The Birmingham Solar Oscillation Network (BiSON) has acquired high precision solar mean magnetic field (SMMF) data on a 40-second cadence for a decade. We present first attempts to compare such data from recent years with the occurence of CME's as recorded by LASCO using correlation techniques applied to measurements from different BiSON instruments to maximise the sensitivity to CME related SMMF responses. SMMF measurements were recorded at the time of occurence of several hundreds CME's.
|Published - 01 Jan 2005
|General Assembly of the International Astronomical Union 2003 - Sydney, Australia
Duration: 13 Jun 2003 → 26 Jun 2003
Conference number: 25
|General Assembly of the International Astronomical Union 2003
|13 Jun 2003 → 26 Jun 2003