SDO HMI 2014-03-31 03:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.11 | 39.99 | 9.50 | 22.18 | -24.06 | 116.48 | 21.00 | 226.77 | 0.4509 | 398.4 | 16.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.63 | -23.33 | 117.78 | 22.30 | 229.69 | 0.4588 | 755.0 | 598.8 | |
| 13.16 | 17.19 | 7.33 | 9.57 | -23.62 | 117.55 | 22.07 | 228.90 | 0.4587 | 919.9 | 643.2 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -23.12 | 117.42 | 21.95 | 229.66 | 0.4528 | 696.0 | 470.5 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -24.44 | 117.41 | 21.93 | 227.29 | 0.4647 | 620.0 | 502.5 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -24.29 | 117.31 | 21.83 | 227.45 | 0.4621 | 762.0 | 617.7 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -23.73 | 117.14 | 21.66 | 228.23 | 0.4550 | 769.0 | 679.1 | |
| 0.00 | 0.61 | 0.00 | 0.34 | -24.49 | 117.10 | 21.62 | 226.85 | 0.4615 | 359.0 | 469.7 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -24.43 | 117.02 | 21.54 | 226.86 | 0.4601 | 501.0 | 508.4 | |
| 0.44 | 1.58 | 0.24 | 0.88 | -24.09 | 116.78 | 21.30 | 227.16 | 0.4542 | 841.2 | 749.1 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -24.80 | 115.43 | 19.95 | 224.20 | 0.4461 | -688.0 | -573.5 | |
| 0.00 | 1.75 | 0.00 | 0.97 | -24.75 | 115.00 | 19.52 | 223.71 | 0.4410 | -833.0 | -668.3 | |
| 3.51 | 10.00 | 1.93 | 5.49 | -24.61 | 114.59 | 19.11 | 223.40 | 0.4351 | -980.3 | -711.0 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -24.61 | 113.58 | 18.10 | 221.95 | 0.4244 | -667.0 | -515.1 | |
| 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. | |