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Role Of the Sun and the Middle atmosphere/thermosphere/ionosphere In Climate (ROSMIC): a retrospective and prospective view

  • William Ward
  • , Annika Seppälä
  • , Erdal Yiğit
  • , Takuji Nakamura
  • , Claudia Stolle
  • , Jan Laštovička
  • , Thomas N. Woods
  • , Yoshihiro Tomikawa
  • , Franz Josef Lübken
  • , Stanley C. Solomon
  • , Daniel R. Marsh
  • , Bernd Funke
  • , Duggirala Pallamraju
  • University of New Brunswick
  • University of Otago
  • George Mason University
  • Research Organization of Information and Systems, National Institute of Polar Research
  • Helmholtz Centre Potsdam - German Research Centre for Geosciences
  • Czech Academy of Sciences
  • University of Colorado Boulder
  • Leibniz-Institute of Atmospheric Physics
  • National Center for Atmospheric Research
  • University of Leeds
  • CSIC - Institute of Astrophysics of Andalusia
  • Physical Research Laboratory India

Research output: Contribution to journalReview articlepeer-review

26 Scopus citations

Abstract

While knowledge of the energy inputs from the Sun (as it is the primary energy source) is important for understanding the solar-terrestrial system, of equal importance is the manner in which the terrestrial part of the system organizes itself in a quasi-equilibrium state to accommodate and re-emit this energy. The ROSMIC project (2014–2018 inclusive) was the component of SCOSTEP’s Variability of the Sun and Its Terrestrial Impact (VarSITI) program which supported research into the terrestrial component of this system. The four themes supported under ROSMIC are solar influence on climate, coupling by dynamics, trends in the mesosphere lower thermosphere, and trends and solar influence in the thermosphere. Over the course of the VarSITI program, scientific advances were made in all four themes. This included improvements in understanding (1) the transport of photochemically produced species from the thermosphere into the lower atmosphere; (2) the manner in which waves produced in the lower atmosphere propagate upward and influence the winds, dynamical variability, and transport of constituents in the mesosphere, ionosphere, and thermosphere; (3) the character of the long-term trends in the mesosphere and lower thermosphere; and (4) the trends and structural changes taking place in the thermosphere. This paper reviews the progress made in these four areas over the past 5 years and summarizes the anticipated research directions in these areas in the future. It also provides a physical context of the elements which maintain the structure of the terrestrial component of this system. The effects that changes to the atmosphere (such as those currently occurring as a result of anthropogenic influences) as well as plausible variations in solar activity may have on the solar terrestrial system need to be understood to support and guide future human activities on Earth. [Figure not available: see fulltext.][Figure not available: see fulltext.][Figure not available: see fulltext.]

Original languageEnglish
Article number47
JournalProgress in Earth and Planetary Science
Volume8
Issue number1
DOIs
StatePublished - Dec 2021

Keywords

  • Atmosphere
  • Atmospheric coupling
  • Climate
  • Energetic particles
  • Ionosphere
  • Middle atmosphere
  • Solar irradiance
  • Thermosphere
  • Trends

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