SDO HMI 2014-11-01 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.23 | 88.76 | 22.28 | 70.37 | -4.54 | 84.13 | -50.58 | 99.41 | 0.7827 | 523.5 | 413.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.64 | 17.23 | 2.83 | 13.51 | -5.23 | 85.04 | -49.67 | 100.48 | 0.7743 | -398.5 | 270.4 | |
| 3.38 | -1.00 | 2.66 | -1.00 | -5.50 | 84.59 | -50.12 | 100.71 | 0.7797 | 708.3 | 999999 | |
| 0.00 | 1.30 | 0.00 | 1.03 | -5.72 | 84.42 | -50.29 | 100.96 | 0.7819 | 443.0 | 345.8 | |
| 3.55 | 63.30 | 2.80 | 50.10 | -4.70 | 84.44 | -50.27 | 99.66 | 0.7798 | 809.0 | 486.9 | |
| 8.57 | -4.00 | 6.76 | -4.00 | -4.37 | 84.29 | -50.42 | 99.22 | 0.7809 | 1002.0 | 999999 | |
| 4.33 | -4.00 | 3.43 | -4.00 | -4.05 | 84.08 | -50.63 | 98.78 | 0.7825 | 829.2 | 999999 | |
| 0.00 | 1.13 | 0.00 | 0.89 | -3.52 | 84.03 | -50.68 | 98.08 | 0.7822 | 319.0 | 339.7 | |
| 0.00 | 2.51 | 0.00 | 2.01 | -5.16 | 83.68 | -51.03 | 100.09 | 0.7887 | 467.0 | 289.6 | |
| 0.00 | 0.87 | 0.00 | 0.69 | -3.05 | 83.87 | -50.83 | 97.46 | 0.7831 | 540.0 | 426.0 | |
| 4.76 | -4.00 | 3.80 | -4.00 | -3.92 | 83.76 | -50.95 | 98.55 | 0.7857 | 614.5 | 999999 | |
| 0.00 | 1.21 | 0.00 | 1.02 | -5.26 | 81.62 | -53.09 | 99.78 | 0.8102 | 570.0 | 488.4 | |
| 0.00 | 0.26 | 0.00 | 0.24 | -6.52 | 78.40 | -56.30 | 100.65 | 0.8432 | -511.0 | -467.7 | |
| 0.00 | 0.69 | 0.00 | 0.63 | -5.52 | 78.46 | -56.25 | 99.48 | 0.8412 | -558.0 | -549.4 | |
| 0.00 | 0.26 | 0.00 | 0.25 | -8.30 | 77.10 | -57.61 | 102.46 | 0.8578 | -392.0 | -371.3 | |
| 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. | |