SDO HMI 2011-10-11 06:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 120.63 | 464.07 | 64.06 | 246.51 | -14.64 | 118.38 | 3.55 | 189.55 | 0.3630 | 265.1 | 242.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.06 | 64.57 | 4.29 | 34.36 | -14.22 | 121.04 | 6.21 | 196.78 | 0.3646 | 1158.7 | 409.8 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -14.02 | 120.81 | 5.99 | 196.37 | 0.3605 | 917.0 | 775.0 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -13.93 | 120.69 | 5.86 | 196.12 | 0.3584 | 868.0 | 738.1 | |
| 12.18 | -1.00 | 6.48 | -1.00 | -14.50 | 120.61 | 5.78 | 195.47 | 0.3671 | 1077.6 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.70 | -14.85 | 120.49 | 5.67 | 194.92 | 0.3721 | 618.0 | 469.5 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -13.41 | 120.43 | 5.60 | 195.84 | 0.3492 | 964.0 | 673.5 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -15.14 | 120.38 | 5.55 | 194.43 | 0.3762 | 514.0 | 351.5 | |
| 0.00 | 3.68 | 0.00 | 1.95 | -13.86 | 120.28 | 5.45 | 195.11 | 0.3556 | 1046.0 | 732.9 | |
| 1.40 | 1.84 | 0.75 | 0.98 | -14.62 | 120.24 | 5.41 | 194.44 | 0.3675 | 871.1 | 829.2 | |
| 0.00 | 1.49 | 0.00 | 0.79 | -14.46 | 120.14 | 5.31 | 194.30 | 0.3646 | 1125.0 | 913.9 | |
| 0.00 | 1.75 | 0.00 | 0.93 | -15.04 | 120.06 | 5.23 | 193.71 | 0.3734 | -140.0 | -37.8 | |
| 1.75 | 5.17 | 0.93 | 2.74 | -14.01 | 119.95 | 5.12 | 194.10 | 0.3567 | 1052.7 | 845.1 | |
| 1.23 | 2.37 | 0.65 | 1.26 | -15.01 | 119.94 | 5.11 | 193.42 | 0.3724 | 626.7 | 400.2 | |
| 0.00 | 2.63 | 0.00 | 1.40 | -15.00 | 119.75 | 4.92 | 192.94 | 0.3716 | 619.0 | 553.2 | |
| 1.49 | 218.33 | 0.79 | 116.10 | -14.27 | 119.67 | 4.84 | 193.21 | 0.3596 | 1155.5 | 532.3 | |
| 0.00 | 1.66 | 0.00 | 0.88 | -13.72 | 119.60 | 4.77 | 193.38 | 0.3507 | 777.0 | 612.8 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -13.50 | 119.25 | 4.43 | 192.59 | 0.3458 | 962.0 | 740.1 | |
| 0.00 | 4.38 | 0.00 | 2.31 | -13.34 | 119.22 | 4.39 | 192.60 | 0.3432 | 916.0 | 810.5 | |
| 4.47 | -15.00 | 2.39 | -15.00 | -15.61 | 119.24 | 4.41 | 191.29 | 0.3795 | 722.8 | 999999 | |
| 45.56 | -15.00 | 24.23 | -15.00 | -14.74 | 119.16 | 4.33 | 191.57 | 0.3654 | 1263.0 | 999999 | |
| 2.10 | 7.80 | 1.11 | 4.11 | -13.43 | 118.73 | 3.90 | 191.17 | 0.3430 | 991.1 | 683.5 | |
| 3.68 | -15.00 | 1.96 | -15.00 | -14.96 | 118.38 | 3.55 | 189.44 | 0.3666 | 681.2 | 999999 | |
| 1.66 | -15.00 | 0.88 | -15.00 | -14.61 | 118.25 | 3.42 | 189.27 | 0.3606 | 730.3 | 999999 | |
| 0.00 | 2.54 | 0.00 | 1.34 | -13.77 | 117.65 | 2.83 | 188.00 | 0.3456 | 970.0 | 726.3 | |
| 0.00 | 23.92 | 0.00 | 12.64 | -14.12 | 117.44 | 2.61 | 187.27 | 0.3508 | 424.0 | 80.3 | |
| 0.00 | 1.75 | 0.00 | 0.92 | -13.74 | 117.38 | 2.55 | 187.23 | 0.3445 | 823.0 | 718.5 | |
| 0.00 | 3.42 | 0.00 | 1.82 | -14.95 | 117.36 | 2.53 | 186.76 | 0.3642 | 141.0 | 156.2 | |
| 0.00 | 1.31 | 0.00 | 0.70 | -14.41 | 117.35 | 2.52 | 186.93 | 0.3553 | -104.0 | -123.5 | |
