| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75.48 | 385.62 | 39.83 | 203.55 | 20.14 | 192.16 | 5.61 | 343.88 | 0.3458 | -98.5 | -191.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.57 | 233.04 | 11.86 | 122.66 | 18.98 | 194.72 | 8.17 | 336.35 | 0.3365 | -1495.5 | -445.8 | |
| 16.16 | -1.00 | 8.51 | -1.00 | 19.39 | 194.65 | 8.10 | 337.04 | 0.3421 | -1176.9 | 999999 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 22.57 | 194.47 | 7.92 | 340.82 | 0.3889 | -620.0 | -501.2 | |
| 2.48 | 6.75 | 1.30 | 3.53 | 18.61 | 193.89 | 7.33 | 338.08 | 0.3255 | -1099.5 | -692.4 | |
| 0.00 | 1.80 | 0.00 | 0.94 | 18.31 | 193.50 | 6.94 | 338.77 | 0.3184 | -769.0 | -611.0 | |
| 1.62 | 2.91 | 0.84 | 1.51 | 17.63 | 192.81 | 6.26 | 339.91 | 0.3039 | -920.2 | -869.9 | |
| 0.00 | 2.65 | 0.00 | 1.40 | 20.93 | 192.85 | 6.29 | 343.19 | 0.3556 | -906.0 | -742.2 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 21.15 | 192.79 | 6.24 | 343.51 | 0.3587 | -852.0 | -692.1 | |
| 0.00 | 1.80 | 0.00 | 0.94 | 19.80 | 192.71 | 6.15 | 342.52 | 0.3373 | -1064.0 | -800.5 | |
| 0.00 | 2.39 | 0.00 | 1.27 | 20.77 | 192.65 | 6.10 | 343.55 | 0.3522 | -904.0 | -727.2 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 18.52 | 192.50 | 5.95 | 341.81 | 0.3163 | -933.0 | -551.8 | |
| 0.00 | 2.05 | 0.00 | 1.08 | 20.21 | 192.03 | 5.47 | 344.69 | 0.3405 | -949.0 | -856.1 | |
| 0.00 | 2.22 | 0.00 | 1.17 | 20.55 | 191.97 | 5.42 | 345.11 | 0.3458 | -767.0 | -643.6 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 19.46 | 191.94 | 5.38 | 344.29 | 0.3283 | -879.0 | -724.1 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 19.89 | 191.92 | 5.37 | 344.71 | 0.3351 | -816.0 | -656.6 | |
| 4.27 | 5.30 | 2.25 | 2.79 | 20.21 | 191.61 | 5.06 | 345.79 | 0.3388 | -1011.1 | -823.4 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 20.27 | 191.30 | 4.75 | 346.68 | 0.3386 | -792.0 | -602.5 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 22.19 | 191.36 | 4.81 | 347.81 | 0.3694 | -779.0 | -547.6 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 19.30 | 190.74 | 4.18 | 347.55 | 0.3210 | -749.0 | -564.8 | |
| 0.00 | 1.71 | 0.00 | 0.90 | 19.62 | 190.56 | 4.00 | 348.29 | 0.3254 | -874.0 | -710.7 | |
| 0.00 | 3.25 | 0.00 | 1.71 | 20.27 | 190.51 | 3.96 | 348.84 | 0.3358 | -846.0 | -643.5 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 19.71 | 190.37 | 3.82 | 348.88 | 0.3263 | -923.0 | -761.2 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 19.90 | 190.28 | 3.73 | 349.25 | 0.3290 | -771.0 | -605.3 | |
| 0.00 | 2.48 | 0.00 | 1.30 | 19.71 | 190.09 | 3.53 | 349.68 | 0.3254 | -877.0 | -686.8 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 20.62 | 188.97 | 2.42 | 353.26 | 0.3375 | 875.0 | 697.6 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 22.16 | 188.55 | 1.99 | 354.87 | 0.3620 | 998.0 | 757.0 | |
| 7.35 | 9.23 | 3.88 | 4.88 | 21.37 | 188.31 | 1.76 | 355.27 | 0.3488 | 1028.1 | 736.4 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 20.43 | 187.99 | 1.43 | 355.94 | 0.3329 | -747.0 | -574.3 | |
| 0.00 | 1.88 | 0.00 | 1.00 | 22.93 | 187.76 | 1.20 | 357.02 | 0.3735 | 682.0 | 587.0 | |
