SDO HMI 2014-10-03 17:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.51 | 81.76 | 15.34 | 86.54 | 7.00 | 211.50 | 62.49 | 274.44 | 0.8843 | -68.4 | 2.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.03 | 51.52 | 7.83 | 57.38 | 7.16 | 213.13 | 64.13 | 274.74 | 0.8977 | -621.2 | -145.4 | |
| 2.29 | -1.00 | 2.51 | -1.00 | 7.08 | 212.70 | 63.69 | 274.62 | 0.8944 | -792.3 | 999999 | |
| 0.00 | 0.97 | 0.00 | 1.02 | 7.11 | 211.49 | 62.49 | 274.57 | 0.8848 | -504.0 | -486.5 | |
| 0.00 | 1.58 | 0.00 | 1.66 | 7.20 | 211.25 | 62.24 | 274.65 | 0.8828 | -527.0 | -590.8 | |
| 0.00 | 1.23 | 0.00 | 1.20 | 6.71 | 208.93 | 59.92 | 273.92 | 0.8635 | 203.0 | 66.0 | |
| 0.00 | 0.88 | 0.00 | 0.86 | 7.28 | 208.93 | 59.93 | 274.58 | 0.8632 | 72.0 | 20.1 | |
| 0.00 | 2.02 | 0.00 | 1.96 | 7.09 | 208.71 | 59.70 | 274.35 | 0.8613 | 263.0 | 176.8 | |
| 4.75 | 7.12 | 4.58 | 6.86 | 6.27 | 208.48 | 59.48 | 273.37 | 0.8598 | 483.3 | 292.1 | |
| 0.44 | 1.23 | 0.42 | 1.19 | 6.62 | 208.55 | 59.55 | 273.79 | 0.8602 | 251.8 | 204.0 | |
| 0.00 | 0.70 | 0.00 | 0.68 | 7.24 | 208.44 | 59.43 | 274.50 | 0.8589 | 372.0 | 358.1 | |
| 0.00 | 1.41 | 0.00 | 1.34 | 6.47 | 207.98 | 58.98 | 273.57 | 0.8552 | 465.0 | 409.9 | |
| 0.00 | 1.14 | 0.00 | 1.09 | 7.75 | 208.14 | 59.13 | 275.08 | 0.8559 | 253.0 | 238.7 | |
| 0.00 | 10.11 | 0.00 | 9.56 | 6.79 | 207.81 | 58.81 | 273.93 | 0.8535 | 719.0 | 571.5 | |
| 0.00 | 0.79 | 0.00 | 0.75 | 5.90 | 207.64 | 58.64 | 272.87 | 0.8525 | 421.0 | 351.1 | |
| 0.00 | 1.06 | 0.00 | 0.99 | 6.48 | 207.57 | 58.57 | 273.55 | 0.8515 | 674.0 | 485.9 | |
| 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. | |