SDO HMI 2014-02-26 16:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.52 | 234.10 | 64.86 | 344.65 | -25.19 | 91.88 | -71.43 | 114.24 | 0.9414 | -127.6 | -7.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.67 | 12.23 | 3.46 | 15.93 | -24.10 | 94.80 | -68.51 | 113.16 | 0.9255 | 247.3 | 104.5 | |
| 1.12 | -1.00 | 1.46 | -1.00 | -24.27 | 94.60 | -68.71 | 113.34 | 0.9268 | 234.7 | 999999 | |
| 5.43 | 88.80 | 6.78 | 115.37 | -23.11 | 95.71 | -67.60 | 112.12 | 0.9197 | 709.3 | 99.3 | |
| 0.00 | 1.29 | 0.00 | 1.75 | -24.82 | 93.75 | -69.57 | 113.90 | 0.9319 | 68.0 | 27.5 | |
| 1.03 | -3.00 | 1.33 | -3.00 | -23.67 | 95.01 | -68.30 | 112.71 | 0.9241 | 348.7 | 999999 | |
| 7.06 | -3.00 | 9.07 | -3.00 | -23.26 | 95.03 | -68.28 | 112.26 | 0.9239 | 543.8 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.12 | -23.63 | 94.61 | -68.70 | 112.64 | 0.9265 | -174.0 | -99.9 | |
| 0.00 | 1.12 | 0.00 | 1.48 | -23.90 | 94.21 | -69.11 | 112.93 | 0.9290 | -350.0 | -332.7 | |
| 0.00 | 1.03 | 0.00 | 1.55 | -25.97 | 91.34 | -71.97 | 115.06 | 0.9452 | -432.0 | -478.1 | |
| 1.46 | -3.00 | 1.93 | -3.00 | -23.37 | 94.36 | -68.95 | 112.36 | 0.9280 | 108.2 | 999999 | |
| 21.96 | 127.99 | 35.17 | 206.30 | -26.39 | 89.87 | -73.44 | 115.48 | 0.9525 | -472.7 | -66.5 | |
| 2.07 | -11.00 | 3.22 | -11.00 | -25.90 | 90.45 | -72.86 | 114.97 | 0.9497 | -573.0 | 999999 | |
| 1.72 | -3.00 | 2.44 | -3.00 | -23.75 | 92.57 | -70.74 | 112.72 | 0.9383 | -458.9 | 999999 | |
| 0.00 | 0.78 | 0.00 | 1.15 | -23.05 | 91.54 | -71.77 | 111.97 | 0.9439 | -47.0 | -56.1 | |
| 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. | |