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Table 4.

Properties of the magnetic map for EV Lac, DS Leo, and CN Leo, reconstructed from different epochs of SPIRou near-infrared time series.

EV Lac
DS Leo
CN Leo
2019b 2020b2021a 2021b 2020b2021a 2021b2022a 2019a 2019b2020a 2020b2021a 2021b2022a
fV [%] 9 19 10 6 15 12 18 15
Bmean [G] 72.5 297.7 265.1 44.3 17.9 350.2 321.8 486.9 420.1
Bmax [G] 175.8 700.0 690.5 115.2 34.9 650.4 607.8 937.6 820.9
Bpol [%] 99.1 99.7 99.2 55.9 72.9 99.9 99.9 99.9 99.9
Btor [%] 0.9 0.3 0.8 44.1 27.0 0.1 0.1 0.1 0.1
Bdip [%] 63.1 88.7 82.8 64.0 83.2 99.4 99.4 99.3 99.2
Bquad [%] 25.4 9.4 14.6 28.5 13.1 0.5 0.6 0.6 0.7
Boct [%] 10.2 1.3 2.4 3.9 2.6 0.0 0.0 0.1 0.1
Baxisym [%] 25.1 12.1 1.8 39.4 30.6 99.5 99.6 99.9 99.9
Baxisym, pol [%] 24.6 12.0 1.2 3.9 9.2 99.5 99.6 99.9 99.9
Obliquity [°] 50.5 68.5 86.5 75.5 69.5 4.5 3.5 1.5 1.5

Notes. The following quantities are listed: filling factor on Stokes V; mean magnetic strength; maximum magnetic strength; poloidal and toroidal magnetic energy as a fraction of the total energy; dipolar, quadrupolar and octupolar magnetic energy as a fraction of the poloidal energy; axisymmetric magnetic energy as a fraction of the total energy; and obliquity of the dipolar component relative to the rotation axis. To compute the local magnetic field (i.e., within a grid cell of the ZDI stellar model) the field strength should be divided by the associated filling factor fV.

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