  Assuming neutrinos are Majorana particles having non-zero transition magnetic
moments, a global analysis of solar neutrino data, together with the new
KamLAND data, is presented in the resonant spin flavor precession (RSFP)
framework. The allowed regions from solar data combined with new KamLAND data
are examined at 0.95 confidence level (CL). The electron antineutrino flux from
the Sun is calculated, and via the results obtained several limits are set for
muB.
