Abstract
This article proposes a pricing model for space weather derivatives with payout depending on solar activity. By measuring the disturbance of the Earth’s magnetosphere, it is possible to price space weather derivatives which trigger a payoff if a certain level of energization is reached. Since energetic particles emitted by the Sun are a non-tradeable quantity, unique prices of contracts in an incomplete market are obtained using inverse transformation sampling as well as the market price of risk. We find a step-wise decline of option prices with increasing barriers of Kp-index values, a dependence of the option prices on the sunspot cycle, as well as reduced sensitivity of longer-dated maturities for higher Kp-index values.
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Notes
X-class flares (R3–R5) have a peak flux of >\(10^{-4}\) W/\({\text(m)}^2\). They are major events that can trigger planet-wide radio blackouts and long-lasting radiation storms, whereas M-class (R1–R2) flares are medium-sized with a peak flux of >\(10^{-5}\) W/\({\text(m)}^2\). They can cause brief radio blackouts that affect Earth’s polar regions. Minor radiation storms are sometimes followed by an M-class flare.
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Lemmerer, B., Unger, S. Modeling and pricing of space weather derivatives. Risk Manag 21, 265–291 (2019). https://doi.org/10.1057/s41283-019-00052-0
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DOI: https://doi.org/10.1057/s41283-019-00052-0