Stellar X-rays and magnetic activity in 3D MHD coronal models

Open Access

Table 1

Summary of numerical experiments.

Run	a ⁽¹⁾	Φ [Mx] ⁽²⁾
1B	1	7.4 × 10²⁰
2B	2	1.5 × 10²¹
5B	5	3.7 × 10²¹
10B	10	7.4 × 10²¹
20B	20	1.5 × 10²²

Notes. ⁽¹⁾The photospheric magnetic field strength is increased by the factor a. ⁽²⁾Φ is the total surface unsigned magnetic flux.

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