1995
DOI: 10.1016/0273-1177(95)00214-y
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Results of spectral analysis of the Phobos-2 magnetic field data

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Cited by 8 publications
(2 citation statements)
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“…The period of 26.7 d can then be interpreted as period of relative rotation of sunspots at mean latitude of their appearance j ¼ 15 with T 1 ¼ 25:28 d, combined with the rotation of the Sun at the base of convection zone, with T ¼ 1:3 yr at the same latitudes (Howe et al, 2000). Taking T 2 ¼ 1:3 yr ¼ 474:81 d and 1=T 12 ¼ 1=T 1 AE 1=T 2 , where alternative signs apply because rotation at T ¼ 1:3 yr occurs in opposite phase below and above the base of the convection zone (Howe et al, 2000), we obtain T 12 ¼ 26:7 or 24.0 d. We have previously found evidence that the 24 d period exists in IMF data measured in the solar wind near the Mars on board Phobos-2 (Kuznetsova et al, 1995;Tsirulnik et al, 1997a).…”
Section: Spectra Of Imf and Sunspotsmentioning
confidence: 80%
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“…The period of 26.7 d can then be interpreted as period of relative rotation of sunspots at mean latitude of their appearance j ¼ 15 with T 1 ¼ 25:28 d, combined with the rotation of the Sun at the base of convection zone, with T ¼ 1:3 yr at the same latitudes (Howe et al, 2000). Taking T 2 ¼ 1:3 yr ¼ 474:81 d and 1=T 12 ¼ 1=T 1 AE 1=T 2 , where alternative signs apply because rotation at T ¼ 1:3 yr occurs in opposite phase below and above the base of the convection zone (Howe et al, 2000), we obtain T 12 ¼ 26:7 or 24.0 d. We have previously found evidence that the 24 d period exists in IMF data measured in the solar wind near the Mars on board Phobos-2 (Kuznetsova et al, 1995;Tsirulnik et al, 1997a).…”
Section: Spectra Of Imf and Sunspotsmentioning
confidence: 80%
“…A description of the method by which the statistical significance of spectral components is estimated can be found in Tsirulnik et al (1997b). A complete description of MGM can be found in Kuznetsova et al (1995) and Tsirulnik et al (1997a). We used series of 27-day averaged jBj values of the IMF based on hourly mean values measured by various spacecrafts in the solar wind near the plane of the ecliptic at a distance of 1 AU during the time period 1964-1997 obtained from the OMNI database (http://www.omni.web.gsfc.nasa.…”
Section: Methods Of Analysis and Data Usedmentioning
confidence: 99%