| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.59 | 39.55 | 9.33 | 39.38 | -23.83 | 94.52 | -56.33 | 118.68 | 0.8696 | 51.1 | -126.2 | |
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back to the solar disc SDO HMI 2014-11-27 04:00:26 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.59 | 20.12 | 9.33 | 19.55 | -24.33 | 95.56 | -55.29 | 119.54 | 0.8630 | 546.3 | 274.1 | |
| 0.00 | 1.97 | 0.00 | 1.92 | -23.88 | 95.28 | -55.57 | 118.95 | 0.8640 | -302.0 | -270.5 | |
| 0.00 | 1.63 | 0.00 | 1.62 | -24.18 | 94.67 | -56.18 | 119.10 | 0.8694 | 136.0 | 55.8 | |
| 0.00 | 0.94 | 0.00 | 0.93 | -23.86 | 94.71 | -56.14 | 118.75 | 0.8683 | -232.0 | -221.2 | |
| 0.00 | 0.26 | 0.00 | 0.26 | -24.63 | 93.82 | -57.03 | 119.34 | 0.8768 | 197.0 | 216.0 | |
| 0.00 | 0.94 | 0.00 | 0.94 | -23.70 | 94.40 | -56.44 | 118.49 | 0.8702 | -422.0 | -440.5 | |
| 0.00 | 1.20 | 0.00 | 1.22 | -23.62 | 93.69 | -57.16 | 118.19 | 0.8754 | -497.0 | -478.4 | |
| 0.00 | 1.46 | 0.00 | 1.48 | -23.20 | 93.68 | -57.17 | 117.72 | 0.8745 | -554.0 | -474.2 | |
| 0.00 | 1.03 | 0.00 | 1.05 | -23.10 | 93.50 | -57.35 | 117.57 | 0.8756 | -294.0 | -361.4 | |
| 0.00 | 2.82 | 0.00 | 2.88 | -22.81 | 93.27 | -57.58 | 117.19 | 0.8767 | -436.0 | -371.4 | |
| 0.00 | 4.19 | 0.00 | 4.35 | -23.08 | 92.84 | -58.00 | 117.36 | 0.8804 | -519.0 | -442.2 | |
| 0.00 | 0.34 | 0.00 | 0.36 | -22.70 | 92.62 | -58.23 | 116.88 | 0.8813 | -281.0 | -260.2 | |
| 0.00 | 2.14 | 0.00 | 2.27 | -23.10 | 92.09 | -58.76 | 117.18 | 0.8860 | -481.0 | -305.7 | |
| 0.00 | 0.51 | 0.00 | 0.55 | -23.24 | 91.80 | -59.04 | 117.25 | 0.8883 | -272.0 | -287.2 | |
| 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. | |