The original paper is in English. Non-English content has been machine-translated and may contain typographical errors or mistranslations. ex. Some numerals are expressed as "XNUMX".
Copyrights notice
The original paper is in English. Non-English content has been machine-translated and may contain typographical errors or mistranslations. Copyrights notice
. Dst indeks ialah ukuran paling popular bagi skala ribut magnet, dan ia digunakan secara meluas sebagai pemantau keadaan magnetosfera Bumi. Sejak Dst indeks mengandungi sumbangan daripada pelbagai fenomena magnetosfera, adalah penting untuk membezakan setiap sumbangan untuk mendapatkan maklumat yang bermakna tentang keadaan magnetosfera. Terdapat beberapa usaha yang memodelkan evolusi temporal Dst indeks secara empirik, dan model empirikal ini mempertimbangkan beberapa sumbangan secara berasingan. Walau bagaimanapun, mereka hanya mengambil kira variasi jangka pendek, dan sumbangan daripada fenomena yang menunjukkan variasi jangka panjang diabaikan. Dalam kajian ini, kami telah membangunkan satu teknik untuk menganggar komponen variasi jangka panjang bagi Dst indeks menggunakan data angin suria dan model empirikal tak linear. Teknik yang baru dibangunkan menggunakan algoritma yang serupa dengan penapis zarah. Algoritma ini membenarkan pemprosesan dalam talian bagi urutan panjang Dst data, yang akan membolehkan anggaran masa nyata pembolehubah sistem dalam model sistem tak linear. Anggaran variasi jangka panjang boleh digunakan untuk anggaran tepat sumbangan lain kepada Dst indeks, yang akan memberikan maklumat yang boleh dipercayai tentang keadaan magnetosfera. Rangka kerja yang dicadangkan dalam kajian ini boleh digunakan untuk tujuan pemantauan masa nyata berterusan persekitaran magnetosfera.
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Salinan
Shin'ya NAKANO, Tomoyuki HIGUCHI, "Estimation of a Long-Term Variation of a Magnetic-Storm Index Using the Merging Particle Filter" in IEICE TRANSACTIONS on Information,
vol. E92-D, no. 7, pp. 1382-1387, July 2009, doi: 10.1587/transinf.E92.D.1382.
Abstract: The Dst index is the most popular measure of a scale of magnetic storms, and it is widely used as a monitor of the conditions of the Earth's magnetosphere. Since the Dst index contains contributions from multiple magnetospheric phenomena, it is important to distinguish each of the contributions in order to obtain meaningful information about the conditions of the magnetosphere. There have been several efforts which modeled temporal evolution of the Dst index empirically, and these empirical models considers some contributions separately. However, they take only short-term varations into accout, and contributions from phenomena which show long-term variations are neglected. In the present study, we have developed a technique for estimating the component of long-term variations of the Dst index using solar wind data and a nonlinear empirical model. The newly-developed technique adopts an algorithm which is similar to the particle filter. This algorithm allows an on-line processing of a long sequence of Dst data, which would enable a real-time estimation of system variables in a nonlinear system model. The estimates of the long-term variations can be used for accurate estimation of other contributions to the Dst index, which would provide credible information about the conditions of the magnetosphere. The framework proposed in the present study could be applied for the purpose of continuous real-time monitoring of the environment of the magnetosphere.
URL: https://global.ieice.org/en_transactions/information/10.1587/transinf.E92.D.1382/_p
Salinan
@ARTICLE{e92-d_7_1382,
author={Shin'ya NAKANO, Tomoyuki HIGUCHI, },
journal={IEICE TRANSACTIONS on Information},
title={Estimation of a Long-Term Variation of a Magnetic-Storm Index Using the Merging Particle Filter},
year={2009},
volume={E92-D},
number={7},
pages={1382-1387},
abstract={The Dst index is the most popular measure of a scale of magnetic storms, and it is widely used as a monitor of the conditions of the Earth's magnetosphere. Since the Dst index contains contributions from multiple magnetospheric phenomena, it is important to distinguish each of the contributions in order to obtain meaningful information about the conditions of the magnetosphere. There have been several efforts which modeled temporal evolution of the Dst index empirically, and these empirical models considers some contributions separately. However, they take only short-term varations into accout, and contributions from phenomena which show long-term variations are neglected. In the present study, we have developed a technique for estimating the component of long-term variations of the Dst index using solar wind data and a nonlinear empirical model. The newly-developed technique adopts an algorithm which is similar to the particle filter. This algorithm allows an on-line processing of a long sequence of Dst data, which would enable a real-time estimation of system variables in a nonlinear system model. The estimates of the long-term variations can be used for accurate estimation of other contributions to the Dst index, which would provide credible information about the conditions of the magnetosphere. The framework proposed in the present study could be applied for the purpose of continuous real-time monitoring of the environment of the magnetosphere.},
keywords={},
doi={10.1587/transinf.E92.D.1382},
ISSN={1745-1361},
month={July},}
Salinan
TY - JOUR
TI - Estimation of a Long-Term Variation of a Magnetic-Storm Index Using the Merging Particle Filter
T2 - IEICE TRANSACTIONS on Information
SP - 1382
EP - 1387
AU - Shin'ya NAKANO
AU - Tomoyuki HIGUCHI
PY - 2009
DO - 10.1587/transinf.E92.D.1382
JO - IEICE TRANSACTIONS on Information
SN - 1745-1361
VL - E92-D
IS - 7
JA - IEICE TRANSACTIONS on Information
Y1 - July 2009
AB - The Dst index is the most popular measure of a scale of magnetic storms, and it is widely used as a monitor of the conditions of the Earth's magnetosphere. Since the Dst index contains contributions from multiple magnetospheric phenomena, it is important to distinguish each of the contributions in order to obtain meaningful information about the conditions of the magnetosphere. There have been several efforts which modeled temporal evolution of the Dst index empirically, and these empirical models considers some contributions separately. However, they take only short-term varations into accout, and contributions from phenomena which show long-term variations are neglected. In the present study, we have developed a technique for estimating the component of long-term variations of the Dst index using solar wind data and a nonlinear empirical model. The newly-developed technique adopts an algorithm which is similar to the particle filter. This algorithm allows an on-line processing of a long sequence of Dst data, which would enable a real-time estimation of system variables in a nonlinear system model. The estimates of the long-term variations can be used for accurate estimation of other contributions to the Dst index, which would provide credible information about the conditions of the magnetosphere. The framework proposed in the present study could be applied for the purpose of continuous real-time monitoring of the environment of the magnetosphere.
ER -