Long-term geospace climate monitoring

Climate change is characterized by global surface warming associated with the increase of greenhouse gas population since the start of the industrial era. Growing evidence shows that the upper atmosphere is experiencing appreciable cooling over the last several decades. The seminal modeling study by Roble and Dickinson (1989) suggested potential effects of increased greenhouse gases on the ionosphere and thermosphere cooling which appear consistent with some observations. However, several outstanding issues remain regarding the role of CO2, other important contributors, and impacts of the cooling trend in the ionosphere and thermosphere: for example, (1) what is the regional variability of the trends? (2) the very strong ionospheric cooling observed by multiple incoherent scatter radars that does not fit with the prevailing theory based on the argument of anthropogenic greenhouse gas increases, why? (3) what is the effect of secular changes in Earth’s main magnetic field? Is it visible now in the ionospheric data and can it explain some of the regional variability in the observed ionospheric trends? (4) what is the impact of long-term cooling in the thermosphere on operational systems? (5) what are the appropriate strategic plans to ensure the long-term monitoring of the critical space climate?

[1]  B. F. de Haro Barbás,et al.  Review of Long-Term Trends in the Equatorial Ionosphere Due the Geomagnetic Field Secular Variations and Its Relevance to Space Weather , 2021, Atmosphere.

[2]  V. Harvey,et al.  A High‐Resolution Whole‐Atmosphere Model With Resolved Gravity Waves and Specified Large‐Scale Dynamics in the Troposphere and Stratosphere , 2021, Journal of Geophysical Research: Atmospheres.

[3]  H. Lewis,et al.  Future Decreases in Thermospheric Neutral Density in Low Earth Orbit due to Carbon Dioxide Emissions , 2021, Journal of Geophysical Research: Atmospheres.

[4]  S. Solomon,et al.  Climate Changes in the Upper Atmosphere: Contributions by the Changing Greenhouse Gas Concentrations and Earth's Magnetic Field From the 1960s to 2010s , 2021, Journal of Geophysical Research: Space Physics.

[5]  Huixin Liu,et al.  Geomagnetic Activity Effects on CO2‐Driven Trend in the Thermosphere and Ionosphere: Ideal Model Experiments With GAIA , 2021, Journal of Geophysical Research: Space Physics.

[6]  I. Cnossen Analysis and Attribution of Climate Change in the Upper Atmosphere From 1950 to 2015 Simulated by WACCM‐X , 2020, Journal of Geophysical Research: Space Physics.

[7]  S. Vadas,et al.  Explicit Global Simulation of Gravity Waves in the Thermosphere , 2020, Journal of Geophysical Research: Space Physics.

[8]  P. Alken,et al.  Evolution of the Geomagnetic Daily Variation at Tatuoca, Brazil, From 1957 to 2019: A Transition From Sq to EEJ , 2020, Journal of Geophysical Research: Space Physics.

[9]  C. Finlay,et al.  Recent north magnetic pole acceleration towards Siberia caused by flux lobe elongation , 2020, Nature Geoscience.

[10]  W. Wan,et al.  Long‐Term Trend of Topside Ionospheric Electron Density Derived From DMSP Data During 1995–2017 , 2019, Journal of Geophysical Research: Space Physics.

[11]  D. Kerridge Objectives of Geomagnetic and Aeronomy Studies , 2019, Geomagnetism, Aeronomy and Space Weather.

[12]  B. T. Marshall,et al.  Thermosphere climate indexes: Percentile ranges and adjectival descriptors , 2018, Journal of Atmospheric and Solar-Terrestrial Physics.

[13]  Martin G. Mlynczak,et al.  On Long‐Term SABER CO2 Trends and Effects Due to Nonuniform Space and Time Sampling , 2018, Journal of Geophysical Research: Space Physics.

[14]  D. Marsh,et al.  Whole Atmosphere Simulation of Anthropogenic Climate Change , 2018 .

[15]  W. Wan,et al.  Ionospheric Trend Over Wuhan During 1947–2017: Comparison Between Simulation and Observation , 2018 .

[16]  J. Laštovička A review of recent progress in trends in the upper atmosphere , 2017 .

[17]  Erdal Yiğit,et al.  Earth’s magnetic field effect on MUF calculation and consequences for hmF2 trend estimates , 2017 .

[18]  Dong L. Wu,et al.  Variations of global gravity waves derived from 14 years of SABER temperature observations , 2017 .

[19]  M. Nicolls,et al.  Ionospheric ion temperature climate and upper atmospheric long‐term cooling , 2016 .

[20]  L. Perrone,et al.  Geomagnetic control of the midlatitude daytime foF1 and foF2 long‐term variations: Physical interpretation using European observations , 2016 .

[21]  R. Garcia,et al.  Increasing carbon dioxide concentration in the upper atmosphere observed by SABER , 2015 .

[22]  J. Emmert Altitude and solar activity dependence of 1967–2005 thermospheric density trends derived from orbital drag , 2015 .

[23]  J. Laštovička Comment on “Long‐term trends in thermospheric neutral temperatures and density above Millstone Hill” by W. L. Oliver et al. , 2015 .

[24]  C. Jacobi Long-term trends and decadal variability of upper mesosphere/lower thermosphere gravity waves at midlatitudes , 2014 .

[25]  S. Nozawa,et al.  Upper atmosphere cooling over the past 33 years , 2014 .

[26]  L. Goncharenko,et al.  Is thermospheric global cooling caused by gravity waves? , 2013 .

[27]  John M. Holt,et al.  Long‐term ionospheric cooling: Dependency on local time, season, solar activity, and geomagnetic activity , 2013 .

[28]  N. Olsen,et al.  Stochastic modeling of the Earth's magnetic field: Inversion for covariances over the observatory era , 2013 .

[29]  A. Richmond,et al.  Changes in the Earth's magnetic field over the past century: Effects on the ionosphere‐thermosphere system and solar quiet (Sq) magnetic variation , 2013 .

[30]  M. Rapp,et al.  Trends of mesospheric gravity waves at northern middle latitudes during summer , 2011 .

[31]  Hugh G. Lewis,et al.  Effect of thermospheric contraction on remediation of the near‐Earth space debris environment , 2011 .

[32]  Shunrong Zhang,et al.  Millstone Hill ISR observations of upper atmospheric long-term changes: Height dependency , 2011 .

[33]  J. Laštovička,et al.  Progress in observations and simulations of global change in the upper atmosphere , 2011 .

[34]  J. Picone,et al.  Statistical uncertainty of 1967–2005 thermospheric density trends derived from orbital drag , 2011 .

[35]  Remko Scharroo,et al.  A global positioning system–based climatology for the total electron content in the ionosphere , 2010 .

[36]  W. Wan,et al.  Modeling the effects of secular variation of geomagnetic field orientation on the ionospheric long term trend over the past century , 2008 .

[37]  J. M. Picone,et al.  Thermospheric global average density trends, 1967–2007, derived from orbits of 5000 near‐Earth objects , 2008 .

[38]  Tuija I. Pulkkinen,et al.  Space Weather: Terrestrial Perspective , 2007 .

[39]  G. Beig,et al.  Global Change in the Upper Atmosphere , 2006, Science.

[40]  J. Lean,et al.  Global change in the thermosphere: Compelling evidence of a secular decrease in density , 2004 .

[41]  Raymond G. Roble,et al.  How will changes in carbon dioxide and methane modify the mean structure of the mesosphere and thermosphere , 1989 .