SDO HMI 2014-08-09 08:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 139.97 | 708.94 | 82.42 | 416.69 | 12.29 | 128.16 | -32.20 | 76.60 | 0.5371 | -105.3 | -44.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.09 | 364.24 | 34.17 | 207.20 | 14.07 | 131.51 | -28.85 | 72.45 | 0.4928 | -1257.8 | -401.8 | |
| 2.89 | -1.00 | 1.65 | -1.00 | 14.42 | 131.03 | -29.33 | 71.97 | 0.5009 | -748.0 | 999999 | |
| 1.90 | -1.00 | 1.08 | -1.00 | 13.95 | 130.95 | -29.41 | 72.91 | 0.5005 | -773.7 | 999999 | |
| 2.71 | -1.00 | 1.55 | -1.00 | 13.85 | 130.82 | -29.54 | 73.16 | 0.5021 | -704.4 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 16.11 | 130.30 | -30.06 | 69.06 | 0.5173 | -751.0 | -591.6 | |
| 0.81 | 3.25 | 0.47 | 1.89 | 13.68 | 129.43 | -30.93 | 73.99 | 0.5216 | -800.1 | -562.4 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 12.86 | 129.00 | -31.36 | 75.68 | 0.5257 | -605.0 | -470.4 | |
| 0.00 | 5.51 | 0.00 | 3.25 | 12.11 | 127.60 | -32.76 | 77.44 | 0.5442 | 994.0 | 816.7 | |
| 0.63 | 2.71 | 0.37 | 1.61 | 11.22 | 127.05 | -33.31 | 79.17 | 0.5506 | -771.7 | -603.0 | |
| 0.45 | 2.62 | 0.27 | 1.56 | 11.83 | 126.52 | -33.84 | 78.17 | 0.5591 | 866.0 | 783.2 | |
| 0.00 | 0.72 | 0.00 | 0.43 | 11.24 | 126.41 | -33.95 | 79.24 | 0.5597 | -320.0 | -252.8 | |
| 0.45 | 2.98 | 0.27 | 1.78 | 9.94 | 126.16 | -34.20 | 81.59 | 0.5618 | 941.4 | 778.1 | |
| 0.00 | 1.17 | 0.00 | 0.71 | 12.13 | 125.83 | -34.53 | 77.78 | 0.5691 | 566.0 | 443.7 | |
| 2.71 | 316.71 | 1.63 | 192.83 | 11.81 | 125.73 | -34.63 | 78.34 | 0.5701 | -793.4 | 325.7 | |
| 2.26 | -14.00 | 1.36 | -14.00 | 11.63 | 125.68 | -34.68 | 78.68 | 0.5705 | -239.6 | 999999 | |
| 0.00 | 2.62 | 0.00 | 1.59 | 11.56 | 125.16 | -35.20 | 78.88 | 0.5778 | 342.0 | 368.8 | |
| 0.00 | 2.08 | 0.00 | 1.25 | 9.80 | 125.35 | -35.01 | 81.92 | 0.5732 | 414.0 | 404.0 | |
| 3.89 | -14.00 | 2.35 | -14.00 | 10.13 | 125.27 | -35.09 | 81.35 | 0.5745 | 1042.2 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.76 | 9.58 | 125.34 | -35.02 | 82.30 | 0.5732 | 370.0 | 359.6 | |
| 11.75 | -14.00 | 7.12 | -14.00 | 10.70 | 125.05 | -35.31 | 80.39 | 0.5782 | 1175.8 | 999999 | |
| 4.52 | -14.00 | 2.74 | -14.00 | 10.42 | 124.97 | -35.39 | 80.88 | 0.5790 | 1021.9 | 999999 | |
| 1.90 | -14.00 | 1.15 | -14.00 | 9.99 | 124.99 | -35.37 | 81.62 | 0.5784 | 946.1 | 999999 | |
| 21.05 | -14.00 | 12.84 | -14.00 | 10.57 | 124.49 | -35.87 | 80.67 | 0.5859 | 901.0 | 999999 | |
| 19.34 | -14.00 | 11.79 | -14.00 | 9.90 | 124.50 | -35.86 | 81.82 | 0.5851 | 981.8 | 999999 | |
| 2.62 | -14.00 | 1.61 | -14.00 | 10.27 | 124.04 | -36.33 | 81.24 | 0.5920 | -335.5 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.68 | 10.59 | 122.83 | -37.53 | 80.82 | 0.6088 | -676.0 | -580.6 | |
| 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. | |