SDO HMI 2014-09-25 21:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 142.38 | 504.57 | 76.02 | 270.44 | -11.20 | 263.87 | 11.50 | 211.46 | 0.3818 | 195.4 | 58.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.71 | 0.00 | 0.40 | -7.07 | 276.88 | 24.52 | 240.66 | 0.4743 | 764.0 | 601.1 | |
| 0.00 | 1.77 | 0.00 | 0.99 | -9.22 | 275.72 | 23.35 | 235.52 | 0.4766 | 739.0 | 583.8 | |
| 0.00 | 2.65 | 0.00 | 1.48 | -10.12 | 273.70 | 21.34 | 231.45 | 0.4599 | 654.0 | 634.9 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -10.18 | 273.54 | 21.18 | 231.14 | 0.4585 | 846.0 | 724.8 | |
| 0.00 | 1.59 | 0.00 | 0.88 | -8.51 | 273.34 | 20.98 | 233.85 | 0.4403 | 806.0 | 580.6 | |
| 0.00 | 0.71 | 0.00 | 0.39 | -9.92 | 273.36 | 21.00 | 231.35 | 0.4538 | 711.0 | 602.2 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -11.57 | 272.92 | 20.56 | 227.97 | 0.4651 | 712.0 | 579.6 | |
| 0.00 | 1.15 | 0.00 | 0.63 | -10.53 | 271.61 | 19.25 | 227.81 | 0.4393 | 651.0 | 491.5 | |
| 13.60 | 137.61 | 7.37 | 74.58 | -8.55 | 270.73 | 18.36 | 230.02 | 0.4083 | 1206.8 | 371.3 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -6.97 | 270.59 | 18.23 | 232.94 | 0.3907 | -670.0 | -533.8 | |
| 14.93 | -9.00 | 8.08 | -9.00 | -8.66 | 270.35 | 17.98 | 229.22 | 0.4048 | 1255.4 | 999999 | |
| 0.00 | 1.77 | 0.00 | 0.95 | -8.83 | 269.84 | 17.48 | 228.09 | 0.4006 | 889.0 | 774.0 | |
| 0.00 | 2.21 | 0.00 | 1.19 | -8.38 | 269.50 | 17.14 | 228.38 | 0.3917 | 947.0 | 777.5 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -8.41 | 269.31 | 16.95 | 228.01 | 0.3897 | 880.0 | 684.7 | |
| 21.55 | 56.97 | 11.60 | 30.64 | -8.90 | 269.18 | 16.81 | 226.84 | 0.3935 | 1083.7 | 561.5 | |
| 1.24 | -15.00 | 0.66 | -15.00 | -8.64 | 268.82 | 16.45 | 226.71 | 0.3864 | 1129.8 | 999999 | |
| 2.74 | -15.00 | 1.47 | -15.00 | -8.79 | 268.79 | 16.43 | 226.37 | 0.3878 | 1103.0 | 999999 | |
| 0.71 | 6.98 | 0.38 | 3.79 | -10.87 | 268.90 | 16.53 | 222.87 | 0.4125 | 883.2 | 806.9 | |
| 1.15 | -15.00 | 0.62 | -15.00 | -8.57 | 268.62 | 16.26 | 226.50 | 0.3833 | 1091.5 | 999999 | |
| 0.00 | 4.86 | 0.00 | 2.59 | -7.88 | 268.53 | 16.17 | 227.68 | 0.3747 | 966.0 | 804.6 | |
| 0.00 | 3.36 | 0.00 | 1.80 | -8.34 | 268.42 | 16.06 | 226.58 | 0.3785 | 938.0 | 814.2 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -8.74 | 268.28 | 15.92 | 225.56 | 0.3814 | 936.0 | 706.9 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -8.86 | 268.19 | 15.83 | 225.17 | 0.3817 | 882.0 | 640.6 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -9.76 | 267.89 | 15.52 | 222.96 | 0.3886 | 909.0 | 731.5 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -15.22 | 267.38 | 15.02 | 213.80 | 0.4513 | 712.0 | 639.1 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -15.80 | 266.04 | 13.67 | 210.68 | 0.4476 | 620.0 | 604.3 | |
| 0.00 | 1.77 | 0.00 | 0.93 | -9.14 | 265.25 | 12.89 | 218.77 | 0.3532 | -818.0 | -751.5 | |
