SDO HMI 2014-06-09 23:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.38 | 0.00 | 12.24 | 4.79 | 261.95 | 22.71 | 283.35 | 0.3912 | 189.5 | 66.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.90 | 0.00 | 1.15 | 4.87 | 273.68 | 34.43 | 278.03 | 0.5710 | -628.0 | -378.8 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 4.79 | 272.53 | 33.28 | 278.11 | 0.5545 | -699.0 | -605.2 | |
| 0.00 | 2.81 | 0.00 | 1.66 | 4.69 | 272.30 | 33.06 | 277.99 | 0.5511 | -645.0 | -581.3 | |
| 0.00 | 1.27 | 0.00 | 0.74 | 2.72 | 271.46 | 32.21 | 274.49 | 0.5361 | -662.0 | -537.3 | |
| 0.00 | 1.36 | 0.00 | 0.78 | 4.59 | 269.43 | 30.18 | 278.42 | 0.5085 | -728.0 | -625.7 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 3.03 | 268.48 | 29.24 | 275.52 | 0.4920 | -437.0 | -396.9 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 6.48 | 261.26 | 22.01 | 285.99 | 0.3891 | 712.0 | 566.4 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 6.39 | 260.93 | 21.68 | 285.98 | 0.3835 | 743.0 | 600.1 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 9.19 | 259.30 | 20.05 | 294.39 | 0.3733 | 656.0 | 438.0 | |
| 0.00 | 2.35 | 0.00 | 1.21 | 6.44 | 253.90 | 14.65 | 292.83 | 0.2739 | 786.0 | 496.5 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 5.11 | 250.72 | 11.48 | 292.60 | 0.2156 | 939.0 | 708.4 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 8.26 | 249.83 | 10.58 | 307.05 | 0.2288 | 476.0 | 425.2 | |
| 0.00 | 2.08 | 0.00 | 1.04 | 1.06 | 246.48 | 7.23 | 275.44 | 0.1270 | 1050.0 | 853.5 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 1.25 | 243.06 | 3.81 | 282.92 | 0.0685 | 1090.0 | 922.6 | |
| 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. | |