SDO HMI 2014-04-17 16:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.63 | 176.85 | 20.75 | 118.77 | 12.00 | 262.71 | 38.74 | 294.77 | 0.6749 | -568.9 | -250.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.41 | 164.19 | 12.51 | 111.35 | 12.02 | 263.71 | 39.74 | 293.99 | 0.6867 | -993.0 | -306.9 | |
| 0.27 | -1.00 | 0.18 | -1.00 | 12.39 | 263.62 | 39.64 | 294.54 | 0.6873 | -752.0 | 999999 | |
| 11.95 | -1.00 | 8.06 | -1.00 | 11.65 | 263.41 | 39.43 | 293.65 | 0.6814 | -1296.6 | 999999 | |
| 0.00 | 1.33 | 0.00 | 0.89 | 12.33 | 262.73 | 38.76 | 294.95 | 0.6768 | -680.0 | -570.9 | |
| 0.00 | 1.59 | 0.00 | 0.97 | 12.39 | 255.05 | 31.08 | 300.11 | 0.5851 | 733.0 | 597.6 | |
| 0.00 | 1.33 | 0.00 | 0.84 | 16.82 | 255.47 | 31.50 | 306.12 | 0.6214 | 624.0 | 485.5 | |
| 0.00 | 0.80 | 0.00 | 0.45 | 12.79 | 246.08 | 22.11 | 309.79 | 0.4795 | 498.0 | 445.7 | |
| 0.00 | 1.06 | 0.00 | 0.60 | 12.96 | 245.46 | 21.49 | 310.86 | 0.4740 | 727.0 | 639.9 | |
| 0.00 | 1.24 | 0.00 | 0.69 | 12.92 | 245.16 | 21.19 | 311.19 | 0.4700 | 663.0 | 575.3 | |
| 0.00 | 1.06 | 0.00 | 0.61 | 15.35 | 245.34 | 21.36 | 314.75 | 0.4966 | 686.0 | 503.8 | |
| 0.00 | 1.68 | 0.00 | 0.94 | 12.88 | 244.99 | 21.02 | 311.35 | 0.4677 | 838.0 | 631.9 | |
| 0.00 | 1.33 | 0.00 | 0.74 | 12.85 | 244.07 | 20.09 | 312.58 | 0.4567 | 781.0 | 625.8 | |
| 0.00 | 1.24 | 0.00 | 0.69 | 13.45 | 242.87 | 18.90 | 315.30 | 0.4496 | 829.0 | 629.3 | |
| 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. | |