| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.98 | 299.30 | 45.01 | 163.13 | -11.01 | 186.89 | 24.01 | 254.20 | 0.4169 | 464.5 | 296.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.60 | 0.00 | 0.89 | -10.26 | 190.07 | 27.20 | 257.34 | 0.4629 | 530.0 | 463.2 | |
| 0.00 | 1.24 | 0.00 | 0.70 | -11.29 | 190.17 | 27.30 | 255.19 | 0.4671 | 567.0 | 450.6 | |
| 0.00 | 1.15 | 0.00 | 0.65 | -11.80 | 190.19 | 27.32 | 254.11 | 0.4690 | 751.0 | 582.6 | |
| 0.00 | 1.42 | 0.00 | 0.79 | -10.45 | 189.95 | 27.08 | 256.90 | 0.4615 | 757.0 | 637.2 | |
| 0.00 | 0.71 | 0.00 | 0.39 | -7.32 | 189.40 | 26.53 | 263.63 | 0.4476 | 578.0 | 443.6 | |
| 0.00 | 2.22 | 0.00 | 1.24 | -12.89 | 189.76 | 26.88 | 251.64 | 0.4663 | 635.0 | 574.6 | |
| 0.00 | 0.98 | 0.00 | 0.55 | -13.14 | 189.61 | 26.74 | 251.05 | 0.4651 | 749.0 | 631.5 | |
| 0.00 | 1.15 | 0.00 | 0.64 | -11.13 | 189.40 | 26.52 | 255.20 | 0.4551 | 613.0 | 495.5 | |
| 1.51 | 132.43 | 0.84 | 73.02 | -10.93 | 189.10 | 26.23 | 255.52 | 0.4500 | 736.8 | 579.2 | |
| 4.53 | -9.00 | 2.51 | -9.00 | -10.64 | 188.91 | 26.03 | 256.10 | 0.4462 | 909.4 | 999999 | |
| 12.88 | -9.00 | 7.11 | -9.00 | -10.77 | 188.61 | 25.74 | 255.68 | 0.4421 | 1186.0 | 999999 | |
| 10.75 | -9.00 | 5.92 | -9.00 | -10.11 | 188.52 | 25.64 | 257.14 | 0.4389 | 1202.5 | 999999 | |
| 7.02 | -9.00 | 3.86 | -9.00 | -10.39 | 188.30 | 25.43 | 256.42 | 0.4363 | 1213.8 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -14.09 | 188.55 | 25.67 | 248.42 | 0.4538 | 602.0 | 503.7 | |
| 0.00 | 2.84 | 0.00 | 1.57 | -13.83 | 188.21 | 25.33 | 248.76 | 0.4476 | 784.0 | 676.0 | |
| 0.00 | 1.33 | 0.00 | 0.74 | -13.10 | 188.09 | 25.22 | 250.27 | 0.4427 | 763.0 | 613.5 | |
| 4.09 | 8.62 | 2.24 | 4.73 | -11.37 | 187.88 | 25.01 | 254.00 | 0.4330 | 882.2 | 661.4 | |
| 0.00 | 3.38 | 0.00 | 1.85 | -10.31 | 187.79 | 24.92 | 256.38 | 0.4283 | 1096.0 | 863.4 | |
| 0.00 | 0.89 | 0.00 | 0.49 | -12.95 | 187.94 | 25.06 | 250.50 | 0.4398 | 664.0 | 573.4 | |
| 0.00 | 1.24 | 0.00 | 0.69 | -13.26 | 187.80 | 24.93 | 249.73 | 0.4391 | 672.0 | 574.9 | |
| 0.53 | 7.28 | 0.29 | 4.03 | -14.02 | 187.85 | 24.98 | 248.11 | 0.4434 | 1029.7 | 769.8 | |
| 0.00 | 3.29 | 0.00 | 1.79 | -8.81 | 187.37 | 24.50 | 259.75 | 0.4182 | 840.0 | 683.1 | |
| 0.00 | 2.04 | 0.00 | 1.13 | -13.51 | 187.76 | 24.89 | 249.17 | 0.4396 | 787.0 | 637.5 | |
| 0.00 | 1.51 | 0.00 | 0.83 | -12.87 | 187.66 | 24.78 | 250.51 | 0.4353 | 844.0 | 667.8 | |
| 0.00 | 0.80 | 0.00 | 0.44 | -10.18 | 187.37 | 24.50 | 256.53 | 0.4215 | 795.0 | 663.6 | |
| 0.00 | 1.42 | 0.00 | 0.77 | -9.22 | 187.10 | 24.22 | 258.70 | 0.4148 | 955.0 | 854.5 | |
| 0.00 | 1.24 | 0.00 | 0.68 | -8.22 | 187.03 | 24.16 | 261.08 | 0.4117 | 733.0 | 606.6 | |
| 0.00 | 5.60 | 0.00 | 3.05 | -10.61 | 187.14 | 24.27 | 255.41 | 0.4192 | 857.0 | 815.4 | |
