SDO HMI 2014-11-04 18:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.87 | 32.15 | 3.28 | 17.69 | -16.47 | 102.03 | 15.65 | 216.25 | 0.4384 | 177.3 | 106.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.04 | 0.00 | 0.57 | -15.24 | 104.36 | 17.99 | 222.37 | 0.4440 | -435.0 | -279.5 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -16.19 | 104.25 | 17.88 | 220.74 | 0.4536 | 672.0 | 507.7 | |
| 0.60 | 8.46 | 0.34 | 4.71 | -16.66 | 104.20 | 17.82 | 219.96 | 0.4585 | 941.9 | 708.0 | |
| 0.00 | 5.27 | 0.00 | 2.90 | -15.11 | 104.03 | 17.65 | 222.05 | 0.4389 | -933.0 | -790.6 | |
| 4.23 | -3.00 | 2.36 | -3.00 | -16.78 | 104.05 | 17.67 | 219.54 | 0.4584 | 913.8 | 999999 | |
| 1.04 | 5.27 | 0.58 | 2.92 | -16.46 | 103.99 | 17.61 | 219.91 | 0.4541 | 999.1 | 738.5 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -16.39 | 103.59 | 17.21 | 219.38 | 0.4493 | 504.0 | 412.2 | |
| 0.00 | 1.55 | 0.00 | 0.85 | -16.78 | 100.95 | 14.57 | 214.30 | 0.4292 | 934.0 | 658.8 | |
| 0.00 | 3.46 | 0.00 | 1.89 | -16.68 | 100.65 | 14.27 | 213.90 | 0.4252 | 812.0 | 753.0 | |
| 0.00 | 1.30 | 0.00 | 0.70 | -17.13 | 95.06 | 8.69 | 201.84 | 0.3897 | -827.0 | -679.5 | |
| 0.00 | 2.25 | 0.00 | 1.21 | -16.94 | 94.99 | 8.61 | 201.87 | 0.3864 | -752.0 | -578.9 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -18.66 | 93.93 | 7.56 | 197.93 | 0.4064 | -650.0 | -508.3 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -18.79 | 91.38 | 5.00 | 192.03 | 0.3980 | -791.0 | -685.6 | |
| 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. | |