Models Gone Wild: The Ionosphere Triggers Earthquakes?

The idea that ionospheric disturbances could influence earthquakes is an emerging and speculative concept in geophysics, primarily explored in a recent theoretical model rather than through established empirical evidence.

The idea that ionospheric disturbances could influence earthquakes is an emerging and speculative concept in geophysics, primarily explored in a recent theoretical model rather than through established empirical evidence.

However, this remains a speculative hypothesis rather than an established fact, and the mainstream scientific view continues to treat ionospheric changes primarily as consequences of earthquakes (co-seismic effects) or potential precursors from below-ground processes, not drivers from above.

From Watts Up With That?

By Anthony Watts

From the โ€œanything goes in modeling these daysโ€ department. Hereโ€™s my take on it.

The paper proposes a capacitive coupling model in which a fractured crustal zone supposedly acts as a capacitor, storing charge that interacts with the ionosphere, and reciprocally, solar-flareโ€“enhanced ionospheric charge induces electrostatic pressures in crustal voids sufficient to trigger rupture.

It is certainly an imaginative (and that is being generous) attempt to unify atmospheric electricity and seismology, but the central weakness is that it moves rapidly from correlation to causation without robust empirical validation.

The authors assume, for example, that descending ionospheric charge density can be treated as equal to total electron content (TEC) and that this charge forms an effective space-charge layer capable of inducing megapascal-scale pressures. That assumption alone carries enormous physical uncertainty: TEC is an integrated vertical column measurement over hundreds of kilometers, not a direct proxy for localized lower-ionospheric space charge. Likewise, the model presumes idealized dielectric behavior in fractured crust saturated with supercritical water, with specified permittivity, breakdown voltage, and uniform void connectivity, yet these parameters are not constrained by real-world field measurements at seismogenic depths. In short, the mechanism rests on layered assumptions rather than observational confirmation. It is a lot like climate science.

Moreover, the invocation of the 2024 Noto Peninsula earthquake and coincident solar flare activity as supporting evidence reads more like post hoc pattern matching than statistical demonstration . Solar flares are frequent; earthquakes are frequent; coincidences will occur. A convincing case would require rigorous statistical analysis across many events, controlling for flare magnitude, geomagnetic latitude, background stress state, and tidal forcing. Instead, the pressure estimates (e.g., ~5 ร— 10โถ N/mยฒ for 10 TECU) are presented as comparable to tidal or gravitational stresses , yet no sensitivity analysis is offered to show how stable those results are under more realistic conductivity, charge dissipation, or geometric heterogeneity. The Earthโ€™s crust is not a laboratory capacitor with neatly parallel plates, and electric fields in conductive, fluid-rich rock are likely to dissipate rapidly. IMHO, the paper reads as speculative fiction.


Via Eurekalert:
Could ionospheric disturbances influence earthquakes?

Kyoto, Japan โ€” Researchers at Kyoto University have proposed a new physical model that explores how disturbances in the ionosphere may exert electrostatic forces within the Earthโ€™s crust and potentially contribute to the initiation of large earthquakes under specific conditions.

The study does not aim to predict earthquakes but rather presents a theoretical mechanism describing how ionospheric charge variations โ€” caused by intense solar activity such as solar flares โ€” could interact with pre-existing fragile structures in the Earthโ€™s crust and influence fracture processes.

In the proposed model, fractured zones within the Earthโ€™s crust are assumed to contain high-temperature, high-pressure water, potentially in a supercritical state. These zones behave electrically like capacitors and are capacitively coupled with both the ground surface and the lower ionosphere, forming a large-scale electrostatic system.

When strong solar activity increases electron density in the ionosphere, a negatively charged layer can form in the lower ionosphere. Through capacitive coupling, this space charge may induce strong electric fields inside nanometer-scale voids within fractured crustal regions. The resulting electrostatic pressure could reach magnitudes comparable to tidal or gravitational stresses known to affect fault stability.

Quantitative estimates in the study suggest that ionospheric disturbances associated with large solar flares โ€” corresponding to increases in total electron content of several tens of TEC units โ€” could generate electrostatic pressures on the order of several megapascals within crustal voids.

Ionospheric anomalies, such as increased electron density, lowered ionospheric altitude, and slowed abnormal propagation of medium-scale traveling ionospheric disturbances, have been repeatedly observed prior to major earthquakes. Traditionally, these phenomena have been interpreted as consequences of stress accumulation within the Earthโ€™s crust.

The new model provides a complementary perspective by proposing a bidirectional interaction: while crustal processes may affect the ionosphere, ionospheric disturbances themselves may also exert feedback forces on the crust. This framework offers a possible physical explanation linking space weather phenomena and seismic processes without invoking direct causation.

The study discusses recent large earthquakes in Japan, including the 2024 Noto Peninsula earthquake, as examples that are temporally consistent with the proposed mechanism. In these cases, intense solar flare activity occurred shortly before the seismic events. The authors emphasize that such temporal coincidence does not establish direct causality but is consistent with a scenario in which ionospheric disturbances act as a contributing factor when the crust is already in a critical state.

By integrating concepts from plasma physics, atmospheric science, and geophysics, the proposed model broadens the conventional view of earthquakes as purely internal Earth processes. The findings suggest that monitoring ionospheric conditions, together with subsurface observations, may help improve scientific understanding of earthquake initiation processes and seismic hazard assessment.

Future research will focus on combining high-resolution GNSS-based ionospheric tomography with space weather data to clarify the conditions under which ionospheric disturbances may exert significant electrostatic influence on the Earthโ€™s crust.

