SDO HMI 2014-05-15 08:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.27 | 71.05 | 12.75 | 39.05 | 8.42 | 195.11 | -23.21 | 64.16 | 0.4347 | -135.4 | 117.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.87 | 24.52 | 5.88 | 13.27 | 8.06 | 197.08 | -21.23 | 63.02 | 0.4041 | -1104.3 | -724.8 | |
| 0.00 | 1.89 | 0.00 | 1.02 | 7.41 | 197.02 | -21.30 | 64.55 | 0.4006 | -987.0 | -805.0 | |
| 1.44 | -1.00 | 0.78 | -1.00 | 7.81 | 196.90 | -21.42 | 63.76 | 0.4050 | -950.2 | 999999 | |
| 1.08 | -1.00 | 0.58 | -1.00 | 8.06 | 196.85 | -21.46 | 63.26 | 0.4074 | -770.8 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 8.40 | 196.77 | -21.55 | 62.60 | 0.4110 | -476.0 | -481.1 | |
| 0.00 | 2.42 | 0.00 | 1.32 | 8.50 | 196.37 | -21.95 | 62.81 | 0.4174 | -937.0 | -751.5 | |
| 0.00 | 3.95 | 0.00 | 2.16 | 8.63 | 195.90 | -22.42 | 63.01 | 0.4250 | -844.0 | -460.4 | |
| 0.00 | 2.07 | 0.00 | 1.15 | 9.78 | 194.24 | -24.07 | 62.29 | 0.4559 | 513.0 | 519.3 | |
| 0.00 | 6.65 | 0.00 | 3.69 | 9.01 | 194.20 | -24.12 | 63.87 | 0.4514 | 972.0 | 790.7 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 9.54 | 194.13 | -24.19 | 62.88 | 0.4559 | 861.0 | 729.5 | |
| 1.44 | 2.78 | 0.80 | 1.55 | 9.05 | 193.76 | -24.56 | 64.19 | 0.4578 | 898.2 | 746.5 | |
| 0.00 | 1.44 | 0.00 | 0.80 | 8.71 | 193.51 | -24.81 | 65.08 | 0.4591 | 810.0 | 695.7 | |
| 5.03 | 22.90 | 2.80 | 12.76 | 8.35 | 193.27 | -25.05 | 66.02 | 0.4604 | 980.5 | 696.3 | |
| 3.41 | -13.00 | 1.91 | -13.00 | 8.57 | 193.15 | -25.17 | 65.68 | 0.4634 | 782.7 | 999999 | |
| 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. | |