SDO HMI 2014-10-31 11:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.56 | 86.02 | 29.44 | 85.81 | -4.88 | 83.38 | -59.59 | 98.20 | 0.8697 | 391.6 | 245.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.87 | 0.00 | 0.82 | -5.50 | 85.34 | -57.64 | 99.24 | 0.8539 | -270.0 | -170.3 | |
| 0.00 | 0.61 | 0.00 | 0.58 | -4.43 | 85.09 | -57.88 | 97.96 | 0.8547 | 274.0 | 291.0 | |
| 1.91 | 67.22 | 1.82 | 65.79 | -4.81 | 84.82 | -58.16 | 98.35 | 0.8577 | -219.5 | 344.6 | |
| 0.00 | 1.13 | 0.00 | 1.08 | -3.62 | 84.62 | -58.35 | 96.94 | 0.8580 | 518.0 | 396.0 | |
| 0.00 | 0.87 | 0.00 | 0.84 | -5.56 | 84.30 | -58.67 | 99.14 | 0.8632 | 339.0 | 291.9 | |
| 3.21 | -3.00 | 3.12 | -3.00 | -5.20 | 84.30 | -58.68 | 98.72 | 0.8627 | 606.0 | 999999 | |
| 0.00 | 1.21 | 0.00 | 1.22 | -6.79 | 83.54 | -59.43 | 100.41 | 0.8713 | -528.0 | -492.3 | |
| 21.40 | -3.00 | 21.03 | -3.00 | -4.66 | 83.85 | -59.12 | 98.03 | 0.8659 | 655.4 | 999999 | |
| 0.00 | 4.59 | 0.00 | 4.54 | -3.84 | 83.55 | -59.43 | 97.04 | 0.8676 | 265.0 | 227.6 | |
| 0.00 | 0.43 | 0.00 | 0.43 | -5.27 | 83.23 | -59.75 | 98.63 | 0.8720 | 194.0 | 232.0 | |
| 1.39 | 3.81 | 1.40 | 3.84 | -4.72 | 82.95 | -60.02 | 97.95 | 0.8737 | 222.9 | 43.8 | |
| 0.00 | 0.43 | 0.00 | 0.55 | -8.09 | 77.14 | -65.84 | 100.76 | 0.9212 | -362.0 | -353.4 | |
| 0.00 | 1.73 | 0.00 | 2.19 | -6.92 | 76.89 | -66.08 | 99.47 | 0.9217 | -415.0 | -284.4 | |
| 1.65 | 3.12 | 2.07 | 3.93 | -6.56 | 76.92 | -66.05 | 99.08 | 0.9212 | -264.1 | -220.8 | |
| 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. | |