| 0.00 | 1.84 | 0.00 | 0.97 | -13.52 | 117.16 | 2.33 | 186.70 | 0.3404 | 237.0 | 256.6 | |
| 4.29 | 11.13 | 2.27 | 5.90 | -14.47 | 116.89 | 2.06 | 185.65 | 0.3555 | -888.9 | -327.8 | |
| 1.58 | 13.14 | 0.84 | 6.99 | -15.18 | 116.77 | 1.94 | 185.14 | 0.3668 | -676.5 | -804.8 | |
| 0.00 | 1.93 | 0.00 | 1.02 | -14.31 | 116.70 | 1.87 | 185.18 | 0.3526 | -1004.0 | -717.1 | |
| 0.00 | 1.31 | 0.00 | 0.70 | -14.63 | 116.67 | 1.85 | 185.02 | 0.3578 | -196.0 | -174.7 | |
| 3.59 | -31.00 | 1.91 | -31.00 | -15.34 | 116.49 | 1.67 | 184.38 | 0.3690 | -860.2 | 999999 | |
| 0.00 | 2.63 | 0.00 | 1.39 | -14.47 | 116.30 | 1.47 | 184.04 | 0.3547 | -955.0 | -708.7 | |
| 1.93 | 5.52 | 1.02 | 2.93 | -14.72 | 116.18 | 1.35 | 183.66 | 0.3587 | -877.7 | -776.6 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -15.40 | 115.84 | 1.01 | 182.66 | 0.3694 | -677.0 | -621.8 | |
| 13.23 | 20.15 | 6.98 | 10.63 | -13.96 | 115.65 | 0.82 | 182.32 | 0.3457 | -1147.3 | -706.6 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -17.51 | 115.48 | 0.65 | 181.54 | 0.4033 | -593.0 | -489.9 | |
| 1.66 | 1.93 | 0.88 | 1.02 | -13.96 | 115.19 | 0.36 | 181.02 | 0.3455 | -820.9 | -640.8 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -14.15 | 115.03 | 0.21 | 180.57 | 0.3486 | -861.0 | -651.0 | |
| 0.00 | 1.40 | 0.00 | 0.75 | -16.92 | 115.01 | 0.18 | 180.43 | 0.3937 | -774.0 | -510.2 | |
| 1.75 | 4.99 | 0.92 | 2.63 | -13.80 | 114.97 | 0.14 | 180.41 | 0.3428 | -1066.0 | -629.1 | |
| 0.00 | 1.93 | 0.00 | 1.04 | -16.66 | 114.91 | 0.08 | 180.21 | 0.3895 | -847.0 | -690.4 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -15.14 | 114.79 | -0.04 | 179.89 | 0.3648 | -777.0 | -530.2 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -13.99 | 114.76 | -0.07 | 179.80 | 0.3459 | -817.0 | -666.7 | |
| 1.31 | 6.92 | 0.70 | 3.71 | -16.37 | 114.72 | -0.10 | 179.74 | 0.3848 | -883.5 | -815.4 | |
| 0.00 | 3.85 | 0.00 | 2.06 | -16.11 | 114.60 | -0.23 | 179.42 | 0.3806 | -1226.0 | -938.2 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -14.69 | 114.51 | -0.32 | 179.13 | 0.3575 | -861.0 | -646.1 | |
| 0.00 | 0.70 | 0.00 | 0.37 | -15.20 | 114.51 | -0.32 | 179.15 | 0.3659 | -739.0 | -598.0 | |
| 0.00 | 1.75 | 0.00 | 0.94 | -16.04 | 114.41 | -0.42 | 178.94 | 0.3796 | -811.0 | -701.5 | |
| 0.00 | 3.33 | 0.00 | 1.77 | -15.14 | 114.20 | -0.63 | 178.32 | 0.3650 | -912.0 | -799.7 | |
| 0.00 | 3.33 | 0.00 | 1.77 | -15.49 | 114.10 | -0.72 | 178.11 | 0.3708 | -850.0 | -764.8 | |
| 0.00 | 1.93 | 0.00 | 1.02 | -14.37 | 113.52 | -1.31 | 176.39 | 0.3529 | -1060.0 | -821.0 | |
| 7.71 | 11.48 | 4.08 | 6.07 | -14.31 | 113.21 | -1.62 | 175.53 | 0.3522 | -1059.2 | -645.4 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -16.27 | 112.60 | -2.22 | 174.42 | 0.3850 | -851.0 | -653.8 | |
| 0.00 | 0.61 | 0.00 | 0.33 | -17.32 | 112.56 | -2.27 | 174.58 | 0.4018 | -617.0 | -373.1 | |
| 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. | |