期刊
ASTROPHYSICAL JOURNAL
卷 709, 期 1, 页码 301-307出版社
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/709/1/301
关键词
solar-terrestrial relations; Sun: activity; Sun: magnetic fields
By coupling a solar surface flux transport model with an extrapolation of the heliospheric field, we simulate the evolution of the Sun's open magnetic flux and the heliospheric current sheet (HCS) based on observational data of sunspot groups since 1976. The results are consistent with measurements of the interplanetary magnetic field near Earth and with the tilt angle of the HCS as derived from extrapolation of the observed solar surface field. This opens the possibility for an improved reconstruction of the Sun's open flux and the HCS into the past on the basis of empirical sunspot data.
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