| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.78 | 183.51 | 38.40 | 263.40 | 11.26 | 10.32 | 67.70 | 284.82 | 0.9397 | -84.1 | -67.1 | |
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back to the solar disc SDO HMI 2014-03-15 10:00:29 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.39 | 86.84 | 8.54 | 134.79 | 11.79 | 12.27 | 69.65 | 284.95 | 0.9514 | -119.0 | -178.9 | |
| 6.09 | -1.00 | 9.33 | -1.00 | 11.66 | 11.67 | 69.05 | 284.94 | 0.9481 | -676.0 | 999999 | |
| 0.96 | -1.00 | 1.46 | -1.00 | 12.00 | 11.43 | 68.81 | 285.35 | 0.9472 | -449.5 | 999999 | |
| 0.00 | 1.91 | 0.00 | 2.78 | 10.55 | 10.68 | 68.06 | 284.00 | 0.9413 | 57.0 | -98.0 | |
| 1.30 | 3.56 | 1.89 | 5.16 | 11.57 | 10.45 | 67.83 | 285.12 | 0.9413 | -576.7 | -547.9 | |
| 0.00 | 1.48 | 0.00 | 2.13 | 11.77 | 10.31 | 67.69 | 285.36 | 0.9407 | -283.0 | -248.9 | |
| 0.00 | 3.82 | 0.00 | 5.41 | 11.48 | 9.92 | 67.30 | 285.14 | 0.9381 | -515.0 | -479.3 | |
| 2.61 | 11.91 | 3.54 | 16.29 | 10.93 | 9.19 | 66.57 | 284.72 | 0.9330 | -90.6 | -371.0 | |
| 0.00 | 2.09 | 0.00 | 2.91 | 11.78 | 9.60 | 66.97 | 285.53 | 0.9366 | -407.0 | -367.9 | |
| 6.09 | 71.20 | 8.02 | 93.07 | 10.50 | 8.47 | 65.85 | 284.44 | 0.9280 | 406.6 | 204.2 | |
| 2.43 | -10.00 | 3.15 | -10.00 | 10.43 | 8.06 | 65.44 | 284.45 | 0.9254 | 854.6 | 999999 | |
| 1.04 | -10.00 | 1.35 | -10.00 | 11.19 | 7.95 | 65.32 | 285.28 | 0.9257 | 101.2 | 999999 | |
| 0.87 | -10.00 | 1.12 | -10.00 | 10.83 | 7.79 | 65.17 | 284.94 | 0.9242 | 354.1 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.86 | 11.09 | 6.82 | 64.20 | 285.44 | 0.9183 | 401.0 | 371.4 | |
| 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. | |