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Table 1

List of the emission lines and intensities used in the EIS DEM analysis for the active region, quiet Sun and flare cases.

Ion λ Transition log Tma AR QS FL1 FL2 FL3
Å K

O V 192.91 2s2p 3P2–2s3d 3D3 5.4 440 7.7
O V 248.46 2s2p 1P1–2s3s 1S0 5.4 389 39
Mg V 276.58 2s22p41D2–2s2p51P1 5.4 104 5
Mg VI (2)b 270.39 2s22p32D5/2–2s2p42P3/2 5.6 382 22
2s22p32D3/2–2s2p42P3/2
Fe VIII 185.21 3s23p63d 2D5/2–3s23p53d22F7/2 5.7 1290 1490 899
Mg VII 278.4 2s22p23P2–2s2p33S1 5.8 988 108
Si VII 275.35 2s22p43P2–2s2p53P2 5.8 739 92 295
Fe X 184.54 3s23p52P3/2–3s23p43d 2S1/2 6.0 2240 365 1150 873 844
Fe XI 180.43 3s23p43P2–3s23p33d 3D3 6.1 6390 1210
Fe XI 188.22 3s23p43P2–3s23p33d 3P2 6.1 3730 430 2120 2350 1460
Fe XI 188.3 3s23p43P2–3s23p33d 1P1 6.1 1080 1040 964
Fe XII 192.39 3s23p34S3/2–3s2 3p23d 4P1/2 6.2 2190 207
Fe XII 195.12 3s23p34S3/2–3s2 3p23d 4P5/2 6.2 2730 2310 2150
Si X 256.4 2s22p 2P1/2–2s2p22P1/2 6.1 1820 1220 2380
Si X 261.06 2s22p 2P3/2–2s2p22P1/2 6.1 1080 104
Fe XIII 202.04 3s23p23P0–3s23p3d 3P1 6.2 3900 457 1530 1190 1120
Fe XIV 264.79 3s23p 2P3/2–3s3p22P3/2 6.3 830 4450 6210
Fe XIV 274.2 3s23p 2P1/2–3s3p22S1/2 6.3 5280 186 7030 2670 3990
Fe XV 284.16 3s21S0–3s3p 1P1 6.3 25 100 747 9180 26 400 45 300
Fe XVI 262.98 3p 2P3/2–3d 2D5/2 6.4 7190 23 1640 4890 12 200
Fe XVI 265.0 3p 2P3/2–3d 2D3/2 6.4 117 642 1090
Ca XV 200.98 2s22p23P0–2s2p33D1 6.6 774 3
Fe XVII 275.55 2s22p53p 1P1–2s22p53d 1D2 6.6 46 0.5
Fe XVII 284.39 2s22p53p 3D3–2s22p53d 3P2 6.6 110 646 410
Ca XVII 192.82 2s21S0–2s2p 1P1 6.7 823 4630 1780 976
Fe XXIII 263.77 2s21S0–2s2p 3P1 7.15 2.5 690 1730 0.3
Fe XXIV 192.03 1s22s 2S1/2–1s22p 2P3/2 7.25 857 658 81.8
Fe XXIV 255.11 1s22s 2S1/2–1s22p 2P1/2 7.25 2060 4870 82.0

Notes.

(a)

Tm corresponds to the temperature of maximum abundance.

(b)

Denotes a self blend. The numbers in the columns are the EIS calibrated intensities for the active region (AR), quiet Sun (QS) and three flare (FL1, FL2, FL3) cases discussed within the text.

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