SDO HMI 2014-10-10 22:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.34 | 432.53 | 46.43 | 298.50 | -20.57 | 18.23 | -35.65 | 128.32 | 0.6979 | 911.2 | 272.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.83 | -21.16 | 20.45 | -33.43 | 130.75 | 0.6806 | -363.0 | -421.4 | |
| 0.00 | 1.58 | 0.00 | 1.04 | -18.93 | 20.58 | -33.31 | 128.13 | 0.6627 | 946.0 | 706.4 | |
| 0.00 | 0.88 | 0.00 | 0.58 | -19.57 | 20.27 | -33.61 | 128.68 | 0.6705 | 677.0 | 519.9 | |
| 0.00 | 2.54 | 0.00 | 1.68 | -18.68 | 20.33 | -33.56 | 127.62 | 0.6634 | 856.0 | 690.4 | |
| 0.00 | 0.70 | 0.00 | 0.47 | -19.19 | 19.64 | -34.25 | 127.70 | 0.6741 | 652.0 | 490.2 | |
| 0.00 | 0.96 | 0.00 | 0.67 | -22.46 | 18.65 | -35.24 | 130.85 | 0.7073 | -777.0 | -650.7 | |
| 0.00 | 0.61 | 0.00 | 0.41 | -19.09 | 19.51 | -34.38 | 127.49 | 0.6748 | 632.0 | 449.4 | |
| 2.01 | 414.75 | 1.37 | 286.21 | -20.34 | 19.16 | -34.73 | 128.74 | 0.6872 | 1124.8 | 280.2 | |
| 0.35 | 2.71 | 0.23 | 1.79 | -17.56 | 19.48 | -34.41 | 125.53 | 0.6643 | 740.0 | 635.5 | |
| 64.98 | -8.00 | 44.83 | -8.00 | -20.60 | 18.22 | -35.66 | 128.35 | 0.6982 | 1175.0 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.53 | -17.52 | 18.06 | -35.82 | 124.43 | 0.6790 | 605.0 | 488.0 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -19.29 | 16.95 | -36.93 | 125.85 | 0.7020 | -504.0 | -470.8 | |
| 0.00 | 1.93 | 0.00 | 1.47 | -24.24 | 13.62 | -40.27 | 129.34 | 0.7644 | -138.0 | -221.9 | |
| 0.00 | 1.31 | 0.00 | 0.94 | -19.48 | 15.17 | -38.72 | 124.87 | 0.7210 | -700.0 | -623.9 | |
| 0.00 | 0.79 | 0.00 | 0.60 | -22.76 | 12.88 | -41.00 | 127.22 | 0.7621 | -631.0 | -545.1 | |
| 0.00 | 0.79 | 0.00 | 0.59 | -21.75 | 13.20 | -40.69 | 126.27 | 0.7534 | -108.0 | -149.7 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -17.83 | 10.92 | -42.96 | 120.32 | 0.7539 | -301.0 | -378.3 | |
| 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. | |