SDO HMI 2014-12-04 05:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.32 | 49.78 | 25.18 | 71.96 | -15.89 | 126.92 | 68.87 | 252.76 | 0.9386 | 81.1 | 46.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.76 | 8.54 | 7.06 | 16.07 | -15.09 | 132.06 | 74.01 | 254.20 | 0.9658 | 245.7 | 121.6 | |
| 0.85 | -1.00 | 1.61 | -1.00 | -15.37 | 132.10 | 74.05 | 253.92 | 0.9661 | 298.9 | 999999 | |
| 0.00 | 0.68 | 0.00 | 1.30 | -15.52 | 132.25 | 74.21 | 253.77 | 0.9668 | -125.0 | -95.4 | |
| 5.38 | 24.51 | 7.78 | 35.68 | -15.20 | 127.13 | 69.09 | 253.61 | 0.9411 | 381.9 | 153.0 | |
| 4.36 | -4.00 | 6.39 | -4.00 | -15.63 | 127.36 | 69.31 | 253.18 | 0.9427 | -163.7 | 999999 | |
| 0.00 | 1.79 | 0.00 | 2.51 | -15.25 | 126.40 | 68.35 | 253.47 | 0.9369 | 316.0 | 317.3 | |
| 0.00 | 1.28 | 0.00 | 1.69 | -17.30 | 124.68 | 66.63 | 251.06 | 0.9282 | 457.0 | 326.7 | |
| 0.77 | 2.56 | 0.94 | 3.14 | -15.71 | 123.02 | 64.97 | 252.54 | 0.9161 | -317.1 | -169.8 | |
| 0.00 | 1.20 | 0.00 | 1.45 | -16.39 | 122.70 | 64.65 | 251.76 | 0.9146 | -310.0 | -261.2 | |
| 1.20 | 4.53 | 1.40 | 5.35 | -17.55 | 121.65 | 63.60 | 250.33 | 0.9087 | -496.8 | -345.5 | |
| 0.00 | 0.68 | 0.00 | 0.81 | -20.72 | 121.39 | 63.34 | 246.85 | 0.9109 | 111.0 | 171.9 | |
| 0.00 | 1.79 | 0.00 | 1.79 | -20.39 | 115.91 | 57.86 | 246.05 | 0.8706 | -594.0 | -488.9 | |
| 0.00 | 0.60 | 0.00 | 0.57 | -18.58 | 114.68 | 56.63 | 247.79 | 0.8571 | -49.0 | -73.4 | |
| 0.00 | 1.62 | 0.00 | 1.60 | -20.38 | 115.43 | 57.38 | 245.93 | 0.8668 | -263.0 | -222.9 | |
| 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. | |