A study on the cosmic electron density profile

H. F. Tsai; D. D. Feng; J. Y. Liu; C. H. Liu; W. H. Tsai

doi:10.1016/S0964-2749(02)80237-2

A study on the cosmic electron density profile

H. F. Tsai, D. D. Feng, J. Y. Liu, C. H. Liu, W. H. Tsai

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

3 引文斯高帕斯（Scopus）

摘要

This paper shows a simulation process of retrieving ionospheric electron density from the Global Positioning System/Meteorology (GPS/MET) to examine the accuracy of the retrieval procedure for the COSMIC project³ during solar minimum and maximum periods. Results show that the error of the maximum electron density (NmF₂) is under 25%, and the error is greater in the solar maximum than in the solar minimum period. The mean error of the height of NmF₂ (i.e. hmF₂) is less than about 13 km and seems to have no correlation with solar activity.3A Taiwan-US joint project for Constellation Observing System for Meteorology, Ionosphere, and Climate.

原文	???core.languages.en_GB???
頁（從 - 到）	329-333
頁數	5
期刊	COSPAR Colloquia Series
卷	12
發行號	C
DOIs	https://doi.org/10.1016/S0964-2749(02)80237-2
出版狀態	已出版 - 2002

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10.1016/S0964-2749(02)80237-2

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@article{6673dec716cb4358bada059299276c7d,

title = "A study on the cosmic electron density profile",

abstract = "This paper shows a simulation process of retrieving ionospheric electron density from the Global Positioning System/Meteorology (GPS/MET) to examine the accuracy of the retrieval procedure for the COSMIC project3 during solar minimum and maximum periods. Results show that the error of the maximum electron density (NmF2) is under 25%, and the error is greater in the solar maximum than in the solar minimum period. The mean error of the height of NmF2 (i.e. hmF2) is less than about 13 km and seems to have no correlation with solar activity.3A Taiwan-US joint project for Constellation Observing System for Meteorology, Ionosphere, and Climate.",

author = "Tsai, {H. F.} and Feng, {D. D.} and Liu, {J. Y.} and Liu, {C. H.} and Tsai, {W. H.}",

note = "Funding Information: We thank Dr. Stig Syndergaard for providing ROSAP program and thank Dr. William Schreiner in UCAR for providing the GPS/MET Level 2 ionospheric data. This work was partially supported by National Science Council in Taiwan Grants NSC 89-2119-M-008-005.",

year = "2002",

doi = "10.1016/S0964-2749(02)80237-2",

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volume = "12",

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TY - JOUR

T1 - A study on the cosmic electron density profile

AU - Tsai, H. F.

AU - Feng, D. D.

AU - Liu, J. Y.

AU - Liu, C. H.

AU - Tsai, W. H.

N1 - Funding Information: We thank Dr. Stig Syndergaard for providing ROSAP program and thank Dr. William Schreiner in UCAR for providing the GPS/MET Level 2 ionospheric data. This work was partially supported by National Science Council in Taiwan Grants NSC 89-2119-M-008-005.

PY - 2002

Y1 - 2002

N2 - This paper shows a simulation process of retrieving ionospheric electron density from the Global Positioning System/Meteorology (GPS/MET) to examine the accuracy of the retrieval procedure for the COSMIC project3 during solar minimum and maximum periods. Results show that the error of the maximum electron density (NmF2) is under 25%, and the error is greater in the solar maximum than in the solar minimum period. The mean error of the height of NmF2 (i.e. hmF2) is less than about 13 km and seems to have no correlation with solar activity.3A Taiwan-US joint project for Constellation Observing System for Meteorology, Ionosphere, and Climate.

AB - This paper shows a simulation process of retrieving ionospheric electron density from the Global Positioning System/Meteorology (GPS/MET) to examine the accuracy of the retrieval procedure for the COSMIC project3 during solar minimum and maximum periods. Results show that the error of the maximum electron density (NmF2) is under 25%, and the error is greater in the solar maximum than in the solar minimum period. The mean error of the height of NmF2 (i.e. hmF2) is less than about 13 km and seems to have no correlation with solar activity.3A Taiwan-US joint project for Constellation Observing System for Meteorology, Ionosphere, and Climate.

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U2 - 10.1016/S0964-2749(02)80237-2

DO - 10.1016/S0964-2749(02)80237-2

M3 - 期刊論文

AN - SCOPUS:23044476397

SN - 0964-2749

VL - 12

SP - 329

EP - 333

JO - COSPAR Colloquia Series

JF - COSPAR Colloquia Series

IS - C

ER -

A study on the cosmic electron density profile

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