| 0.71 | 4.00 | 0.39 | 2.18 | -11.15 | 187.15 | 24.28 | 254.14 | 0.4211 | -847.6 | -524.4 | |
| 1.42 | 5.33 | 0.77 | 2.90 | -11.41 | 186.91 | 24.03 | 253.42 | 0.4183 | -905.9 | -763.8 | |
| 0.00 | 1.42 | 0.00 | 0.78 | -11.71 | 186.93 | 24.06 | 252.73 | 0.4198 | 316.0 | 366.6 | |
| 0.00 | 0.44 | 0.00 | 0.24 | -10.44 | 186.82 | 23.95 | 255.67 | 0.4138 | 533.0 | 458.0 | |
| 0.00 | 0.36 | 0.00 | 0.19 | -13.84 | 187.08 | 24.20 | 247.99 | 0.4312 | 202.0 | 435.5 | |
| 0.00 | 0.53 | 0.00 | 0.29 | -14.02 | 187.03 | 24.16 | 247.55 | 0.4314 | 749.0 | 663.2 | |
| 1.15 | -30.00 | 0.63 | -30.00 | -11.56 | 186.72 | 23.84 | 252.95 | 0.4160 | -807.8 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -10.63 | 186.64 | 23.76 | 255.13 | 0.4115 | 773.0 | 537.2 | |
| 0.00 | 1.07 | 0.00 | 0.58 | -13.86 | 186.40 | 23.53 | 247.45 | 0.4214 | 843.0 | 689.8 | |
| 0.00 | 0.98 | 0.00 | 0.53 | -11.09 | 185.51 | 22.63 | 253.41 | 0.3957 | -531.0 | -437.2 | |
| 9.68 | 48.41 | 5.20 | 25.93 | -11.16 | 185.01 | 22.14 | 252.93 | 0.3884 | -896.5 | -732.9 | |
| 1.07 | 2.13 | 0.57 | 1.15 | -11.74 | 185.06 | 22.19 | 251.53 | 0.3915 | -734.5 | -588.2 | |
| 0.00 | 0.98 | 0.00 | 0.52 | -10.08 | 184.77 | 21.89 | 255.55 | 0.3807 | -773.0 | -628.5 | |
| 1.07 | -39.00 | 0.57 | -39.00 | -10.87 | 184.76 | 21.88 | 253.52 | 0.3834 | -861.7 | 999999 | |
| 1.69 | -39.00 | 0.90 | -39.00 | -11.05 | 184.71 | 21.83 | 253.03 | 0.3832 | -1135.9 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -8.18 | 184.52 | 21.64 | 260.45 | 0.3718 | 638.0 | 542.8 | |
| 0.00 | 1.24 | 0.00 | 0.67 | -15.26 | 184.86 | 21.99 | 243.01 | 0.4071 | 793.0 | 677.5 | |
| 5.60 | -39.00 | 2.99 | -39.00 | -10.88 | 184.40 | 21.52 | 253.28 | 0.3778 | -1053.4 | 999999 | |
| 0.00 | 1.24 | 0.00 | 0.66 | -9.35 | 183.90 | 21.02 | 257.05 | 0.3648 | -665.0 | -536.1 | |
| 1.51 | -39.00 | 0.80 | -39.00 | -10.87 | 183.83 | 20.96 | 252.95 | 0.3690 | -1100.7 | 999999 | |
| 0.00 | 2.66 | 0.00 | 1.42 | -10.44 | 183.80 | 20.93 | 254.06 | 0.3669 | -813.0 | -676.4 | |
| 0.00 | 4.44 | 0.00 | 2.36 | -9.57 | 183.49 | 20.61 | 256.23 | 0.3589 | -785.0 | -598.2 | |
| 0.00 | 3.20 | 0.00 | 1.69 | -7.58 | 183.34 | 20.47 | 261.73 | 0.3518 | -811.0 | -757.5 | |
| 0.00 | 3.46 | 0.00 | 1.83 | -10.22 | 183.07 | 20.19 | 254.20 | 0.3546 | -513.0 | -550.2 | |
| 7.73 | 27.62 | 4.10 | 14.66 | -12.29 | 182.86 | 19.98 | 248.45 | 0.3606 | 1139.0 | 699.8 | |
| 5.15 | -53.00 | 2.73 | -53.00 | -12.63 | 182.72 | 19.85 | 247.43 | 0.3603 | 1007.1 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -9.69 | 182.48 | 19.61 | 255.32 | 0.3435 | -1049.0 | -839.1 | |
| 4.89 | -53.00 | 2.59 | -53.00 | -12.42 | 182.60 | 19.73 | 247.88 | 0.3574 | 1295.6 | 999999 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -15.15 | 176.87 | 13.99 | 232.58 | 0.2951 | 798.0 | 682.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |