SDO HMI 2014-10-10 07:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.67 | 369.74 | 47.34 | 288.74 | -20.55 | 18.50 | -43.63 | 123.17 | 0.7741 | 850.4 | 226.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.93 | 0.00 | 1.44 | -20.05 | 20.68 | -41.46 | 123.83 | 0.7511 | 586.0 | 491.6 | |
| 0.61 | 354.56 | 0.47 | 277.05 | -20.33 | 19.98 | -42.15 | 123.76 | 0.7592 | 887.1 | 228.6 | |
| 0.53 | -2.00 | 0.40 | -2.00 | -20.45 | 19.77 | -42.37 | 123.77 | 0.7618 | 780.3 | 999999 | |
| 2.28 | -2.00 | 1.75 | -2.00 | -20.44 | 19.38 | -42.76 | 123.54 | 0.7655 | 998.2 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.93 | -19.24 | 19.61 | -42.53 | 122.26 | 0.7570 | 652.0 | 491.9 | |
| 0.35 | 1.23 | 0.26 | 0.91 | -17.70 | 19.66 | -42.48 | 120.45 | 0.7486 | 781.0 | 644.6 | |
| 56.90 | -2.00 | 44.46 | -2.00 | -20.65 | 18.42 | -43.71 | 123.24 | 0.7754 | 1019.4 | 999999 | |
| 0.00 | 4.82 | 0.00 | 3.61 | -17.75 | 19.34 | -42.80 | 120.34 | 0.7520 | 663.0 | 499.4 | |
| 0.00 | 0.96 | 0.00 | 0.73 | -18.07 | 18.59 | -43.54 | 120.31 | 0.7609 | -521.0 | -444.1 | |
| 0.00 | 0.79 | 0.00 | 0.66 | -23.92 | 16.30 | -45.84 | 125.74 | 0.8101 | 497.0 | 423.9 | |
| 0.00 | 0.88 | 0.00 | 0.67 | -16.69 | 18.05 | -44.08 | 118.37 | 0.7596 | -647.0 | -590.1 | |
| 0.00 | 0.88 | 0.00 | 0.70 | -20.24 | 16.86 | -45.27 | 121.93 | 0.7877 | -169.0 | -150.4 | |
| 0.00 | 0.88 | 0.00 | 0.68 | -17.83 | 17.53 | -44.61 | 119.46 | 0.7701 | -432.0 | -342.0 | |
| 0.00 | 1.58 | 0.00 | 1.36 | -17.04 | 11.78 | -50.36 | 115.89 | 0.8205 | -619.0 | -449.0 | |
| 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. | |