SDO HMI 2014-10-10 21:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.02 | 415.88 | 41.00 | 289.06 | -20.52 | 18.22 | -36.21 | 127.84 | 0.7031 | 931.7 | 285.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.83 | -21.27 | 20.40 | -34.04 | 130.39 | 0.6872 | -479.0 | -298.6 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -18.96 | 20.59 | -33.85 | 127.74 | 0.6684 | 802.0 | 730.7 | |
| 0.00 | 1.66 | 0.00 | 1.11 | -18.68 | 20.35 | -34.09 | 127.20 | 0.6689 | 793.0 | 644.6 | |
| 0.00 | 1.14 | 0.00 | 0.76 | -18.92 | 19.76 | -34.68 | 127.04 | 0.6766 | 874.0 | 621.2 | |
| 0.00 | 0.96 | 0.00 | 0.68 | -22.42 | 18.69 | -35.74 | 130.43 | 0.7117 | -735.0 | -611.4 | |
| 2.36 | 400.36 | 1.62 | 278.46 | -20.34 | 19.16 | -35.28 | 128.33 | 0.6926 | 1151.3 | 289.6 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -17.54 | 19.77 | -34.67 | 125.31 | 0.6670 | 670.0 | 595.3 | |
| 0.00 | 3.42 | 0.00 | 2.27 | -17.66 | 19.51 | -34.93 | 125.26 | 0.6705 | 801.0 | 664.6 | |
| 56.66 | -6.00 | 39.38 | -6.00 | -20.61 | 18.18 | -36.25 | 127.92 | 0.7040 | 1179.8 | 999999 | |
| 0.00 | 0.53 | 0.00 | 0.36 | -17.58 | 18.17 | -36.26 | 124.19 | 0.6841 | 578.0 | 414.8 | |
| 0.00 | 1.14 | 0.00 | 0.82 | -19.52 | 15.26 | -39.17 | 124.61 | 0.7257 | -691.0 | -517.3 | |
| 0.00 | 0.79 | 0.00 | 0.61 | -22.76 | 12.87 | -41.57 | 126.88 | 0.7672 | -533.0 | -476.3 | |
| 0.00 | 0.35 | 0.00 | 0.24 | -13.88 | 14.16 | -40.28 | 116.89 | 0.7061 | -590.0 | -518.5 | |
| 0.00 | 1.84 | 0.00 | 1.30 | -14.51 | 13.78 | -40.66 | 117.49 | 0.7134 | -435.0 | -322.7 | |
| 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. | |