, damage power grids, and produce stunning auroras visible at low latitudes. The 1859 Carrington Event, an estimated X45+ flare, caused telegraph lines to spark and catch fire.

Measurements

Total energy released10 septillion J
2.4 quintillionTNT sticks
100 sextillionthsSupernova blasts

Large X-class flare; equivalent to ~10 billion megatons of TNT

CME ejection speed2 million m/s
909,091Olympic swimmers
260Orbiting satellites
250,000Rolled bowling balls

Fastest CMEs exceed 2,000 km/s; typical fast ones ~1,000 km/s

Flare plasma temperature20 million K
68,458Office thermostats
64,175Human fevers
58,140Car dashboards in summer

~20 million K at the reconnection site; hotter than the Sun's core

Flare loop height100 million m
5.2 billionPenny diameters
7.2 hundredthsSun diameters

~100,000 km; magnetic loops taller than Jupiter's diameter

Peak radiated power10 sextillion W
20 sextillionLED nightlights
2.7 quintillionLawnmowers
33.3 quintillionStair climbers

Peak X-ray luminosity during the flare impulsive phase

Flare duration1,800 s
1.9 millionthsGenerations
60 millionLightning discharges

Impulsive phase lasts minutes; decay phase can last hours

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