International Reference Ionosphere 2000

By Dieter Bilitza. 2001

1,314 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/14f51f7c99b01c776c6e6dca48bb1d7218117333

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Citations in the corpus

Comparison of COSMIC ionospheric measurements with ground-based observations and model predictions : Preliminary results (2007, methodology): “Comparisons are also made between these observations and electron densities calculated by the latest International Reference Ionosphere model (IRI-2001) [ Bilitza, 2001 ] and the National Center for Atmospheric Research Thermosphere-Ionosphere-Electrodynamics General Circulation Model (NCAR-TIEGCM) ”
Assimilation of GIRO data into a real‐time IRI (2012, methodology): “The International Reference Ionosphere (IRI) empirical model with a long history of development and refinement [Rawer et al., 1978; Bilitza, 1990, 2001; Bilitza and Reinisch, 2008] has been used for a wide range of applications in science, engineering, and education and has generally outperformed…”
Does the F10.7 index correctly describe solar EUV flux during the deep solar minimum of 2007-2009? (2011, methodology): “F10.7 is also usually used as the solar activity proxy to develop ionospheric and thermospheric models, such as the IRI model [ Bilitza, 2001 ] and the NRLMSISE‐00 model [Picone et al., 2002].”
STORM: An empirical storm‐time ionospheric correction model 1. Model description (2002, methodology): “This correction has now been included in the International Reference Ionosphere, IRI 2000 [Bilitza, 2001].”
The IGS VTEC maps: a reliable source of ionospheric information since 1998 (2009, background): “Useful because, in both Science and Technology fields, they can provide valuable information concerning space weather events, empirical model predictions, and user navigation improvement, among others (see for example Coster and Komjathy 2008; Bilitza 2001; Hernández-Pajares et al. 2000).”
tempo2, a new pulsar timing package ¿ II. The timing model and precision estimates (2006, methodology): “Models of the ionosphere are available (e.g. Schaer 1999; Bilitza 2001); however, the predicted TEC is accurate to only ∼3–20 TECU (Mamoru, Kondo & Kawai 2003).”
The international reference ionosphere today and in the future (2011, methodology): “Of the 80,000 topside electron density profiles obtained from digitized ISIS-2 ionograms (Huang et al. 2002; Bilitza et al. 2004; Benson and Bilitza 2009; Jackson 1969).”
Global distributions and occurrence rates of transient luminous events (2008, methodology): “On the basis of the IRI model [Bilitza, 2001], the mean nighttimes ambient electron density at 80–90 km is 90 cm 3 and this leads to a 1.3.”
TEC derived from GPS network in India and comparison with the IRI (2007, background): “Measured TEC were then compared with the TEC predicted by the International Reference Ionosphere, 2001 [ 4 ] and a regional TEC model developed for the Indian zone [5] to assess their predictability vis -a-vis the observations.”
Variations of electron density based on long‐term incoherent scatter radar and ionosonde measurements over Millstone Hill (2005, methodology): “Many efforts have been made on the improvement for the IRI topside electron density profile model [e.g., Bilitza, 2001, 2004; Huang and Reinisch, 2001].”
Three‐dimensional waveform modeling of ionospheric signature induced by the 2004 Sumatra tsunami (2006, methodology): “The 3D ionosphere is based on the IRI model [Bilitza, 2001] at 3:00 UT for electron density, the SAMI model [Huba et al., 2000] for collision, production and loss ion parameters and the IGRF model (F. J. Lowes, The International Geomagnetic Reference Field: A health warning,…”
Ionospheric remote sensing of the Denali Earthquake Rayleigh surface waves (2003, background): “We then computed the mean cross-correlation of these pairs for altitudes up to 400 km.Amaximum correlation of 0.8 is found for an altitude of 290–300 km, which is slightly more than the modeled altitude of maximum ionization, in the range 280–285 km after IRI [Bilitza, 2001] at the local time of obs”
Behavior of the O+/H+ transition height during the extreme solar minimum of 2008 (2009, result): “[11] The observed behavior of the transition height and the plasma properties in the topside ionosphere stand in significant contrast to those predicted using the international reference ionosphere (IRI) [Bilitza, 2001].”
The International Reference Ionosphere 2012 – a model of international collaboration (2014, methodology): “More global ionosonde data – Incoherent scatter (ICS) data 1995 IRI-95: online (IRIWeb) (Bilitza 1997) Improvements at low latitudes DE-2 data 1999 URSI resolution IRI recognized as the international standard for the ionosphere 2001 IRI-2001 (Bilitza 2001) –”