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The paper โ€œPossible Mechanism of Ionospheric Anomalies to Trigger Earthquakes: Electrostatic Coupling Between the Ionosphere and the Crust and the Resulting Electric Forces Acting Within the Crustโ€ appeared on 3 February 2026 in International Journal of Plasma Environmental Science and Technology, with doi: 10.34343/ijpest.2026.20.e01003

https://ijpest.com/Contents/20/1/e01003.html

To study atmosphere, NASA rockets will fly into October eclipse’s shadow

From Phys.org

By Miles Hatfield,ย NASA

This map details the path the Moonโ€™s shadow will take as it crosses the contiguous U.S. during theย annular solar eclipse on Oct. 14, 2023, andย total solar eclipse on April 8, 2024. Credit: NASA/Scientific Visualization Studio/Michala Garrison; eclipse calculations by Ernie Wright

A NASA sounding rocket mission will launch three rockets during the 2023 annular eclipse in October to study how the sudden drop in sunlight affects our upper atmosphere.

On Oct. 14, 2023, viewers of an annularย solarย eclipse in the Americas will experience the sun dimming to 10% its normal brightness, leaving only a bright “ring of fire” of sunlight as the moon eclipses the sun. Those in the vicinity of the White Sands Missile Range in New Mexico, however, might also notice sudden bright streaks across the sky: trails of scientific rockets, hurtling toward the eclipse’s shadow.

A NASA sounding rocket mission will launch three rockets to study how the sudden drop in sunlight affects our upper atmosphere. The mission, known as Atmospheric Perturbations around the Eclipse Path or APEP, is led by Aroh Barjatya, a professor of engineering physics at Embry-Riddle Aeronautical University in Daytona Beach, Florida, where he directs the Space and Atmospheric Instrumentation Lab.

Some 50 miles up and beyond, the air itself becomes electric. Scientists call this atmospheric layer the ionosphere because it is where the UV component of sunlight can pry electrons away from atoms to form a sea of high-flying ions and electrons. The sun’s constant energy keeps these mutually attracted particles separated throughout the day. But as the sun dips below the horizon, many recombine into neutral atoms for the night, only to part ways again at sunrise.

During a solar eclipse, the sunlight vanishes and reappears over a small part of the landscape almost at once. In a flash, ionospheric temperature and density drop, then rise again, sending waves rippling through the ionosphere.

“If you think of the ionosphere as a pond with some gentle ripples on it, the eclipse is like a motorboat that suddenly rips through the water,” Barjatya said. “It creates a wake immediately underneath and behind it, and then the water level momentarily goes up as it rushes back in.”

During theย 2017 total solar eclipseย visible across North America, instruments many hundreds of miles outside the eclipse’s path detected atmospheric changes. So did critical infrastructure like GPS andย communications satellitesย that we rely on every day.

“All satellite communications go through the ionosphere before they reach Earth,” Barjatya said. “As we become more dependent on space-based assets, we need to understand and model all perturbations in the ionosphere.”

To this end, Barjatya designed the APEP mission, choosing the acronym because it is also the name of the serpent deity from ancient Egyptian mythology, nemesis of the sun deity Ra. It was said that Apep pursued Ra and every so often nearly consumed him, resulting in an eclipse.

The APEP team plans to launch three rockets in successionโ€”one about 35 minutes before local peak eclipse, one during peak eclipse, and one 35 minutes after. They will fly just outside the path of annularity, where the moon passes directly in front of the sun. Each rocket will deploy four small scientific instruments that will measure changes in electric and magnetic fields, density, and temperature. If they are successful, these will be the first simultaneous measurements taken from multiple locations in the ionosphere during a solar eclipse.

Barjatya chose sounding rockets to answer the team’s science questions because they can pinpoint and measure specific regions of space with high fidelity. They can also measure changes that happen at different altitudes as the suborbital rocket ascends and falls back to Earth. The APEP rockets will take measurements between 45 and 200 miles (70 to 325 kilometers) above the ground along their trajectory.

“Rockets are the best way to look at the vertical dimension at the smallest possible spatial scales,” said Barjatya. “They can wait to launch at just the right moment and explore the lower altitudes where satellites can’t fly.”

While the in-situ rocket instruments are all being built by Embry-Riddle and Dartmouth College in New Hampshire, a host of ground-based observations will also support the mission. Co-investigators from the Air Force Research Laboratory at Kirtland Air Force Base in Albuquerque, New Mexico, will collect ionospheric density and neutral wind measurements.

Co-investigators from the Massachusetts Institute of Technology’s Haystack Observatory in Westford, Massachusetts, will run their radar to measure ionospheric perturbations farther away from the eclipse path. Finally, a team of students from Embry-Riddle will deploy high-altitude balloons (reaching 100,000 feet) every 20 minutes to measure weather changes as the eclipse passes by. All of these measurements will aid ionosphere modeling efforts led by scientists at the University of Colorado Boulder and Embry-Riddle.

This won’t be the only APEP launch. The APEP rockets launched in New Mexico will be recovered and then relaunched from NASA’s Wallops Flight Facility in Virginia, on April 8, 2024, when a total solar eclipse will cross the U.S. from Texas to Maine. The April launches are farther from the eclipse path than for the October annular eclipse, but will present an opportunity to measure just how widespread the effects of an eclipse are.

After these two eclipses, the next total solar eclipse over the contiguous U.S. is not until 2044, and the next annular eclipse is not until 2046. “We have to make hay while the sun shines โ€ฆ or, I suppose for eclipse science, while it doesn’t,” Barjatya joked. “In all seriousness though, this data set will reveal the widespread effects that eclipses have on the ionosphere at the smallest spatial scales.”

Provided by NASA 


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