SDO HMI 2014-05-28 15:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.01 | 83.17 | 5.35 | 45.68 | -12.75 | 65.14 | 22.64 | 240.94 | 0.4303 | 202.2 | 247.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.72 | 10.92 | 0.41 | 6.19 | -13.64 | 69.17 | 26.68 | 243.33 | 0.4902 | -868.8 | -742.2 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -14.80 | 69.18 | 26.68 | 241.19 | 0.4975 | 834.0 | 735.0 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -14.02 | 68.73 | 26.23 | 242.26 | 0.4865 | -645.0 | -477.6 | |
| 0.00 | 2.35 | 0.00 | 1.31 | -11.82 | 68.31 | 25.81 | 246.21 | 0.4677 | 820.0 | 694.7 | |
| 0.00 | 2.89 | 0.00 | 1.61 | -11.08 | 68.14 | 25.64 | 247.59 | 0.4612 | 820.0 | 646.7 | |
| 0.00 | 2.26 | 0.00 | 1.26 | -11.67 | 68.16 | 25.66 | 246.41 | 0.4647 | 750.0 | 413.2 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -12.97 | 68.05 | 25.55 | 243.73 | 0.4707 | 271.0 | 313.0 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -9.97 | 67.70 | 25.20 | 249.59 | 0.4493 | 615.0 | 498.3 | |
| 1.26 | 3.52 | 0.71 | 1.97 | -12.75 | 67.75 | 25.26 | 243.91 | 0.4652 | 977.6 | 685.4 | |
| 0.00 | 6.59 | 0.00 | 3.65 | -11.21 | 67.36 | 24.86 | 246.74 | 0.4508 | 874.0 | 824.5 | |
| 0.00 | 2.44 | 0.00 | 1.35 | -11.42 | 67.21 | 24.71 | 246.17 | 0.4498 | 824.0 | 724.9 | |
| 0.00 | 2.17 | 0.00 | 1.20 | -11.12 | 67.01 | 24.51 | 246.66 | 0.4452 | 1010.0 | 916.4 | |
| 0.00 | 3.25 | 0.00 | 1.79 | -11.33 | 66.89 | 24.40 | 246.11 | 0.4448 | 862.0 | 729.8 | |
| 0.00 | 5.68 | 0.00 | 3.15 | -12.42 | 66.89 | 24.40 | 243.87 | 0.4512 | 921.0 | 733.0 | |
| 0.00 | 1.99 | 0.00 | 1.09 | -10.50 | 66.69 | 24.19 | 247.73 | 0.4372 | 789.0 | 721.5 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -17.68 | 67.12 | 24.62 | 234.13 | 0.4918 | 578.0 | 442.2 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -16.39 | 66.49 | 23.99 | 235.78 | 0.4736 | 495.0 | 366.5 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -14.61 | 65.11 | 22.61 | 237.72 | 0.4419 | 791.0 | 699.0 | |
| 0.00 | 0.81 | 0.00 | 0.44 | -12.03 | 64.79 | 22.29 | 242.77 | 0.4190 | 811.0 | 630.9 | |
| 0.00 | 1.71 | 0.00 | 0.93 | -12.00 | 64.35 | 21.86 | 242.39 | 0.4126 | 883.0 | 627.9 | |
| 0.00 | 1.99 | 0.00 | 1.07 | -11.60 | 63.85 | 21.36 | 242.78 | 0.4028 | 986.0 | 834.9 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -12.81 | 63.92 | 21.42 | 240.17 | 0.4123 | 779.0 | 699.5 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -11.85 | 63.51 | 21.01 | 241.85 | 0.3996 | 862.0 | 726.1 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -14.77 | 63.63 | 21.14 | 235.73 | 0.4237 | 768.0 | 616.3 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -12.53 | 63.39 | 20.90 | 240.20 | 0.4030 | 1003.0 | 796.2 | |
| 0.00 | 1.80 | 0.00 | 0.97 | -12.41 | 63.05 | 20.56 | 240.09 | 0.3973 | 1036.0 | 897.3 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -13.78 | 62.57 | 20.07 | 236.50 | 0.4014 | 762.0 | 658.5 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -14.22 | 61.54 | 19.05 | 234.22 | 0.3916 | -821.0 | -638.4 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -12.61 | 60.23 | 17.74 | 236.02 | 0.3601 | -711.0 | -576.8 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -12.89 | 60.06 | 17.56 | 235.10 | 0.3601 | -867.0 | -604.7 | |
| 0.81 | 3.07 | 0.43 | 1.62 | -11.62 | 59.87 | 17.38 | 237.91 | 0.3468 | -1025.4 | -881.0 | |
| 0.00 | 2.53 | 0.00 | 1.35 | -14.88 | 60.05 | 17.55 | 230.63 | 0.3786 | -581.0 | -458.4 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -13.76 | 59.63 | 17.13 | 232.44 | 0.3625 | -936.0 | -714.8 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -13.61 | 59.26 | 16.76 | 232.21 | 0.3562 | -927.0 | -702.9 | |
| 7.22 | 9.65 | 3.80 | 5.09 | -14.17 | 57.60 | 15.11 | 228.09 | 0.3411 | -1027.9 | -751.0 | |
| 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. | |