SDO HMI 2014-12-01 12:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.76 | 139.37 | 38.52 | 226.00 | -13.88 | 165.19 | 71.43 | 255.12 | 0.9533 | 383.7 | 138.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.31 | 19.14 | 4.33 | 36.27 | -12.25 | 167.93 | 74.16 | 257.05 | 0.9658 | 351.3 | 32.4 | |
| 0.77 | -1.00 | 1.46 | -1.00 | -12.40 | 167.93 | 74.17 | 256.90 | 0.9659 | 342.3 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.42 | -11.49 | 165.71 | 71.94 | 257.67 | 0.9550 | 264.0 | 188.0 | |
| 0.00 | 1.20 | 0.00 | 1.98 | -11.70 | 165.74 | 71.98 | 257.45 | 0.9553 | 355.0 | 257.3 | |
| 0.00 | 1.79 | 0.00 | 2.92 | -11.37 | 165.53 | 71.77 | 257.79 | 0.9541 | 377.0 | 334.6 | |
| 1.20 | 113.13 | 1.91 | 179.29 | -13.67 | 164.94 | 71.18 | 255.32 | 0.9521 | 111.2 | 169.0 | |
| 3.67 | -6.00 | 5.88 | -6.00 | -13.91 | 164.93 | 71.16 | 255.07 | 0.9522 | 164.8 | 999999 | |
| 14.44 | -6.00 | 22.88 | -6.00 | -14.37 | 164.69 | 70.93 | 254.57 | 0.9512 | 597.2 | 999999 | |
| 1.03 | -6.00 | 1.62 | -6.00 | -14.89 | 164.52 | 70.75 | 254.00 | 0.9506 | 640.9 | 999999 | |
| 0.00 | 1.37 | 0.00 | 1.83 | -12.55 | 161.36 | 67.59 | 256.14 | 0.9311 | -370.0 | -322.1 | |
| 0.00 | 0.68 | 0.00 | 0.99 | -15.63 | 162.81 | 69.05 | 253.03 | 0.9418 | 173.0 | 81.9 | |
| 0.00 | 0.77 | 0.00 | 0.99 | -14.45 | 160.00 | 66.24 | 253.93 | 0.9240 | -543.0 | -478.8 | |
| 0.34 | 1.03 | 0.44 | 1.31 | -14.63 | 159.96 | 66.19 | 253.73 | 0.9238 | -483.2 | -431.1 | |
| 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. | |