| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.42 | 183.64 | 62.72 | 315.91 | -18.42 | 124.30 | -71.60 | 109.89 | 0.9580 | 334.6 | 26.2 | |
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back to the solar disc SDO HMI 2014-11-23 18:00:26 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.77 | 166.94 | 1.28 | 276.67 | -19.24 | 125.09 | -70.81 | 110.83 | 0.9554 | 77.4 | 83.0 | |
| 12.93 | -1.00 | 21.10 | -1.00 | -18.79 | 125.25 | -70.65 | 110.39 | 0.9543 | 536.6 | 999999 | |
| 10.28 | -1.00 | 16.46 | -1.00 | -17.90 | 125.53 | -70.37 | 109.51 | 0.9522 | 688.3 | 999999 | |
| 0.00 | 1.54 | 0.00 | 2.76 | -19.57 | 123.74 | -72.16 | 110.98 | 0.9619 | -388.0 | -352.3 | |
| 1.97 | -1.00 | 3.35 | -1.00 | -18.60 | 124.47 | -71.43 | 110.08 | 0.9579 | -211.6 | 999999 | |
| 1.11 | -1.00 | 1.87 | -1.00 | -18.31 | 124.56 | -71.34 | 109.79 | 0.9572 | 83.8 | 999999 | |
| 2.66 | -1.00 | 4.46 | -1.00 | -18.09 | 124.58 | -71.32 | 109.57 | 0.9570 | 250.7 | 999999 | |
| 0.00 | 1.11 | 0.00 | 2.35 | -20.32 | 121.11 | -74.78 | 111.41 | 0.9731 | -336.0 | -316.2 | |
| 5.82 | -1.00 | 10.08 | -1.00 | -17.61 | 123.95 | -71.94 | 108.99 | 0.9596 | 215.3 | 999999 | |
| 0.00 | 1.11 | 0.00 | 2.34 | -20.06 | 121.10 | -74.80 | 111.15 | 0.9730 | -392.0 | -372.0 | |
| 1.88 | 8.82 | 4.12 | 19.02 | -19.48 | 120.53 | -75.37 | 110.49 | 0.9748 | -8.5 | -231.3 | |
| 0.00 | 0.26 | 0.00 | 0.79 | -19.65 | 116.42 | -79.48 | 110.25 | 0.9877 | -470.0 | -470.3 | |
| 0.00 | 1.20 | 0.00 | 3.72 | -19.49 | 116.38 | -79.52 | 110.08 | 0.9877 | -444.0 | -438.8 | |
| 0.00 | 2.66 | 0.00 | 8.26 | -19.08 | 116.28 | -79.61 | 109.66 | 0.9879 | -428.0 | -415.6 | |
| 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. | |