Hinode observations and 3D magnetic structure of an X-ray bright point

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Table 1

Some of the prominent EIS lines present in the CAM_QS_2AS_CONTEXT study used.

Ion	λ (Å)	Waveband	Region	log T_max(K)

He II	256.320	lw	Chromosphere	4.9
O V	192.910	sw	TR	5.4
Fe VIII	185.216	sw	Low Corona	5.6
Si VII^*	275.35	lw	Corona	5.8
Mg VII^*	278.395	lw	Corona	5.8
Fe X^*	184.543	sw	Corona	6.0
Fe XII	186.880	sw	Corona	6.2
Fe XII^*	195.119	sw	Corona	6.2
Si X^*	261.056	lw	Corona	6.2
Fe XIII^*	202.044	sw	Corona	6.2
Fe XV^*	284.160	lw	Hot Corona	6.4
Fe XVI^*	262.984	lw	Hot Corona	6.8

Notes. TR refers to the transition region while SW and LW refer to the short and long wavebands of the EIS CCDs. The approximate temperature T_max of line formation is also shown.

indicates that these lines were used in the Emission Measure Loci discussed in Sect. 3.1.

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