Effects observed in the equatorial and low latitude ionospheric F-region in the Brazilian sector during low solar activity geomagnetic storms and comparison with the COSMIC measurements

Abstract The main objective of the present investigation has been to compare the ionospheric parameters (NmF2 and hmF2) observed by two ground-based ionospheric sounders (one at PALMAS- located near the magnetic equator and the other at Sao Jose dos Campos-located in the low-latitude region) in the Brazilian sector with that by the satellite FORMOSAT-3/COSMIC radio occultation (RO) measurements during two geomagnetic storms which occurred in December 2006 and July 2009. It should be pointed out that in spite of increasing the latitude (to 10°) and longitude (to 20°) around the stations; we had very few common observations. It has been observed that both the peak electron density (NmF2) and peak height (hmF2) observed by two different techniques (space-borne COSMIC and ground-based ionosondes) during both the geomagnetic storm events compares fairly well (with high correlation coefficients) at the two stations in the Brazilian sector. It should be pointed out that due to equatorial spread F (ESF) in the first storm (December 2006) and no-reflections from the ionosphere during nighttime in the second storm (July 2009), we had virtually daytime data from the two ionosondes.

[1]  Ying-Hwa Kuo,et al.  Artificial plasma cave in the low‐latitude ionosphere results from the radio occultation inversion of the FORMOSAT‐3/COSMIC , 2010 .

[2]  Jann‐Yenq Liu,et al.  Three-dimensional ionospheric electron density structure of the Weddell Sea Anomaly , 2008 .

[3]  Thomas J. Immel,et al.  Temporal modulations of the longitudinal structure in F2 peak height in the equatorial ionosphere as observed by COSMIC , 2009 .

[4]  T. Fang,et al.  Motions of the equatorial ionization anomaly crests imaged by FORMOSAT‐3/COSMIC , 2007 .

[5]  W. S. Chen,et al.  Dayside ionospheric response to recurrent geomagnetic activity during the extreme solar minimum of 2008 , 2010 .

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

[7]  Pawel Wielgosz,et al.  Ionospheric electron density observed by FORMOSAT-3/COSMIC over the European region and validated by ionosonde data , 2011 .

[8]  C. Liu,et al.  A near real‐time phenomenological model of ionospheric electron density based on GPS radio occultation data , 2009 .

[9]  R. Roble,et al.  A dayside ionospheric positive storm phase driven by neutral winds , 2008 .

[10]  Biqiang Zhao,et al.  Global characteristics of occurrence of an additional layer in the ionosphere observed by COSMIC/FORMOSAT‐3 , 2011 .

[11]  V. Klimenko,et al.  Disturbances in the ionospheric F-region peak heights in the American longitudinal sector during geomagnetic storms of September 2005 , 2011 .

[12]  S. Kawamura,et al.  A physical mechanism of positive ionospheric storms at low latitudes and midlatitudes , 2010 .

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

[14]  P. Fagundes,et al.  Numerical modeling of ionospheric effects in the middle‐ and low‐latitude F region during geomagnetic storm sequence of 9–14 September 2005 , 2011 .

[15]  S. Solomon,et al.  Observations and simulations of the ionospheric and thermospheric response to the December 2006 geomagnetic storm : Initial phase , 2007 .

[16]  Stanley C. Solomon,et al.  Meridional winds derived from COSMIC radio occultation measurements , 2007 .

[17]  M. Buonsanto Ionospheric Storms — A Review , 1999 .

[18]  P. Fagundes,et al.  Effects observed in the ionospheric F-region in the South American sector during the intense geomagnetic storm of 14 December 2006 , 2010 .

[19]  Libo Liu,et al.  Seasonal variations of the ionospheric electron densities retrieved from Constellation Observing System for Meteorology, Ionosphere, and Climate mission radio occultation measurements , 2009 .

[20]  R. W. Spiro,et al.  Penetration of high latitude electric fields effects tolow latitude during Sundial 1984 , 1988 .

[21]  K. Subbarao,et al.  Response of the equatorial ionosphere in the Indian (midnight) sector to the severe magnetic storm of July 15, 2000 , 2002 .

[22]  K. Shiokawa,et al.  Super plasma fountain and equatorial ionization anomaly during penetration electric field , 2009 .

[23]  Libo Liu,et al.  Topside ionospheric scale heights retrieved from Constellation Observing System for Meteorology, Ionosphere, and Climate radio occultation measurements , 2008 .

[24]  Michael C. Kelley,et al.  Imaging the structure of a large‐scale TID using ISR and TEC data , 2004 .

[25]  Jann‐Yenq Liu,et al.  Longitudinal structure of the equatorial ionosphere: Time evolution of the four-peaked EIA structure , 2007 .

[26]  Jann‐Yenq Liu,et al.  Plausible effect of atmospheric tides on the equatorial ionosphere observed by the FORMOSAT‐3/COSMIC: Three‐dimensional electron density structures , 2007 .

[27]  Jens Wickert,et al.  A global climatology of ionospheric irregularities derived from GPS radio occultation , 2008 .

[28]  Michel Blanc,et al.  On the control of magnetospheric convection by the spatial distribution of ionospheric conductivities , 1982 .

[29]  Larry J. Paxton,et al.  First look at the 20 November 2003 superstorm with TIMED/GUVI: Comparisons with a thermospheric global circulation model , 2005 .

[30]  Xinan Yue,et al.  Error analysis of Abel retrieved electron density profiles from radio occultation measurements , 2010 .

[31]  I. F. Grant,et al.  Comparison of plasma flow velocities determined by the ionosonde Doppler drift technique, SuperDARN radars, and patch motion , 1995 .

[32]  S. Solomon,et al.  Midlatitude nighttime enhancement in F region electron density from global COSMIC measurements under solar minimum winter condition , 2008 .

[33]  Arthur D. Richmond,et al.  The ionospheric disturbance dynamo , 1980 .

[34]  Anthony J. Mannucci,et al.  Comparison of COSMIC occultation‐based electron density profiles and TIP observations with Arecibo incoherent scatter radar data , 2009 .

[35]  Ying-Hwa Kuo,et al.  Behavior of the F2 peak ionosphere over the South Pacific at dusk during quiet summer conditions from COSMIC data , 2008 .

[36]  Ying-Hwa Kuo,et al.  Comparison of COSMIC ionospheric measurements with ground-based observations and model predictions : Preliminary results , 2007 .