SDO HMI 2014-08-14 16:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.31 | 52.07 | 18.98 | 63.53 | 16.14 | 22.95 | -66.90 | 75.22 | 0.9149 | 18.8 | 32.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.34 | 0.00 | 2.56 | 16.69 | 26.11 | -63.74 | 74.60 | 0.8929 | -551.0 | -503.3 | |
| 0.00 | 2.43 | 0.00 | 2.66 | 16.41 | 26.07 | -63.79 | 74.92 | 0.8932 | -637.0 | -473.4 | |
| 0.00 | 2.25 | 0.00 | 2.49 | 16.90 | 25.69 | -64.17 | 74.37 | 0.8961 | -486.0 | -439.8 | |
| 1.44 | 4.15 | 1.61 | 4.62 | 16.63 | 25.49 | -64.36 | 74.68 | 0.8975 | -495.5 | -364.1 | |
| 1.89 | 3.61 | 2.12 | 4.04 | 16.23 | 25.29 | -64.56 | 75.13 | 0.8989 | -373.5 | -214.2 | |
| 0.00 | 2.07 | 0.00 | 2.38 | 16.86 | 24.59 | -65.26 | 74.44 | 0.9040 | -246.0 | -166.4 | |
| 0.00 | 1.44 | 0.00 | 1.67 | 17.08 | 24.29 | -65.56 | 74.20 | 0.9062 | -30.0 | -57.8 | |
| 0.00 | 1.08 | 0.00 | 1.24 | 15.47 | 24.55 | -65.30 | 75.98 | 0.9043 | -150.0 | -189.5 | |
| 3.15 | 6.40 | 3.77 | 7.69 | 16.61 | 23.43 | -66.43 | 74.72 | 0.9122 | -221.6 | 86.8 | |
| 0.00 | 0.99 | 0.00 | 1.22 | 17.08 | 22.77 | -67.08 | 74.21 | 0.9167 | 186.0 | 179.5 | |
| 5.77 | 15.59 | 7.28 | 19.63 | 15.43 | 22.09 | -67.76 | 76.00 | 0.9212 | 423.0 | 318.0 | |
| 1.17 | 3.42 | 1.60 | 4.67 | 16.39 | 20.15 | -69.70 | 74.94 | 0.9333 | 352.7 | 380.2 | |
| 1.17 | 3.24 | 1.59 | 4.41 | 15.83 | 20.22 | -69.63 | 75.54 | 0.9329 | 470.3 | 428.7 | |
| 0.72 | 2.79 | 1.01 | 3.89 | 16.24 | 19.62 | -70.23 | 75.09 | 0.9365 | 55.6 | 118.5 | |
| 0.00 | 0.27 | 0.00 | 0.36 | 15.14 | 20.47 | -69.38 | 76.30 | 0.9315 | 399.0 | 360.0 | |
| 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. | |