SDO HMI 2014-05-26 17:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.65 | 104.02 | 27.86 | 150.63 | -14.21 | 137.29 | 69.44 | 255.32 | 0.9390 | 15.5 | -3.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.60 | 58.33 | 7.32 | 92.29 | -14.37 | 139.49 | 71.64 | 255.31 | 0.9518 | 48.7 | 67.6 | |
| 5.50 | -1.00 | 8.35 | -1.00 | -14.61 | 138.49 | 70.64 | 254.99 | 0.9466 | 621.6 | 999999 | |
| 0.00 | 1.26 | 0.00 | 1.71 | -13.72 | 136.08 | 68.23 | 255.77 | 0.9323 | 3.0 | 73.4 | |
| 0.00 | 0.54 | 0.00 | 0.76 | -15.21 | 136.89 | 69.04 | 254.24 | 0.9378 | 610.0 | 585.0 | |
| 0.00 | 2.34 | 0.00 | 3.14 | -13.94 | 135.79 | 67.94 | 255.51 | 0.9306 | 235.0 | 236.6 | |
| 1.26 | 2.79 | 1.67 | 3.69 | -13.76 | 135.43 | 67.58 | 255.68 | 0.9283 | -333.4 | -179.8 | |
| 0.00 | 1.98 | 0.00 | 2.63 | -14.20 | 135.53 | 67.68 | 255.22 | 0.9291 | -1.0 | 117.4 | |
| 5.59 | 22.18 | 7.11 | 28.04 | -13.41 | 134.57 | 66.72 | 256.00 | 0.9226 | -397.4 | -203.6 | |
| 0.72 | 2.43 | 0.94 | 3.17 | -14.40 | 135.07 | 67.22 | 254.97 | 0.9263 | -328.1 | -179.5 | |
| 0.00 | 4.24 | 0.00 | 5.55 | -14.68 | 135.25 | 67.40 | 254.68 | 0.9276 | 369.0 | 176.3 | |
| 1.98 | -8.00 | 2.47 | -8.00 | -13.63 | 134.07 | 66.22 | 255.71 | 0.9194 | -468.4 | 999999 | |
| 0.00 | 1.98 | 0.00 | 2.44 | -13.80 | 133.69 | 65.84 | 255.50 | 0.9169 | -465.0 | -398.8 | |
| 0.00 | 5.50 | 0.00 | 6.68 | -13.52 | 133.39 | 65.54 | 255.77 | 0.9147 | -393.0 | -357.6 | |
| 0.00 | 0.45 | 0.00 | 0.53 | -14.14 | 132.44 | 64.59 | 255.01 | 0.9085 | -501.0 | -492.8 | |
| 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. | |