| 0.00 | 2.74 | 0.00 | 1.44 | -9.39 | 263.95 | 11.59 | 215.40 | 0.3436 | -770.0 | -743.2 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -9.58 | 263.96 | 11.59 | 215.09 | 0.3462 | -621.0 | -552.2 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -11.35 | 263.21 | 10.85 | 210.60 | 0.3640 | -701.0 | -545.4 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -11.00 | 263.01 | 10.65 | 210.64 | 0.3574 | -796.0 | -652.7 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -11.05 | 262.64 | 10.27 | 209.68 | 0.3551 | -902.0 | -699.4 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -4.25 | 261.38 | 9.02 | 219.03 | 0.2493 | 762.0 | 644.2 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -13.18 | 261.09 | 8.73 | 203.31 | 0.3749 | -686.0 | -681.8 | |
| 0.00 | 1.50 | 0.00 | 0.80 | -13.31 | 260.94 | 8.58 | 202.82 | 0.3758 | -951.0 | -761.6 | |
| 0.62 | 3.18 | 0.33 | 1.71 | -14.75 | 260.55 | 8.19 | 200.50 | 0.3951 | 881.7 | 690.5 | |
| 0.00 | 3.00 | 0.00 | 1.63 | -15.49 | 260.14 | 7.78 | 198.91 | 0.4040 | 855.0 | 636.7 | |
| 0.00 | 2.56 | 0.00 | 1.36 | -12.42 | 259.33 | 6.96 | 199.70 | 0.3528 | -902.0 | -709.0 | |
| 7.51 | 127.81 | 4.00 | 68.22 | -13.53 | 259.14 | 6.77 | 198.19 | 0.3690 | -1268.8 | -457.9 | |
| 0.53 | 3.62 | 0.28 | 1.92 | -12.69 | 258.84 | 6.47 | 198.15 | 0.3545 | -1015.2 | -864.2 | |
| 22.96 | -39.00 | 12.26 | -39.00 | -13.94 | 258.84 | 6.47 | 197.09 | 0.3740 | -1212.4 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -15.73 | 258.86 | 6.50 | 195.80 | 0.4016 | -796.0 | -570.0 | |
| 0.97 | 8.92 | 0.53 | 4.83 | -15.98 | 258.65 | 6.28 | 195.14 | 0.4047 | -980.8 | -763.5 | |
| 0.53 | -39.00 | 0.28 | -39.00 | -13.97 | 258.47 | 6.10 | 196.14 | 0.3726 | -853.3 | 999999 | |
| 0.00 | 1.85 | 0.00 | 1.00 | -16.21 | 258.31 | 5.94 | 194.21 | 0.4067 | -783.0 | -633.2 | |
| 0.00 | 3.62 | 0.00 | 1.91 | -12.30 | 258.18 | 5.81 | 196.74 | 0.3452 | 265.0 | 50.7 | |
| 24.20 | 54.41 | 12.69 | 28.54 | -11.35 | 257.88 | 5.52 | 196.74 | 0.3287 | 1127.6 | 420.3 | |
| 4.77 | -47.00 | 2.50 | -47.00 | -11.66 | 257.70 | 5.34 | 195.96 | 0.3328 | 896.4 | 999999 | |
| 0.88 | 6.09 | 0.47 | 3.23 | -13.18 | 257.33 | 4.97 | 193.77 | 0.3555 | 613.8 | -58.8 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -13.54 | 257.12 | 4.76 | 192.98 | 0.3603 | -435.0 | -472.8 | |
| 10.69 | 40.10 | 5.69 | 21.31 | -14.04 | 256.57 | 4.21 | 191.24 | 0.3665 | -952.2 | -741.6 | |
| 6.80 | -51.00 | 3.61 | -51.00 | -13.82 | 256.35 | 3.98 | 190.78 | 0.3622 | -1202.0 | 999999 | |
| 5.12 | -51.00 | 2.73 | -51.00 | -14.14 | 256.26 | 3.90 | 190.39 | 0.3671 | -1006.7 | 999999 | |
| 0.88 | -51.00 | 0.47 | -51.00 | -13.65 | 256.10 | 3.73 | 190.20 | 0.3588 | -1150.4 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -13.39 | 255.97 | 3.61 | 189.99 | 0.3543 | -840.0 | -575.8 | |
| 0.00 | 1.85 | 0.00 | 0.99 | -13.88 | 255.95 | 3.58 | 189.69 | 0.3620 | -829.0 | -635.9 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -7.93 | 254.55 | 2.18 | 188.36 | 0.2606 | 866.0 | 631.2 | |
| 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. | |