globalchange  > 气候减缓与适应
DOI: 10.1002/2014GL060047
论文题名:
The wavelet transform function to analyze interplanetary scintillation observations
作者: Aguilar-Rodriguez E.; Rodriguez-Martinez M.; Romero-Hernandez E.; Mejia-Ambriz J.C.; Gonzalez-Esparza J.A.; Tokumaru M.
刊名: Geophysical Research Letters
ISSN: 0094-10047
EISSN: 1944-9778
出版年: 2014
卷: 41, 期:10
起始页码: 3331
结束页码: 3335
语种: 英语
英文关键词: earthquakes ; finite fault models ; overdamped dynamics ; radiated energy ; seismic energy ; seismic source
Scopus关键词: Earthquakes ; Radio telescopes ; Fault model ; Overdamped ; Radiated energies ; Seismic energy ; Seismic source ; Scintillation ; magnetosphere ; observational method ; remote sensing ; solar wind ; wavelet analysis
英文摘要: Interplanetary scintillation (IPS) observations are useful to remotely sense the inner heliosphere. We present a new technique to analyze IPS observations using a wavelet transform (WT) function. This technique allows us to derive, in a straightforward way, a simple method to obtain the scintillation index (m). We tested this WT technique to analyze IPS observations obtained by the Solar-Terrestrial Environment Laboratory (STEL) radio telescope. The analysis of the m index of the radio source 3C48 detected by STEL over the year 2012 shows the expected decrease with solar elongation reported in previous studies. The WT technique has a great potential for future solar wind studies using IPS observations from contemporary radio telescopes. © 2014. American Geophysical Union. All Rights Reserved.
URL: https://www.scopus.com/inward/record.uri?eid=2-s2.0-84902273645&doi=10.1002%2f2014GL060047&partnerID=40&md5=3a0dd5620aa4be14c71abb19a09ec74a
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资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/7311
Appears in Collections:气候减缓与适应

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作者单位: Instituto de Geofisica, Unidad Michoacan, Universidad Nacional Autõnoma de México, Mexico City, Mexico

Recommended Citation:
Aguilar-Rodriguez E.,Rodriguez-Martinez M.,Romero-Hernandez E.,et al. The wavelet transform function to analyze interplanetary scintillation observations[J]. Geophysical Research Letters,2014-01-01,41(10).
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