SDO HMI 2014-03-23 17:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.17 | 189.87 | 41.73 | 156.49 | 10.34 | 142.91 | -50.40 | 71.46 | 0.8009 | -152.1 | -101.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.18 | 115.18 | 20.68 | 90.92 | 10.14 | 144.86 | -48.45 | 71.01 | 0.7813 | -900.5 | -346.3 | |
| 0.70 | -1.00 | 0.56 | -1.00 | 10.44 | 144.29 | -49.02 | 70.86 | 0.7881 | -77.8 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.70 | 10.02 | 144.15 | -49.16 | 71.42 | 0.7883 | -178.0 | -158.2 | |
| 3.93 | 10.82 | 3.19 | 8.81 | 9.93 | 143.46 | -49.85 | 71.78 | 0.7949 | -491.5 | -322.9 | |
| 0.00 | 0.70 | 0.00 | 0.58 | 10.98 | 142.61 | -50.70 | 70.83 | 0.8065 | 578.0 | 507.2 | |
| 0.00 | 0.87 | 0.00 | 0.74 | 10.94 | 142.08 | -51.23 | 71.07 | 0.8115 | -468.0 | -377.5 | |
| 1.22 | 3.14 | 1.03 | 2.65 | 9.67 | 141.68 | -51.63 | 72.71 | 0.8116 | 575.6 | 506.2 | |
| 0.00 | 1.92 | 0.00 | 1.65 | 9.86 | 141.05 | -52.26 | 72.70 | 0.8182 | -104.0 | -164.6 | |
| 0.00 | 1.05 | 0.00 | 0.92 | 11.18 | 140.58 | -52.73 | 71.31 | 0.8263 | 672.0 | 627.2 | |
| 0.00 | 0.70 | 0.00 | 0.61 | 9.49 | 140.13 | -53.18 | 73.43 | 0.8260 | 636.0 | 561.6 | |
| 13.35 | 48.08 | 11.93 | 43.00 | 11.02 | 139.65 | -53.66 | 71.80 | 0.8345 | 742.8 | 472.4 | |
| 1.13 | -11.00 | 1.01 | -11.00 | 10.80 | 139.65 | -53.66 | 72.05 | 0.8338 | 666.8 | 999999 | |
| 2.79 | -11.00 | 2.55 | -11.00 | 11.17 | 138.82 | -54.49 | 71.90 | 0.8423 | 355.7 | 999999 | |
| 0.87 | 2.53 | 0.78 | 2.26 | 9.45 | 139.21 | -54.10 | 73.76 | 0.8344 | 531.5 | 477.8 | |
| 0.00 | 0.87 | 0.00 | 0.79 | 9.42 | 138.90 | -54.41 | 73.88 | 0.8372 | 197.0 | 211.7 | |
| 0.00 | 0.70 | 0.00 | 0.63 | 9.22 | 138.47 | -54.84 | 74.25 | 0.8406 | 74.0 | 143.2 | |
| 0.00 | 2.44 | 0.00 | 2.23 | 8.54 | 138.20 | -55.11 | 75.11 | 0.8414 | -339.0 | -477.6 | |
| 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. | |