TY - JOUR
T1 - Comparison of the IRI 2001 model with electron density profiles observed from topside sounder on-board the Ohzora (EXOS-C) and the Akebono (EXOS-D) satellites
AU - Uemoto, J.
AU - Ono, T.
AU - Kumamoto, A.
AU - Iizima, M.
N1 - Funding Information:
The Ohzora and Akebono satellites were established by the Institute of Space and Astronautical Science (ISAS). The activity of the first author (J. Uemoto) was supported by the Grant-in-Aid for JSPS Fellows, The Ministry of Education, Culture, Sports, Science and Technology, Japan. Activities of three authors (T. Ono, M. Iizima, and A. Kumamoto) are supported by the 21th century COE program “Advanced Science and Technology Center for the Dynamic Earth” at Tohoku University.
PY - 2007
Y1 - 2007
N2 - For the purpose of evaluation of the IRI 2001 model, the topside sounder data obtained from the Ohzora (EXOS-C) and the Akebono (EXOS-D) satellites in the magnetic latitude range from -50° to 50° were compared with the profiles calculated from the IRI model. Based on the electron density profiles obtained from the Ohzora satellite, the difference between the IRI model and observations is within a factor of 0.2-2.0. However, within the magnetic latitude range from 10° to 30° for the local time sector from 19 LT to 21 LT, the calculated peak height and density of the F 2 layer (hmF2 and foF2) were higher and lower than the observational profiles. The IRI 2001 model was able to reproduce well density profiles in the mid-latitude region, on the other hand, it tended to overestimate in the equatorial region. As a result of the comparison with the Akebono satellite sounder data, it was confirmed that the IRI model generally tended to reproduce observed profiles well in lower altitude region (<1000 km) and overestimate in higher altitude region (>1000 km). However, even below 1000 km, the IRI model also overestimated in the magnetic latitude range from -50° to 20° for the local time sector from 00 LT to 09 LT.
AB - For the purpose of evaluation of the IRI 2001 model, the topside sounder data obtained from the Ohzora (EXOS-C) and the Akebono (EXOS-D) satellites in the magnetic latitude range from -50° to 50° were compared with the profiles calculated from the IRI model. Based on the electron density profiles obtained from the Ohzora satellite, the difference between the IRI model and observations is within a factor of 0.2-2.0. However, within the magnetic latitude range from 10° to 30° for the local time sector from 19 LT to 21 LT, the calculated peak height and density of the F 2 layer (hmF2 and foF2) were higher and lower than the observational profiles. The IRI 2001 model was able to reproduce well density profiles in the mid-latitude region, on the other hand, it tended to overestimate in the equatorial region. As a result of the comparison with the Akebono satellite sounder data, it was confirmed that the IRI model generally tended to reproduce observed profiles well in lower altitude region (<1000 km) and overestimate in higher altitude region (>1000 km). However, even below 1000 km, the IRI model also overestimated in the magnetic latitude range from -50° to 20° for the local time sector from 00 LT to 09 LT.
KW - Akebono (EXOS-D) satellite
KW - IRI
KW - Ohzora (EXOS-C) satellite
KW - Topside ionosphere
KW - Topside sounder
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U2 - 10.1016/j.asr.2006.10.019
DO - 10.1016/j.asr.2006.10.019
M3 - Article
AN - SCOPUS:34248512098
VL - 39
SP - 750
EP - 754
JO - Life sciences and space research
JF - Life sciences and space research
SN - 0273-1177
IS - 5
ER -