SDO HMI 2014-11-03 10:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.91 | 53.88 | 9.24 | 32.35 | 5.70 | 69.61 | -34.35 | 85.93 | 0.5639 | -206.1 | 130.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.37 | 27.85 | 1.95 | 16.09 | 5.65 | 73.10 | -30.86 | 85.91 | 0.5138 | -1151.3 | -678.8 | |
| 8.56 | -1.00 | 4.95 | -1.00 | 5.82 | 72.92 | -31.04 | 85.59 | 0.5166 | -948.4 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.70 | 5.22 | 72.81 | -31.15 | 86.75 | 0.5180 | -720.0 | -596.1 | |
| 3.29 | -1.00 | 1.90 | -1.00 | 5.54 | 72.69 | -31.27 | 86.13 | 0.5199 | -768.2 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 5.05 | 71.34 | -32.62 | 87.10 | 0.5398 | -671.0 | -534.2 | |
| 0.00 | 0.78 | 0.00 | 0.48 | 5.45 | 67.87 | -36.09 | 86.43 | 0.5897 | -500.0 | -393.1 | |
| 0.00 | 1.47 | 0.00 | 0.91 | 6.07 | 67.01 | -36.95 | 85.41 | 0.6020 | 801.0 | 676.8 | |
| 0.00 | 1.04 | 0.00 | 0.64 | 6.24 | 66.81 | -37.15 | 85.13 | 0.6048 | 714.0 | 606.5 | |
| 0.00 | 3.63 | 0.00 | 2.27 | 6.03 | 66.14 | -37.82 | 85.50 | 0.6139 | 667.0 | 496.6 | |
| 0.00 | 1.12 | 0.00 | 0.71 | 7.01 | 66.06 | -37.90 | 83.90 | 0.6155 | 503.0 | 494.8 | |
| 0.00 | 8.22 | 0.00 | 5.15 | 5.55 | 65.99 | -37.97 | 86.29 | 0.6159 | 913.0 | 713.8 | |
| 0.00 | 2.51 | 0.00 | 1.58 | 5.09 | 65.79 | -38.17 | 87.03 | 0.6186 | 791.0 | 633.4 | |
| 0.69 | 4.58 | 0.44 | 2.93 | 5.55 | 64.69 | -39.27 | 86.30 | 0.6337 | 802.0 | 630.4 | |
| 0.00 | 0.52 | 0.00 | 0.33 | 6.23 | 64.51 | -39.45 | 85.23 | 0.6361 | 575.0 | 433.3 | |
| 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. | |