Global and regional trends in ionospheric total electron content

[1] A statistically significant positive trend of 0.6 ± 0.3 total electron content unit (TECU; 1 TECU = 1016 el m−2) per decade is detected in the 15 year record of daily averaged global total electron content obtained from multiple GPS observations between 1995 and 2010. The trend is extracted using a multiple regression analysis that simultaneously accounts for the comparatively larger global ionospheric responses to solar irradiance variability, solar-modulated annual and semiannual ionospheric oscillations, and geomagnetic activity. Geographical maps of regional trends in total electron content reveal both positive and negative local secular change during the past 15 years, with an overall larger increase in the Northern Hemisphere than in the Southern Hemisphere. Largest regional changes of as much as ±3 TECU per decade occur in the vicinity of 60°W to 60°E longitude and 15°S to 30°N latitude. TEC trend magnitude depends sensitively on the specification of solar EUV irradiance variations in the multiple regression model. The +0.6 TECU per decade trend pertains to equal solar irradiance levels during the 1996 and 2008 solar activity minima. When the specified solar irradiance is 15% lower in 2008 than in 1996, the derived global ionospheric trend increases to 3 TECU per decade. We contend that such a large global trend is implausible and that the associated anomalously low level of EUV irradiance in cycle 2008 minimum, reported in earlier publications, is unlikely to be real.

[1]  Barry E. Schwartz,et al.  Detecting environmental changes and trends , 2002 .

[2]  R. Roble,et al.  Model simulations of global change in the ionosphere , 2008 .

[3]  J. Bremer,et al.  Long-term trends in the ionosphere and upper atmosphere parameters , 2004 .

[4]  Jan Laštovička,et al.  Emerging pattern of global change in the upper atmosphere and ionosphere , 2008 .

[5]  Shunrong Zhang,et al.  Ionospheric climatology and variability from long-term and multiple incoherent scatter radar observations: variability , 2008 .

[6]  J. M. Picone,et al.  Record‐low thermospheric density during the 2008 solar minimum , 2010 .

[7]  H. Rishbeth,et al.  Cooling of the upper atmosphere by enhanced greenhouse gases — modelling of thermospheric and ionospheric effects , 1992 .

[8]  Libo Liu,et al.  Solar activity variations of nighttime ionospheric peak electron density , 2006 .

[9]  F. G. Eparvier,et al.  Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model Developments , 2010 .

[10]  Gary J. Rottman,et al.  Solar EUV Experiment (SEE): Mission overview and first results , 2005 .

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

[12]  S. Solomon,et al.  The effect of carbon dioxide cooling on trends in the F2-layer ionosphere , 2009 .

[13]  A. Garcia-Rigo,et al.  The IGS VTEC maps: a reliable source of ionospheric information since 1998 , 2009 .

[14]  J. Bremer Long-term trends in the ionospheric E and F1 regions , 2008 .

[15]  J. Picone,et al.  Climatology of globally averaged thermospheric mass density , 2010 .

[16]  M. Jarvis Longitudinal variation in E- and F-region ionospheric trends , 2009 .

[17]  P. Field,et al.  Latitude and solar-cycle patterns in the response of the ionosphere F2-layer to geomagnetic activity , 1997 .

[18]  I. V. Zhivetiev,et al.  Global electron content: a new conception to track solar activity , 2008 .

[19]  S. Pulinets,et al.  Improvements of the International Reference Ionosphere model for the topside electron density profile , 2006 .

[20]  L. R. Canfield,et al.  First Solar EUV Irradiances Obtained from SOHO by the Celias/Sem , 1998 .

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

[22]  Yuk L. Yung,et al.  Short‐period solar cycle signals in the ionosphere observed by FORMOSAT‐3/COSMIC , 2008 .

[23]  J. Holt,et al.  Long‐term temperature trends in the ionosphere above Millstone Hill , 2008 .

[24]  D. J. Strickland,et al.  Solar extreme ultraviolet irradiance: Present, past, and future , 2011 .

[25]  J. Bremer,et al.  Long-term trends in foF2: A comparison of various methods , 2005 .

[26]  T. Woods,et al.  Anomalously low solar extreme‐ultraviolet irradiance and thermospheric density during solar minimum , 2010 .