Atmospheric electricity
Atmospheric electricity refers to the study of electric charges, fields, currents, and conductivities in Earth's atmosphere, arising from ionization processes and charge separation in clouds, which form a global electric circuit linking the planet's surface to the ionosphere.[1] The lower atmosphere functions as a weakly conducting medium primarily due to the presence of positive and negative ions generated by cosmic rays, radioactive decay in soil and air, and other natural sources, with small ion densities near the surface averaging about 600 positive and 500 negative ions per cubic centimeter.[1] In fair-weather conditions, this results in a downward-directed electric field of approximately 130 V/m near the ground, decreasing with altitude to 0.1–1 mV/m at around 70 km, accompanied by a conduction current density of 2.3 pA/m² over continents and 3.3 pA/m² over oceans, and surface conductivity of about 2.5 × 10⁻¹⁴ S/m.[1] The global electric circuit maintains a total current of roughly 1800 A and a potential difference of 275 ± 50 kV between the Earth and ionosphere, primarily powered by charge separation in thunderstorms that act as generators.[1] During disturbed weather, thunderstorms—occurring about 50,000 times daily worldwide, with around 2000 active at any given time—build intense electric fields up to 150 kV/m within clouds, sustaining total charges of approximately 1000 coulombs per storm.[1] These conditions lead to lightning flashes, which are electrical breakdowns in charged clouds, predominantly intracloud (IC) types but including cloud-to-ground (CG) discharges; globally, lightning produces about 45 flashes per second, or 1.4 billion annually, with peak currents of 20–30 kA and charge transfers of around 15 C per flash.[2][1] Lightning activity peaks between 16–17 local time and is concentrated over land masses between 60°S and 60°N latitudes, influencing atmospheric conductivity, electromagnetic radiation, and related phenomena such as transient luminous events.[2] Observations from networks like the Lightning Imaging Sensor confirm that over 90% of flashes occur over continents, with intracloud discharges often initiating in negative charge centers via strong breakdown pulses lasting 50–80 μs.[2]Fundamentals
Basic Principles
Atmospheric electricity is the study of electrical charges, currents, and fields within Earth's neutral atmosphere, encompassing phenomena driven by natural ionization and charge separation processes.[3] Electrostatic interactions in the atmosphere follow Coulomb's law, which governs the force between charged particles over atmospheric scales, given byF = k \frac{q_1 q_2}{r^2},
where k = \frac{1}{4\pi \epsilon} is the Coulomb constant adjusted for the permittivity \epsilon of air (approximately that of free space, \epsilon_0, since air's relative permittivity is near 1).[4] The primary charge carriers in the atmosphere are ions, formed mainly through ionization by galactic cosmic rays interacting with air molecules, producing secondary electrons and ions at rates of about 10–20 ion pairs per cubic centimeter per second near the surface.[5] These ions exhibit mobility, typically around 1 cm/s in a 100 V/m field for small ions, enabling weak conduction despite the atmosphere's overall insulating nature.[4] In fair weather conditions, a vertical electric field exists near the Earth's surface, directed downward with the Earth negatively charged relative to the ionosphere, such that positive ions drift downward while negative ions move upward to sustain the conduction current. Typical magnitudes range from 100 to 300 V/m, decreasing with altitude until negligible above about 50 km.[6][4] Atmospheric electrical conductivity exhibits a gradient, increasing with altitude from low values near the surface (around $10^{-14} S/m) to higher levels in the ionosphere due to greater ionization and reduced ion attachment to aerosols. This conductivity is approximated by
\sigma \approx e (n_+ \mu_+ + n_- \mu_-),
where e is the elementary charge, n_\pm are the densities of positive and negative ions, and \mu_\pm are their respective mobilities.[4][7]