SDO HMI 2014-05-19 09:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.72 | 43.73 | 8.31 | 36.99 | -18.17 | 217.74 | 52.88 | 249.06 | 0.8132 | 131.8 | 64.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.47 | 22.76 | 6.47 | 19.66 | -18.48 | 218.65 | 53.79 | 248.88 | 0.8225 | 650.5 | 217.0 | |
| 0.00 | 1.26 | 0.00 | 1.09 | -18.11 | 218.48 | 53.62 | 249.30 | 0.8202 | 442.0 | 588.4 | |
| 0.00 | 1.53 | 0.00 | 1.31 | -17.98 | 218.37 | 53.51 | 249.43 | 0.8189 | 572.0 | 433.6 | |
| 0.00 | 2.97 | 0.00 | 2.49 | -17.00 | 217.53 | 52.67 | 250.45 | 0.8091 | 608.0 | 493.5 | |
| 0.00 | 0.63 | 0.00 | 0.53 | -18.80 | 217.72 | 52.85 | 248.30 | 0.8143 | -371.0 | -277.3 | |
| 0.00 | 1.44 | 0.00 | 1.22 | -18.80 | 217.51 | 52.64 | 248.25 | 0.8123 | -524.0 | -435.8 | |
| 0.72 | 3.06 | 0.60 | 2.56 | -18.62 | 217.16 | 52.30 | 248.39 | 0.8087 | -479.6 | -382.3 | |
| 0.00 | 1.53 | 0.00 | 1.23 | -15.72 | 215.92 | 51.06 | 251.69 | 0.7908 | -574.0 | -474.8 | |
| 0.00 | 1.26 | 0.00 | 1.04 | -18.26 | 216.48 | 51.62 | 248.67 | 0.8014 | -410.0 | -261.7 | |
| 0.90 | 1.80 | 0.74 | 1.48 | -18.42 | 216.40 | 51.53 | 248.45 | 0.8009 | -474.0 | -416.6 | |
| 0.00 | 0.81 | 0.00 | 0.66 | -18.43 | 216.14 | 51.28 | 248.38 | 0.7984 | -535.0 | -504.0 | |
| 0.63 | 1.98 | 0.50 | 1.58 | -17.18 | 215.29 | 50.43 | 249.72 | 0.7874 | -622.4 | -469.4 | |
| 0.00 | 1.17 | 0.00 | 0.94 | -17.56 | 215.29 | 50.43 | 249.25 | 0.7881 | -430.0 | -371.9 | |
| 0.00 | 1.53 | 0.00 | 1.20 | -17.53 | 214.09 | 49.22 | 248.99 | 0.7758 | 376.0 | 265.3 | |
| 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. | |