SDO HMI 2014-10-16 19:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.75 | 341.50 | 36.70 | 251.35 | -21.11 | 16.53 | 40.13 | 234.42 | 0.7415 | 856.2 | 304.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.00 | 323.51 | 17.80 | 238.82 | -21.22 | 16.99 | 40.60 | 234.59 | 0.7466 | 1004.2 | 325.4 | |
| 0.00 | 1.57 | 0.00 | 1.11 | -18.12 | 15.72 | 39.33 | 237.54 | 0.7163 | -260.0 | -300.6 | |
| 20.51 | -1.00 | 15.05 | -1.00 | -21.02 | 16.42 | 40.02 | 234.47 | 0.7400 | 1313.1 | 999999 | |
| 4.54 | -1.00 | 3.35 | -1.00 | -21.42 | 16.46 | 40.07 | 234.03 | 0.7428 | 964.2 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.56 | -20.75 | 14.97 | 38.57 | 233.85 | 0.7244 | 157.0 | 141.0 | |
| 0.00 | 2.53 | 0.00 | 1.82 | -21.37 | 14.79 | 38.39 | 233.00 | 0.7265 | 771.0 | 693.2 | |
| 0.70 | 4.10 | 0.50 | 2.94 | -21.59 | 14.53 | 38.13 | 232.57 | 0.7254 | 584.6 | 373.5 | |
| 0.00 | 1.75 | 0.00 | 1.25 | -22.39 | 13.92 | 37.52 | 231.21 | 0.7248 | -420.0 | -348.1 | |
| 0.00 | 1.40 | 0.00 | 0.97 | -21.08 | 12.80 | 36.40 | 231.96 | 0.7054 | -374.0 | -314.3 | |
| 0.00 | 0.96 | 0.00 | 0.67 | -21.42 | 12.42 | 36.02 | 231.28 | 0.7040 | -120.0 | -261.5 | |
| 0.00 | 1.66 | 0.00 | 1.07 | -15.13 | 10.31 | 33.91 | 237.72 | 0.6393 | -724.0 | -593.4 | |
| 0.00 | 2.18 | 0.00 | 1.42 | -17.69 | 9.53 | 33.14 | 233.71 | 0.6485 | -625.0 | -516.8 | |
| 0.00 | 1.05 | 0.00 | 0.72 | -23.23 | 9.58 | 33.19 | 226.97 | 0.6905 | -436.0 | -453.0 | |
| 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. | |