SDO HMI 2014-09-16 17:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.19 | 146.64 | 46.47 | 261.59 | 15.39 | 88.53 | 75.16 | 284.01 | 0.9618 | 332.5 | 119.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.66 | 114.06 | 31.70 | 205.04 | 14.85 | 88.63 | 75.26 | 283.45 | 0.9624 | 472.8 | 157.1 | |
| 1.78 | 6.66 | 3.35 | 12.54 | 16.69 | 89.55 | 76.18 | 285.41 | 0.9660 | -138.6 | -115.1 | |
| 0.00 | 3.46 | 0.00 | 6.35 | 18.06 | 89.17 | 75.81 | 286.81 | 0.9640 | -574.0 | -498.7 | |
| 0.00 | 0.98 | 0.00 | 1.70 | 17.32 | 88.25 | 74.88 | 286.00 | 0.9600 | -40.0 | -50.0 | |
| 3.91 | 9.94 | 6.53 | 16.69 | 17.19 | 87.50 | 74.13 | 285.83 | 0.9564 | 440.2 | 256.0 | |
| 0.00 | 2.22 | 0.00 | 3.59 | 16.57 | 86.84 | 73.47 | 285.16 | 0.9533 | 419.0 | 328.4 | |
| 1.60 | -5.00 | 2.70 | -5.00 | 17.45 | 87.67 | 74.31 | 286.11 | 0.9573 | 370.7 | 999999 | |
| 0.00 | 0.89 | 0.00 | 1.58 | 18.31 | 88.72 | 75.35 | 287.05 | 0.9619 | -596.0 | -563.9 | |
| 0.62 | 1.95 | 1.13 | 3.54 | 18.66 | 88.93 | 75.56 | 287.43 | 0.9628 | -288.3 | -210.7 | |
| 0.62 | 2.22 | 1.06 | 3.79 | 18.08 | 87.94 | 74.57 | 286.78 | 0.9584 | -430.3 | -341.1 | |
| 0.00 | 1.24 | 0.00 | 1.89 | 15.94 | 85.58 | 72.21 | 284.44 | 0.9469 | 299.0 | 224.7 | |
| 0.00 | 2.31 | 0.00 | 3.84 | 17.89 | 87.47 | 74.10 | 286.56 | 0.9562 | 369.0 | 321.5 | |
| 0.00 | 0.71 | 0.00 | 1.04 | 18.13 | 84.89 | 71.52 | 286.74 | 0.9427 | 286.0 | 279.0 | |
| 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. | |