SDO HMI 2014-10-01 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.65 | 106.77 | 15.13 | 66.11 | -10.20 | 140.37 | -32.82 | 117.01 | 0.6011 | 558.4 | 292.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.32 | 0.00 | 0.86 | -16.91 | 140.39 | -32.80 | 126.45 | 0.6466 | 534.0 | 442.0 | |
| 24.65 | 93.39 | 15.13 | 57.36 | -9.63 | 140.74 | -32.45 | 116.45 | 0.5931 | 1092.8 | 384.5 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -13.51 | 140.18 | -33.01 | 121.70 | 0.6248 | 664.0 | 563.0 | |
| 0.00 | 0.97 | 0.00 | 0.62 | -14.80 | 139.55 | -33.63 | 122.99 | 0.6407 | 368.0 | 284.9 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -11.38 | 139.90 | -33.28 | 118.45 | 0.6141 | 655.0 | 600.4 | |
| 0.00 | 1.23 | 0.00 | 0.81 | -16.10 | 138.89 | -34.29 | 124.21 | 0.6569 | 573.0 | 404.6 | |
| 0.00 | 1.06 | 0.00 | 0.70 | -15.05 | 137.77 | -35.42 | 122.00 | 0.6622 | -491.0 | -380.3 | |
| 0.00 | 1.67 | 0.00 | 1.09 | -13.42 | 137.69 | -35.50 | 119.76 | 0.6529 | -659.0 | -521.4 | |
| 0.00 | 1.50 | 0.00 | 0.99 | -13.97 | 136.67 | -36.52 | 119.81 | 0.6678 | -494.0 | -437.2 | |
| 0.00 | 0.88 | 0.00 | 0.58 | -12.57 | 136.73 | -36.46 | 117.95 | 0.6589 | -636.0 | -555.1 | |
| 0.00 | 1.50 | 0.00 | 0.99 | -12.86 | 136.64 | -36.55 | 118.29 | 0.6616 | -572.0 | -475.2 | |
| 0.00 | 0.79 | 0.00 | 0.52 | -12.36 | 136.57 | -36.62 | 117.56 | 0.6595 | -709.0 | -647.7 | |
| 0.00 | 1.06 | 0.00 | 0.70 | -12.54 | 136.35 | -36.84 | 117.66 | 0.6631 | -619.0 | -509.1 | |
| 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. | |