SDO HMI 2014-10-03 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.87 | 84.42 | 17.31 | 87.20 | 6.98 | 211.31 | 61.76 | 274.36 | 0.8783 | -81.7 | -27.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.03 | 50.03 | 7.68 | 54.57 | 7.19 | 213.07 | 63.52 | 274.73 | 0.8929 | -618.7 | -185.5 | |
| 2.37 | -1.00 | 2.56 | -1.00 | 7.08 | 212.70 | 63.15 | 274.58 | 0.8901 | -797.5 | 999999 | |
| 0.00 | 1.23 | 0.00 | 1.27 | 7.11 | 211.46 | 61.90 | 274.53 | 0.8800 | -548.0 | -481.7 | |
| 0.00 | 1.41 | 0.00 | 1.45 | 7.23 | 211.23 | 61.67 | 274.64 | 0.8781 | -538.0 | -560.4 | |
| 0.70 | 2.29 | 0.68 | 2.19 | 6.73 | 208.95 | 59.39 | 273.91 | 0.8588 | -34.2 | -138.2 | |
| 0.00 | 3.87 | 0.00 | 3.70 | 7.14 | 208.79 | 59.24 | 274.37 | 0.8572 | 125.0 | 130.8 | |
| 4.84 | 7.12 | 4.59 | 6.75 | 6.30 | 208.45 | 58.89 | 273.36 | 0.8545 | 488.1 | 254.9 | |
| 0.00 | 3.61 | 0.00 | 3.42 | 6.66 | 208.46 | 58.90 | 273.78 | 0.8544 | 402.0 | 219.2 | |
| 0.00 | 0.62 | 0.00 | 0.58 | 7.42 | 208.38 | 58.82 | 274.67 | 0.8533 | 332.0 | 285.0 | |
| 1.14 | 9.76 | 1.07 | 9.09 | 6.85 | 208.08 | 58.53 | 273.98 | 0.8509 | 447.3 | 584.2 | |
| 0.00 | 1.93 | 0.00 | 1.81 | 6.46 | 208.01 | 58.45 | 273.52 | 0.8505 | 562.0 | 396.6 | |
| 0.00 | 0.35 | 0.00 | 0.33 | 6.30 | 207.80 | 58.25 | 273.31 | 0.8487 | 288.0 | 385.5 | |
| 0.79 | -10.00 | 0.73 | -10.00 | 6.61 | 207.69 | 58.13 | 273.67 | 0.8475 | 683.0 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.90 | 5.93 | 207.57 | 58.01 | 272.86 | 0.8468 | 365.0 | 337.2 | |
| 0.00 | 1.23 | 0.00 | 1.14 | 6.45 | 207.54 | 57.99 | 273.47 | 0.8462 | 462.0 | 494.3 | |
| 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. | |