Table of Contents
Fetching ...

Terrestrial space weather protection through human-produced mass-loading

B. M. Walsh, D. T. Welling, Z. Huang

TL;DR

The paper addresses the growing risk of space weather by proposing an active defense—artificially mass-loading Earth's dayside magnetopause to suppress magnetic reconnection and energy transfer during solar wind disturbances. It employs global MHD simulations, specifically the Space Weather Modeling Framework, to test a six-spacecraft GEO constellation releasing mass-loading material that photoionizes and drifts to the magnetopause, showing substantial reductions in storm indicators (AE, CPCP, and dB/dt) for the 2024 Gannon storm. The results indicate a potential 50% or greater reduction in major geomagnetic storm intensity with near-future capabilities, requiring about 436 metric tons of payload deployed over several launches, and are discussed in the context of materials science, launch logistics, and international collaboration. This work introduces a novel defense paradigm, StormWall, complementing predictive space weather systems and offering a path toward mitigating risks to power grids, satellites, and human activities in space and on Earth.

Abstract

While humans become more reliant on Earth's space environment, the potential for significant harm from severe space weather continues to grow. As structures from the sun reach Earth's magnetosphere and space environment, they deposit energy that fuels geomagnetic storms. Currently, space weather researchers work to predict the timing and intensity of space weather events, often providing warnings of several days prior to the initiation of a strong geomagnetic storm. Here a new paradigm is presented where, rather than prediction, active steps are taken to mitigate the impact of solar wind structures through temporarily modifying Earth's magnetosphere. Global magnetohydrodynamic simulations are used to demonstrate that artificial mass-loading Earth's dayside magnetosphere can fortify Earth's space environment against strong space weather events. The simulations and supporting analysis use realistic mass-loading from model spacecraft at geosynchronous orbit to show the validity of the enabling physics as well as technical feasibility with current technology. The results demonstrate that with modern technology, the intensity of a major geomagnetic storm could be actively reduced by 50 percent or more, protecting technology and human life.

Terrestrial space weather protection through human-produced mass-loading

TL;DR

The paper addresses the growing risk of space weather by proposing an active defense—artificially mass-loading Earth's dayside magnetopause to suppress magnetic reconnection and energy transfer during solar wind disturbances. It employs global MHD simulations, specifically the Space Weather Modeling Framework, to test a six-spacecraft GEO constellation releasing mass-loading material that photoionizes and drifts to the magnetopause, showing substantial reductions in storm indicators (AE, CPCP, and dB/dt) for the 2024 Gannon storm. The results indicate a potential 50% or greater reduction in major geomagnetic storm intensity with near-future capabilities, requiring about 436 metric tons of payload deployed over several launches, and are discussed in the context of materials science, launch logistics, and international collaboration. This work introduces a novel defense paradigm, StormWall, complementing predictive space weather systems and offering a path toward mitigating risks to power grids, satellites, and human activities in space and on Earth.

Abstract

While humans become more reliant on Earth's space environment, the potential for significant harm from severe space weather continues to grow. As structures from the sun reach Earth's magnetosphere and space environment, they deposit energy that fuels geomagnetic storms. Currently, space weather researchers work to predict the timing and intensity of space weather events, often providing warnings of several days prior to the initiation of a strong geomagnetic storm. Here a new paradigm is presented where, rather than prediction, active steps are taken to mitigate the impact of solar wind structures through temporarily modifying Earth's magnetosphere. Global magnetohydrodynamic simulations are used to demonstrate that artificial mass-loading Earth's dayside magnetosphere can fortify Earth's space environment against strong space weather events. The simulations and supporting analysis use realistic mass-loading from model spacecraft at geosynchronous orbit to show the validity of the enabling physics as well as technical feasibility with current technology. The results demonstrate that with modern technology, the intensity of a major geomagnetic storm could be actively reduced by 50 percent or more, protecting technology and human life.
Paper Structure (9 sections, 4 figures)

This paper contains 9 sections, 4 figures.

Figures (4)

  • Figure 1: Schematic diagram of mass-loading concept. Spacecraft in geosynchronous orbit release material that drifts to the dayside magnetopause. Geometry shows a slice in Earth's equatorialk plane.
  • Figure 2: Time-evolution of mass-loading process. Panels present simulated mass density in ecliptic plane shortly after mass-loading is initiated at the six spacecraft (panel (a)) and then at 40 minute intervals ((b) to (c)). X and Y axis are geocentric solar magnetospheric (GSM) coordinates in units of Earth radii.
  • Figure 3: Quantified impact of artificial mass-loading at the global level. Two measures of the intensity of geomagnetic storms are extracted from the model and presented, AE Index (a) and cross polar cap potential (b). The panels show the state of Earth's space-environment with and without mass-loading. The orange line shows the time window in which mass-loading is occurring (14:00 UT on 10 May 2024 to 4:00 UT on 11 May 2024). Mass-loading significantly reduces the impact of the CME on Earth's space environment through both measures of geomagnetic activity
  • Figure 4: Quantified impact of artificial mass-loading at the surface of Earth from the MHD simulation. $dB_{H}/dt$ is a measure of the change in the horizontal component in the magnetic field.