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| * **by how much do magnetospheric gaps & winds vary with time as a result of the non- stationary dynamos operating in cTTSs?** Magnetospheric gaps / winds are expected to vary in size / strength with time, reflecting changes in the large-scale magnetic topologies of cTTSs on timescales of a few yr. By monitoring selected cTTSs (those that already showed time-variable large-scale fields in particular) over the whole LP, we can work out how variable magnetospheric gaps / winds are and whether this variability is compatible with the survival of hJs. | * **by how much do magnetospheric gaps & winds vary with time as a result of the non- stationary dynamos operating in cTTSs?** Magnetospheric gaps / winds are expected to vary in size / strength with time, reflecting changes in the large-scale magnetic topologies of cTTSs on timescales of a few yr. By monitoring selected cTTSs (those that already showed time-variable large-scale fields in particular) over the whole LP, we can work out how variable magnetospheric gaps / winds are and whether this variability is compatible with the survival of hJs. | ||
| - | MaTYSSE aims at addressing these major issues through a detailed spectropolarimetric & photometric survey of ~30 wTTSs as well as a regular monitoring of ~5 cTTSs. | + | MaTYSSE aims at addressing these major issues through a detailed spectropolarimetric & photometric survey of ~40 wTTSs as well as a regular monitoring of ~5 cTTSs. |
| ===== References ===== | ===== References ===== | ||
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