On the Analytical Description of the Topside Ionosphere by NeQuick: Modeling the Scale Height Through COSMIC/FORMOSAT-3 Selected Data

The analytical description of the topside ionosphere included in the NeQuick model is studied in detail. First, the modeled scale height behavior is analyzed at infinity and for the lowest part of the topside region; in the latter case, the analysis is done through an expansion in Taylor series near the F2-layer peak. Moreover, the significant influence of the three NeQuick topside parameters in the modeling of the topside profile is investigated in detail and, in particular, it is shown that for the lowest part of the topside the model assumes a linearly increasing trend of the topside scale height. Second, the topside formulation is inverted to derive a fully analytical expression of the topside scale height as a function of the electron density and F2-layer peak parameters. This expression has been applied to a selected and very reliable dataset of Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC)/FORMOSAT-3 radio occultation profiles. Statistical analyses strongly support the hypothesis embedded in NeQuick regarding the linear trend of the topside scale height for the lowest part of the topside.

[1]  S. Pulinets,et al.  A global empirical model of the ionospheric topside electron density , 2004 .

[2]  Sandro M. Radicella,et al.  A new version of the NeQuick ionosphere electron density model , 2008 .

[3]  Riccardo Notarpietro,et al.  Electron density extrapolation above F2 peak by the linear Vary‐Chap model supporting new Global Navigation Satellite Systems‐LEO occultation missions , 2017 .

[4]  S. Pulinets,et al.  RECENT ADVANCES IN TOPSIDE PROFILE MODELING , 2002 .

[5]  Libo Liu,et al.  An analysis of the scale heights in the lower topside ionosphere based on the Arecibo incoherent scatter radar measurements , 2007 .

[6]  D. Themens,et al.  Examining the use of the NeQuick bottomside and topside parameterizations at high latitudes , 2018 .

[7]  Reinhart Leitinger,et al.  Topside electron density in IRI and NeQuick: Features and limitations , 2006 .

[8]  R. Rizzi,et al.  Modeling the Lower Part of the Topside Ionospheric Vertical Electron Density Profile Over the European Region by Means of Swarm Satellites Data and IRI UP Method , 2018 .

[9]  Christian Rocken,et al.  The COSMIC/FORMOSAT-3 Mission: Early Results , 2008 .

[10]  D. Bilitza,et al.  Topside Electron Density Representations for Middle and High Latitudes: A Topside Parameterization for E‐CHAIM Based On the NeQuick , 2018 .

[11]  S. Radicella,et al.  On the use of NeQuick topside option in IRI-2007 , 2009 .

[12]  Bodo W. Reinisch,et al.  Global Ionospheric Radio Observatory (GIRO) , 2011 .

[13]  Jaume Sanz,et al.  Improvement of ionospheric electron density estimation with GPSMET occultations using Abel inversion and VTEC information , 2003 .

[14]  M. Hernández‐Pajares,et al.  Linear Vary-Chap Topside Electron Density Model with Topside Sounder and Radio-Occultation Data , 2019, Surveys in Geophysics.

[15]  G. Hulot,et al.  Swarm: A constellation to study the Earth’s magnetic field , 2006 .

[16]  A. Farmer,et al.  The solar-terrestrial environment , 1996 .

[17]  D. Bilitza,et al.  International Reference Ionosphere 2007: Improvements and new parameters , 2008 .

[18]  S. Pulinets,et al.  Results of the modeling of the topside electron density profile using the Chapman and Epstein functions , 2002 .

[19]  Michael Pezzopane,et al.  Comparison between IRI and preliminary Swarm Langmuir probe measurements during the St. Patrick storm period , 2016, Earth, Planets and Space.

[20]  J. Habarulema,et al.  A simultaneous study of ionospheric parameters derived from FORMOSAT‐3/COSMIC, GRACE, and CHAMP missions over middle, low, and equatorial latitudes: Comparison with ionosonde data , 2014 .

[21]  D. Themens,et al.  A top to bottom evaluation of IRI 2007 within the polar cap , 2014 .

[22]  Karl Rawer,et al.  Replacement of the present sub-peak plasma density profile by a unique expression , 1982 .

[23]  Xiong Hu,et al.  Analysis of inversion errors of ionospheric radio occultation , 2009 .

[24]  Henry Rishbeth,et al.  Introduction to ionospheric physics , 1969 .

[25]  D. Bilitza,et al.  Modeling the F2 Topside and Plasmasphere for IRI , 2005 .

[26]  L. Roininen,et al.  Validation of NeQuick TEC data ingestion technique against C/NOFS and EISCAT electron density measurements , 2016 .

[27]  D. Bilitza,et al.  Enhancing the ISIS‐I Topside Digital Ionogram Database , 2018, Radio Science.

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

[29]  S. Chapman,et al.  The absorption and dissociative or ionizing effect of monochromatic radiation in an atmosphere on a rotating earth , 1931 .

[30]  Sandro M. Radicella,et al.  Diffusive equilibrium models for the height region above the F2 peak , 2002 .

[31]  J. J. Angerami,et al.  Studies of planetary atmospheres: 1. The distribution of electrons and ions in the Earth's exosphere , 1964 .

[32]  Y. Chu,et al.  A global survey of COSMIC ionospheric peak electron density and its height: A comparison with ground-based ionosonde measurements , 2010 .

[34]  B. Nava,et al.  On the Use of Topside RO‐Derived Electron Density for Model Validation , 2018 .

[35]  P. S. Epstein,et al.  REFLECTION OF WAVES IN AN INHOMOGENEOUS ABSORBING MEDIUM. , 1930, Proceedings of the National Academy of Sciences of the United States of America.

[36]  M. Pezzopane,et al.  The ESA Swarm mission to help ionospheric modeling: a new NeQuick topside formulation for mid-latitude regions , 2019, Scientific Reports.

[37]  S. Radicella,et al.  Comparison of analytical functions used to describe topside electron density profiles with satellite data , 2005 .

[38]  Bodo W. Reinisch,et al.  International Reference Ionosphere 2016: From ionospheric climate to real‐time weather predictions , 2017 .

[39]  Reinhart Leitinger,et al.  An improved bottomside for the ionospheric electron density, model NeQuick , 2005 .

[40]  W. Wan,et al.  Variations of topside ionospheric scale heights over Millstone Hill during the 30-day incoherent scatter radar experiment , 2007 .

[41]  John Bosco Habarulema,et al.  Adapting a climatology model to improve estimation of ionosphere parameters and subsequent validation with radio occultation and ionosonde data , 2017 .

[42]  D. Bilitza Evaluation of the IRI-2007 model options for the topside electron density , 2009 .

[43]  J. Wahlund,et al.  Thermal ion imagers and Langmuir probes in the Swarm electric field instruments , 2017 .