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The wind braking model and its applications of magnetars are discussed. Thedecreasing torque of magnetars during outbursts, anti-glitch, andanti-correlations between radiation and timing are understandable in the windbraking model. Recent timing observations of magnetars are also consistent withthe previous modeling. A magnetism-powered wind nebula and a braking indexsmaller than three are the two predictions. Besides isolated magnetars, theremay also be accreting magnetars in binary systems and magnetars accreting fromfallback disks. Observationally, ultra-luminous X-ray pulsars may be accretingmagnetars, while super-slow magnetars may be magnetars with fallback disks inthe past. Many works are needed for both isolated magnetars and accretingmagnetars.

Understanding recent observations of isolated magnetars and accreting magnetars from the magnetospheric point of view