SDO HMI 2014-04-04 13:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.20 | 182.47 | 25.81 | 99.47 | 17.08 | 29.64 | -7.59 | 17.50 | 0.4192 | -138.9 | -308.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.76 | 134.04 | 0.95 | 72.79 | 16.94 | 31.29 | -5.94 | 14.08 | 0.4086 | -1058.5 | -484.9 | |
| 14.50 | -1.00 | 7.88 | -1.00 | 17.20 | 31.00 | -6.23 | 14.57 | 0.4138 | -1155.2 | 999999 | |
| 1.76 | -1.00 | 0.95 | -1.00 | 16.68 | 30.92 | -6.31 | 15.09 | 0.4061 | -1303.2 | 999999 | |
| 8.44 | -1.00 | 4.58 | -1.00 | 16.88 | 30.76 | -6.47 | 15.33 | 0.4098 | -1158.7 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 16.79 | 30.35 | -6.88 | 16.31 | 0.4102 | -555.0 | -515.2 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 15.95 | 29.81 | -7.42 | 18.16 | 0.4000 | -799.0 | -634.0 | |
| 0.00 | 1.67 | 0.00 | 0.90 | 15.90 | 29.09 | -8.14 | 19.84 | 0.4029 | -904.0 | -773.8 | |
| 0.00 | 2.11 | 0.00 | 1.14 | 15.96 | 28.96 | -8.27 | 20.07 | 0.4046 | -642.0 | -590.5 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 17.17 | 27.04 | -10.19 | 23.05 | 0.4336 | 736.0 | 608.2 | |
| 12.74 | 33.66 | 7.03 | 18.57 | 17.17 | 25.89 | -11.34 | 25.34 | 0.4409 | 1054.1 | 676.7 | |
| 8.00 | -10.00 | 4.42 | -10.00 | 17.21 | 25.53 | -11.70 | 25.99 | 0.4439 | 1024.2 | 999999 | |
| 0.00 | 4.13 | 0.00 | 2.29 | 17.52 | 25.03 | -12.20 | 26.62 | 0.4517 | 698.0 | 633.0 | |
| 0.00 | 1.41 | 0.00 | 0.79 | 18.58 | 24.60 | -12.63 | 26.33 | 0.4693 | 582.0 | 460.2 | |
| 0.00 | 1.76 | 0.00 | 0.98 | 18.36 | 24.26 | -12.97 | 27.16 | 0.4686 | 905.0 | 733.5 | |
| 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. | |