Sunspot drawings obtained at National Astronomical Observatory of Japan during the years 1954-1986 were used to determine the differential rotation of the Sun. From the limited data set of three solar cycles it was found that three factors (the level of cycle activity, the cycle phase, and sunspot t
Solar meridional motions derived from sunspot observations
β Scribed by M. A. Kambry; J. Nishikawa; T. Sakurai; K. Ichimoto; E. Hiei
- Publisher
- Springer
- Year
- 1991
- Tongue
- English
- Weight
- 395 KB
- Volume
- 132
- Category
- Article
- ISSN
- 0038-0938
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β¦ Synopsis
Sunspot drawings obtained at the National Astronomical Observatory of Japan during the years 1954-1986 were used to determine meridional motions of the Sun. A meridional flow of a few ms -~ was found, which is equatorward in the latitude range from -20 ~ to + 15 ~ and is poleward at higher latitudes in both hemispheres. A northward flow of 0.01 ~ day-1 or 1.4 ms i at mid-latitudes (between 10 ~ and 20 ~ was also detected. From our limited data-set of three solar cycles, an indication of solar-cycle dependence of meridional motions was found.
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