The risks and impacts of space weather: Policy recommendations and initiatives
Introduction
On 1 September 1859 Richard Carrington witnessed a white-light solar flare on the surface of the Sun. This solar storm remains the largest on record in 450 years [1]. The following morning, the aurora borealis was observed as far south as Cuba and Hawaii. The resulting geomagnetic storm silenced telegraph systems around the globe, and in some cases produced electrical currents strong enough to light telegraph paper on fire. Over 150 years later, the effect of a Carrington-level event on today's technology-dependent society would be catastrophic. The increased sophistication of susceptible technologies dramatically raises our vulnerability to space weather events.
Space weather consists of the dynamic conditions on the Sun and in the space environment and their impacts on technological systems. Large solar storms produce coronal mass ejections (CMEs) that interact with the Earth's atmosphere to create geomagnetic storms [2]. Over several hours or days, these geomagnetic storms can induce powerful electric currents in the atmosphere and the ground that can surge through natural rock and man-made structures such as power lines and pipelines [2]. These extra electrical currents are particularly dangerous to power grids, by potentially causing transformers on high-voltage transmission lines to overheat and burn out.
Powerful electrical currents can also cause corrosion damage to oil and gas pipelines. According to the Electric Power Research Institute (EPRI), a power transformer can take two months to be replaced if it is in stock, and as long as two years if one must be manufactured [3].
A large geomagnetic storm could result in electrical blackouts or even the complete collapse of power grids . Geomagnetic storms can also cause electric charges in space that affect electronic systems onboard spacecraft, degrade satellite navigation (such as GPS receivers), and disrupt HF radio propagation used in aircraft communications [4]. In December 2006 a solar storm damaged part of the GOES satellite solar x-ray imager, and also caused an unexpectedly severe disruption to the GPS navigation system. The airline industry's dependence on GPS is increasing and a similar space weather event could have potentially disastrous consequences for aviation navigation during takeoffs and landings [5].
A large geomagnetic storm could also threaten the sustainability of the space environment. Significant damage to a satellite during a space weather event could cause complete power failure. The loss of control of the spacecraft would potentially contribute to an increase in space debris. Recent studies have shown that geomagnetic storms can increase atmospheric density as much as 134%, causing a significant increase in atmospheric drag [4]. This increase contributes to orbital decay for objects in low-Earth orbit (LEO) such as the Hubble Space Telescope and the International Space Station, which may require additional orbital boosts to maintain their altitude. However, the increase in atmospheric drag can also reduce the amount of space debris in LEO by shortening the time to de-orbit.
Solar storms produce radiation hazards to humans. Astronauts outside the protection of a shielded spaceship or on the surface of the Moon or a planet may be exposed to high levels of radiation during a solar storm. Airline passengers and crews are also at risk of additional modest radiation exposure. Many airlines now fly faster and more economical routes at higher elevations and at higher latitudes, often over the poles, which can further increase the risk of exposure [5].
In 1989 a solar flare produced a geomagnetic storm that caused the collapse of the transmission system for Canada's Hydro Quebec electricity provider, leaving millions of people without power for more than nine hours. [3]. This space weather event also produced enough energetic particles to have killed an unshielded astronaut on the Moon (wearing only a spacesuit) from acute radiation sickness [6]. The late October and early November solar storms of 2003 caused power outages in Europe and permanently damaged transformers in South Africa [5]. Fig. 1 shows the interplanetary shock wave and CME just as they arrived at Earth at 0600UT on 29 October 2003 and initiated an intense geomagnetic storm.
A future Carrington-level event could cause a large geomagnetic storm that would threaten worldwide energy supplies, air transport, telecommunications and other critical infrastructure [7]. Given the global nature of today's economy, a widespread disaster caused by such a geomagnetic storm would have global implications, even if the immediate damage was contained in one hemisphere. The distribution of food, medication, water and other vital necessities might be disrupted with catastrophic consequences for public health and safety. A massive space weather event today would potentially cost over $2 trillion globally [8].
However, space weather can have a global economic impact even in the absence of a major event. A 2004 study by Dr. Kevin Forbes, Chair of the Department of Business and Economics at the Catholic University of America, concluded that a relationship exists between space weather and the real-time market price in the New York wholesale electricity market [9]. Lloyd's of London published a 2010 risk insight briefing outlining the space weather risk and implications to businesses. The report described a series of space weather events in January of 2005 that cause degradation of HF radio links with trans-polar flights. This interruption of radio communications caused airlines to re-route 26 flights during this period, requiring costly refuelling stops and a reduction in cargo capacity [10].
Section snippets
Current international efforts
The international community recognizes the implications of a catastrophic space weather event. The director of the US Federal Emergency Management Agency (FEMA), W. Craig Fugate, stated: “Addressing such a large-scale disaster in purely national terms is not sufficient and requires international cooperation” [11]. A joint statement following the 1st EU–US Expert Meeting on Critical Infrastructure Protection (CIP) emphasised that the “interconnectivity and interdependence of today's essential
Common international objectives
Many of the objectives and recommendations of these meetings were similar and in this order of priority:
- 1.
More accurate space weather forecast capabilities;
- 2.
Better technologies that are more resistant to the negative effects of space weather;
- 3.
Policy initiatives to mitigate risk to communications, power supply and human life;
- 4.
Greater international collaboration to share research;
- 5.
Better promotion of education and public outreach programs.
As a result, several new policies and programs have been
Recommendations
It is important for the international community to continue to expand space weather programs and initiatives in all the areas of opportunity outlined by recent international meetings. Many improvements have been made with more accurate forecast models, resistant technologies, and policy initiatives to mitigate societal risk. These objectives remain important goals for the space weather community. However, the greatest opportunity for advancement resides in the ability of the space weather
Conclusions
There have been numerous recent advancements in space weather mitigation, particularly in the arena of international efforts to collaborate on research and the development of policies and programs to mitigate risks to society and technology. The global space weather community is under-utilizing social media. It is time to bring space weather and its impacts to the forefront of public awareness through social media resources that already have hundreds of millions of users. Space weather needs to
Acknowledgements
This research was made possible by The Office of the Vice President for Research at the University of Alabama in Huntsville. Fig. 1 of the HAFv2 real-time solar wind forecast of the interplanetary magnetic field was provided courtesy of Exploration Physics International, Inc., Huntsville, AL.
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