SDO HMI 2014-09-30 23:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.84 | 34.81 | 4.24 | 18.74 | 7.02 | 208.56 | 23.28 | 272.06 | 0.3942 | 81.7 | 52.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.15 | 0.00 | 0.63 | 7.38 | 211.18 | 25.90 | 273.01 | 0.4356 | -755.0 | -649.5 | |
| 2.64 | 4.67 | 1.45 | 2.56 | 7.37 | 210.77 | 25.49 | 272.99 | 0.4293 | -967.5 | -745.3 | |
| 0.00 | 1.32 | 0.00 | 0.72 | 8.14 | 210.45 | 25.18 | 274.80 | 0.4244 | -688.0 | -568.1 | |
| 0.00 | 1.94 | 0.00 | 1.05 | 7.02 | 209.91 | 24.64 | 272.14 | 0.4158 | -826.0 | -587.5 | |
| 0.00 | 2.38 | 0.00 | 1.29 | 6.85 | 209.77 | 24.49 | 271.72 | 0.4136 | -962.0 | -850.8 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 6.39 | 209.38 | 24.11 | 270.56 | 0.4076 | -840.0 | -653.0 | |
| 4.76 | 12.33 | 2.56 | 6.63 | 6.68 | 208.37 | 23.10 | 271.20 | 0.3914 | 764.6 | 289.0 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 7.10 | 207.09 | 21.81 | 272.25 | 0.3706 | 629.0 | 468.1 | |
| 0.44 | 4.40 | 0.23 | 2.34 | 7.55 | 206.88 | 21.61 | 273.50 | 0.3673 | 1011.6 | 810.4 | |
| 0.00 | 1.50 | 0.00 | 0.80 | 7.36 | 206.55 | 21.27 | 272.97 | 0.3618 | 655.0 | 540.6 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 7.07 | 206.37 | 21.09 | 272.15 | 0.3589 | 757.0 | 608.8 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 6.82 | 205.81 | 20.53 | 271.44 | 0.3499 | 659.0 | 476.4 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 5.89 | 205.09 | 19.81 | 268.64 | 0.3388 | 818.0 | 632.9 | |
| 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. | |