SDO HMI 2014-03-14 11:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.82 | 122.67 | 50.95 | 112.61 | 11.16 | 9.82 | 54.57 | 288.22 | 0.8435 | -146.6 | -108.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.89 | 32.49 | 24.90 | 31.23 | 11.65 | 11.48 | 56.23 | 288.24 | 0.8592 | -636.0 | -304.6 | |
| 0.00 | 1.39 | 0.00 | 1.29 | 10.23 | 10.47 | 55.22 | 286.95 | 0.8471 | 402.0 | 260.6 | |
| 0.00 | 1.22 | 0.00 | 1.15 | 11.83 | 10.83 | 55.57 | 288.65 | 0.8541 | -661.0 | -587.0 | |
| 0.00 | 3.82 | 0.00 | 3.58 | 11.27 | 10.55 | 55.29 | 288.10 | 0.8503 | -458.0 | -471.8 | |
| 1.56 | 2.87 | 1.48 | 2.71 | 12.18 | 10.67 | 55.41 | 289.10 | 0.8537 | -373.5 | -284.6 | |
| 5.99 | 60.73 | 5.57 | 54.84 | 11.67 | 10.18 | 54.93 | 288.67 | 0.8482 | -695.4 | -106.1 | |
| 3.48 | 5.82 | 3.15 | 5.28 | 10.28 | 9.69 | 54.44 | 287.24 | 0.8402 | 481.5 | 259.5 | |
| 0.00 | 1.04 | 0.00 | 0.95 | 10.71 | 9.65 | 54.39 | 287.75 | 0.8409 | 171.0 | 71.5 | |
| 11.29 | -6.00 | 10.06 | -6.00 | 10.44 | 8.85 | 53.60 | 287.70 | 0.8330 | 763.4 | 999999 | |
| 0.78 | -6.00 | 0.70 | -6.00 | 10.82 | 8.95 | 53.70 | 288.11 | 0.8350 | 516.0 | 999999 | |
| 2.52 | -6.00 | 2.24 | -6.00 | 10.92 | 8.72 | 53.46 | 288.30 | 0.8331 | 541.1 | 999999 | |
| 0.00 | 3.48 | 0.00 | 3.12 | 11.43 | 8.86 | 53.60 | 288.85 | 0.8358 | -585.0 | -475.6 | |
| 2.09 | 3.56 | 1.80 | 3.08 | 11.01 | 7.48 | 52.22 | 288.83 | 0.8219 | 557.9 | 378.4 | |
| 1.22 | 3.21 | 1.05 | 2.77 | 11.60 | 7.08 | 51.83 | 289.65 | 0.8200 | 622.1 | 458.9 | |
| 0.00 | 3.04 | 0.00 | 2.61 | 11.61 | 6.89 | 51.63 | 289.73 | 0.8182 | 620.0 | 402.4 | |
| 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. | |