Abstract

AbstractIncreasing carbon dioxide causes cooling in the upper atmosphere and a secular decrease in atmospheric density over time. With the use of the Whole Atmospheric Community Climate Model with thermosphere and ionosphere extension (WACCM‐X), neutral thermospheric densities up to 500 km have been modeled under increasing carbon dioxide concentrations. Only carbon dioxide and carbon monoxide concentrations are changed between simulations, and solar activity is held low at F10.7 = 70 throughout. Neutral density decreases through to the year 2100 have been modeled using four carbon dioxide emission scenarios produced by the Intergovernmental Panel on Climate Change (IPCC). The years 1975 and 2005 have also been simulated, which indicated a historic trend of −5.8% change in neutral density per decade. Decreases in the neutral density relative to the year 2000 have been given for increasing ground‐level carbon dioxide concentrations. WACCM‐X shows there has already been a 17% decrease in neutral densities at 400 km relative to the density in the year 2000. This becomes a 30% reduction at the 50:50 probability threshold of limiting warming to 1.5°C, as set out in the Paris Agreement. A simple orbital propagator has been used to show the impact the decrease in density has on the orbital lifetime of objects traveling through the thermosphere. If the 1.5°C target is met, objects in Low Earth Orbit (LEO) will have orbital lifetimes around 30% longer than comparable objects from the year 2000.

Highlights

  • While there is global warming in the lower atmosphere, the opposite is true in the upper atmosphere where carbon dioxide (CO2) contributes to global cooling (Akmaev & Fomichev, 1998; Roble & Dickinson, 1989)

  • Carbon dioxide and carbon monoxide concentrations are changed between simulations, and solar activity is held low at F10.7 = 70 throughout

  • Density reductions reported throughout the paper have been given relative to the density in the year 2000 to provide a scaling ratio which can be applied to fast, empirical atmospheric models such as NRLMSISE-00

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Summary

Introduction

While there is global warming in the lower atmosphere (below around 15 km altitude), the opposite is true in the upper atmosphere where carbon dioxide (CO2) contributes to global cooling (Akmaev & Fomichev, 1998; Roble & Dickinson, 1989). CO2 molecules gain energy by collisional excitation, notably with atomic oxygen (O), or by absorption of infrared (IR) radiation (Sharma & Roble, 2002). Energy can be lost from excited CO2 via collisions with other atmospheric molecules or via IR radiation emission at a wavelength of 15 μm. Solar activity has a major impact on thermospheric neutral densities, and is often measured in either sunspot number or the F10.7 radio emission index (Hathaway, 2015).

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