The planetary K-index (Kp) quantifies the magnitude of geomagnetic disturbances caused by solar activity. It ranges from 0 (quiet) to 9 (extreme storm) and is derived from measurements at highβlatitude magnetometer stations worldwide.
Coronal Mass Ejections (CMEs) drive the most intense storms. Their speed (VCME) determines how much kinetic energy reaches Earth, while the southward component of the interplanetary magnetic field (Bz) controls magnetic reconnection efficiency. A strong, sustained southward Bz allows solar wind energy to couple into the magnetosphere, amplifying the Kp response.
Empirical studies have shown that Kp can be approximated by a simple product of CME speed and the effective southward Bz. The following formula captures this relationship:
What is the planetary K-index (Kp)?
How are Kp values determined?
What causes the most intense geomagnetic storms?
How does the southward component of the interplanetary magnetic field affect geomagnetic storms?
What is the relationship between CME speed and geomagnetic storm intensity?
Can Kp values predict solar flares?
How often are Kp index values updated?
Results are for informational purposes only and do not constitute professional advice.
