SDO HMI 2014-10-02 07:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.82 | 95.21 | 11.51 | 55.52 | -9.80 | 140.44 | -27.25 | 120.96 | 0.5282 | 693.4 | 425.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.11 | 0.00 | 1.24 | -11.71 | 141.15 | -26.54 | 124.72 | 0.5343 | 432.0 | 424.5 | |
| 0.00 | 0.70 | 0.00 | 0.41 | -11.90 | 141.10 | -26.59 | 124.97 | 0.5366 | 695.0 | 577.2 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -11.99 | 140.64 | -27.05 | 124.64 | 0.5428 | 687.0 | 589.4 | |
| 3.08 | 85.62 | 1.78 | 49.79 | -9.10 | 140.72 | -26.97 | 120.05 | 0.5195 | 1071.4 | 462.8 | |
| 3.52 | -4.00 | 2.05 | -4.00 | -9.60 | 140.60 | -27.09 | 120.79 | 0.5247 | 1233.6 | 999999 | |
| 6.08 | -4.00 | 3.53 | -4.00 | -9.32 | 140.59 | -27.10 | 120.31 | 0.5227 | 1002.0 | 999999 | |
| 3.35 | -4.00 | 1.95 | -4.00 | -10.01 | 140.50 | -27.19 | 121.37 | 0.5291 | 967.3 | 999999 | |
| 2.38 | -4.00 | 1.38 | -4.00 | -9.76 | 140.52 | -27.17 | 120.98 | 0.5269 | 1186.6 | 999999 | |
| 1.41 | -4.00 | 0.82 | -4.00 | -9.74 | 140.32 | -27.37 | 120.75 | 0.5294 | 815.7 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -11.52 | 139.93 | -27.76 | 123.23 | 0.5477 | 938.0 | 817.0 | |
| 0.00 | 1.15 | 0.00 | 0.68 | -12.86 | 139.67 | -28.02 | 125.03 | 0.5614 | 715.0 | 575.7 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -12.56 | 137.74 | -29.95 | 122.81 | 0.5820 | -773.0 | -645.5 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -12.34 | 136.69 | -31.00 | 121.60 | 0.5928 | -769.0 | -750.1 | |
| 0.00 | 1.50 | 0.00 | 0.92 | -12.54 | 136.52 | -31.17 | 121.75 | 0.5963 | -563.0 | -510.0 | |
| 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. | |