SDO HMI 2014-05-19 10:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.53 | 157.34 | 32.34 | 186.39 | -13.31 | 229.33 | 65.01 | 256.22 | 0.9085 | 314.4 | 149.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.40 | 143.75 | 16.49 | 174.79 | -12.67 | 230.43 | 66.12 | 257.11 | 0.9169 | 541.0 | 192.0 | |
| 13.13 | -1.00 | 15.85 | -1.00 | -13.24 | 229.89 | 65.57 | 256.45 | 0.9134 | 641.0 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.74 | -12.55 | 229.17 | 64.85 | 257.16 | 0.9080 | 645.0 | 612.9 | |
| 0.00 | 0.81 | 0.00 | 0.91 | -11.57 | 228.01 | 63.69 | 258.17 | 0.8991 | -310.0 | -251.3 | |
| 0.00 | 0.99 | 0.00 | 1.05 | -15.85 | 225.84 | 61.53 | 253.19 | 0.8853 | -258.0 | -202.1 | |
| 0.00 | 0.81 | 0.00 | 0.79 | -14.08 | 223.35 | 59.04 | 254.92 | 0.8634 | -490.0 | -433.7 | |
| 0.00 | 0.90 | 0.00 | 0.76 | -20.45 | 216.28 | 51.97 | 246.08 | 0.8095 | -625.0 | -491.4 | |
| 0.00 | 0.27 | 0.00 | 0.23 | -20.84 | 216.36 | 52.05 | 245.64 | 0.8111 | -427.0 | -395.0 | |
| 0.00 | 1.53 | 0.00 | 1.30 | -21.73 | 216.65 | 52.34 | 244.64 | 0.8159 | -494.0 | -399.4 | |
| 0.00 | 2.07 | 0.00 | 1.77 | -21.93 | 216.70 | 52.38 | 244.42 | 0.8168 | -520.0 | -389.8 | |
| 0.00 | 0.45 | 0.00 | 0.37 | -20.87 | 215.27 | 50.96 | 245.31 | 0.8010 | -686.0 | -619.6 | |
| 0.00 | 2.16 | 0.00 | 1.63 | -16.28 | 212.14 | 47.82 | 250.24 | 0.7582 | -689.0 | -550.2 | |
| 0.00 | 0.63 | 0.00 | 0.49 | -19.57 | 212.31 | 48.00 | 246.07 | 0.7683 | -509.0 | -473.4 | |
| 0.00 | 2.34 | 0.00 | 1.56 | -24.26 | 201.20 | 36.89 | 235.01 | 0.6702 | -776.0 | -628.3 | |
| 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. | |