ИСТИНА

Juno spacecraft provided plenty of new valuable data on the magnetic field inside the Jovian magnetosphere. We use this data to develop a new empirical model of the Jupiter's current sheet. Our model combines successful elements from several previous models. It has a disk-like current with constant north-south thickness and a piecewise current density dependence on the cylindrical distance. The model also takes into account the lagging of the magnetodisc from magnetic equator. We test the model using the Juno spacecraft magnetometer data and compare performance of our model with the results of previous ones.