SDO HMI 2014-02-28 19:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.71 | 78.78 | 13.67 | 40.19 | -6.69 | 149.13 | 13.82 | 271.71 | 0.2388 | 522.8 | 285.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.44 | -8.09 | 150.75 | 15.44 | 265.69 | 0.2655 | -854.0 | -727.4 | |
| 13.96 | 43.70 | 7.16 | 22.39 | -7.30 | 150.50 | 15.19 | 268.71 | 0.2612 | 1064.7 | 730.4 | |
| 6.46 | -2.00 | 3.31 | -2.00 | -6.90 | 149.75 | 14.44 | 270.33 | 0.2486 | 1173.3 | 999999 | |
| 0.00 | 2.67 | 0.00 | 1.36 | -7.42 | 149.49 | 14.17 | 268.26 | 0.2440 | 682.0 | 404.0 | |
| 3.19 | 8.96 | 1.63 | 4.57 | -6.48 | 149.06 | 13.75 | 272.23 | 0.2373 | 1148.2 | 810.8 | |
| 0.69 | 2.50 | 0.35 | 1.27 | -6.31 | 148.66 | 13.34 | 273.08 | 0.2307 | 1158.0 | 908.8 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -5.82 | 148.25 | 12.93 | 275.42 | 0.2247 | 1003.0 | 816.1 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -4.72 | 146.91 | 11.60 | 281.52 | 0.2054 | -1064.0 | -861.4 | |
| 1.55 | 2.84 | 0.78 | 1.44 | -5.65 | 146.81 | 11.49 | 277.13 | 0.2007 | -1034.9 | -835.2 | |
| 0.86 | 10.34 | 0.44 | 5.23 | -5.32 | 146.80 | 11.49 | 278.74 | 0.2015 | -1151.1 | -867.3 | |
| 0.00 | 1.90 | 0.00 | 0.96 | -6.37 | 146.24 | 10.93 | 273.76 | 0.1897 | 826.0 | 413.0 | |
| 0.00 | 0.78 | 0.00 | 0.39 | -8.52 | 145.56 | 10.25 | 261.94 | 0.1785 | 965.0 | 837.6 | |
| 0.00 | 0.69 | 0.00 | 0.35 | -5.89 | 145.17 | 9.86 | 277.10 | 0.1724 | -909.0 | -597.6 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -5.17 | 144.19 | 8.88 | 282.53 | 0.1582 | -752.0 | -615.2 | |
| 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. | |