Published June 2003 | Version v1
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Checking the new IRI model: The bottomside B parameters

  • 1. CASLEO, CONICET, San Juan (Argentina)
  • 2. Institute of Atmospheric Physics, Prague (Czech Republic)
  • 3. Estacion de Sondeos Atmosfericos, INTA, Huelva (Spain)
  • 4. Instituto de Geofisica y Astronomia, La Lisa, Havana (Cuba)
  • 5. Fac. Regional Tucuman, Univ. Tecnologica Nacional, Tucuman (Argentina)
  • 6. Laboratorio de lonosfera, Dpto. de Fisica, CONICET, Tucuman (Argentina)

Description

Electron density profiles obtained at Pruhonice (50.0, 15.0), El Arenosillo (37.1, 353.2) and Havana (23, 278) were used to check the bottom-side B parameters BO (thickness parameter) and B1 (shape parameter) predicted by the new IRI - 2000 version. The electron density profiles were derived from ionograms using the ARP technique. The data base includes daytime and nighttime ionograms recorded under different seasonal and solar activity conditions. Comparisons with IRI predictions were also done. The analysis shows that: a) The parameter B1 given by IRI 2000 reproduces better the observed ARP values than the IRI-90 version and b) The observed BO values are in general well reproduced by both IRI versions: IRI-90 and IRI-2000. (author)

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Part of:
Proceedings of the IRI Task Force Activity 2002. 1. ed

Additional details

Publishing Information

ISBN
92-95003-18-7
Imprint Title
Proceedings of the IRI Task Force Activity 2002. 1. ed
Imprint Pagination
193 p.
Journal Page Range
p. 39-50
Report number
IC/IR--2003/3

Optional Information

Notes
7 refs, 9 figs, 2 tabs