SDO HMI 2014-05-16 18:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.80 | 39.90 | 4.50 | 20.38 | -15.50 | 193.81 | -5.78 | 156.64 | 0.2468 | 431.5 | 379.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.60 | -16.81 | 195.00 | -4.59 | 162.80 | 0.2600 | 771.0 | 623.4 | |
| 5.57 | 9.88 | 2.85 | 5.06 | -16.34 | 194.95 | -4.64 | 162.04 | 0.2527 | 1078.3 | 815.3 | |
| 0.00 | 1.08 | 0.00 | 0.54 | -12.84 | 194.97 | -4.62 | 156.37 | 0.1969 | -833.0 | -682.6 | |
| 0.00 | 0.45 | 0.00 | 0.23 | -16.81 | 194.84 | -4.74 | 162.24 | 0.2608 | 774.0 | 603.0 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -15.19 | 194.60 | -4.99 | 159.10 | 0.2363 | 742.0 | 588.1 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -12.59 | 194.57 | -5.02 | 154.02 | 0.1959 | -977.0 | -802.6 | |
| 0.00 | 2.07 | 0.00 | 1.06 | -16.40 | 194.41 | -5.18 | 160.19 | 0.2566 | 770.0 | 721.8 | |
| 0.00 | 0.81 | 0.00 | 0.41 | -15.03 | 194.01 | -5.58 | 156.60 | 0.2376 | 861.0 | 788.6 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -15.09 | 193.81 | -5.77 | 156.00 | 0.2399 | 1079.0 | 913.5 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -14.93 | 193.69 | -5.89 | 155.28 | 0.2383 | 879.0 | 746.1 | |
| 0.00 | 1.35 | 0.00 | 0.69 | -15.83 | 193.25 | -6.33 | 155.31 | 0.2552 | -578.0 | -396.7 | |
| 0.99 | 10.15 | 0.50 | 5.18 | -15.27 | 193.21 | -6.38 | 154.16 | 0.2470 | 1000.2 | 827.9 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -14.84 | 192.78 | -6.81 | 151.83 | 0.2437 | 836.0 | 640.7 | |
| 2.24 | 7.00 | 1.15 | 3.59 | -15.36 | 192.45 | -7.14 | 151.73 | 0.2542 | -1051.4 | -689.4 | |
| 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. | |