| 0.00 | 1.88 | 0.00 | 1.00 | 21.72 | 187.65 | 1.10 | 357.11 | 0.3538 | 915.0 | 675.6 | |
| 0.00 | 3.33 | 0.00 | 1.76 | 21.06 | 187.55 | 1.00 | 357.27 | 0.3428 | 891.0 | 635.1 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 22.83 | 187.47 | 0.91 | 357.73 | 0.3717 | 808.0 | 629.2 | |
| 4.19 | 12.74 | 2.22 | 6.74 | 21.78 | 187.30 | 0.75 | 358.03 | 0.3546 | 1105.4 | 949.1 | |
| 0.94 | 9.23 | 0.50 | 4.90 | 22.26 | 187.11 | 0.56 | 358.57 | 0.3622 | 1030.8 | 803.9 | |
| 0.00 | 2.74 | 0.00 | 1.48 | 24.92 | 186.96 | 0.41 | 359.09 | 0.4052 | 833.0 | 720.6 | |
| 0.00 | 1.80 | 0.00 | 0.95 | 21.09 | 186.95 | 0.40 | 358.92 | 0.3430 | 965.0 | 724.6 | |
| 14.28 | 15.64 | 7.59 | 8.31 | 22.35 | 186.76 | 0.21 | 359.47 | 0.3637 | 974.3 | 718.1 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 24.95 | 186.67 | 0.11 | 359.75 | 0.4057 | 840.0 | 724.3 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 21.31 | 186.60 | 0.05 | 359.87 | 0.3466 | 986.0 | 811.7 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 21.97 | 186.44 | -0.11 | 0.29 | 0.3575 | 845.0 | 660.2 | |
| 0.00 | 3.16 | 0.00 | 1.67 | 21.31 | 186.44 | -0.11 | 0.30 | 0.3466 | 925.0 | 894.9 | |
| 0.00 | 3.16 | 0.00 | 1.67 | 21.50 | 186.25 | -0.30 | 0.81 | 0.3497 | 671.0 | 633.5 | |
| 0.00 | 3.25 | 0.00 | 1.73 | 22.61 | 185.99 | -0.56 | 1.41 | 0.3679 | 1014.0 | 804.9 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 22.89 | 185.99 | -0.56 | 1.40 | 0.3726 | 811.0 | 608.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 20.90 | 185.90 | -0.65 | 1.79 | 0.3400 | 882.0 | 758.1 | |
| 0.00 | 1.62 | 0.00 | 0.87 | 23.28 | 185.73 | -0.82 | 2.00 | 0.3789 | 753.0 | 567.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 20.78 | 185.71 | -0.84 | 2.33 | 0.3381 | 842.0 | 688.9 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 22.67 | 185.64 | -0.91 | 2.30 | 0.3692 | 786.0 | 678.7 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 25.66 | 185.52 | -1.03 | 2.24 | 0.4174 | 744.0 | 604.7 | |
| 0.00 | 3.16 | 0.00 | 1.69 | 22.96 | 185.48 | -1.08 | 2.66 | 0.3739 | 830.0 | 686.5 | |
| 0.00 | 2.48 | 0.00 | 1.33 | 23.25 | 185.44 | -1.11 | 2.71 | 0.3786 | 770.0 | 664.0 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 25.89 | 185.29 | -1.27 | 2.72 | 0.4212 | 593.0 | 512.7 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 23.31 | 184.86 | -1.69 | 4.11 | 0.3802 | 851.0 | 638.7 | |
| 1.62 | 3.93 | 0.88 | 2.14 | 25.30 | 184.74 | -1.82 | 4.00 | 0.4124 | 802.7 | 647.3 | |
| 0.00 | 2.14 | 0.00 | 1.15 | 24.43 | 184.59 | -1.97 | 4.51 | 0.3986 | 780.0 | 658.6 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 22.77 | 184.55 | -2.01 | 5.00 | 0.3718 | 778.0 | 562.7 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 24.59 | 184.45 | -2.10 | 4.78 | 0.4014 | 627.0 | 567.3 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 25.30 | 183.00 | -3.55 | 7.79 | 0.4152 | 614.0 | 595.4 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 21.09 | 182.48 | -4.08 | 10.99 | 0.3494 | 823.0 | 608.6 | |
| 0.00 | 0.51 | 0.00 | 0.29 | 27.92 | 180.63 | -5.92 | 11.42 | 0.4620 | 272.0 | 336.2 | |
| 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. | |