SDO HMI 2014-02-24 16:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.48 | 123.30 | 19.94 | 119.22 | 8.36 | 132.55 | -57.11 | 75.73 | 0.8588 | 363.5 | 138.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.84 | 0.00 | 2.19 | 7.45 | 141.59 | -48.06 | 74.04 | 0.7694 | -659.0 | -564.5 | |
| 0.00 | 1.55 | 0.00 | 1.23 | 8.19 | 140.52 | -49.13 | 73.49 | 0.7830 | -662.0 | -534.3 | |
| 0.00 | 1.12 | 0.00 | 0.89 | 8.60 | 140.40 | -49.25 | 73.03 | 0.7854 | -625.0 | -532.9 | |
| 0.00 | 1.12 | 0.00 | 0.90 | 8.77 | 140.24 | -49.42 | 72.88 | 0.7877 | -373.0 | -357.3 | |
| 0.00 | 1.03 | 0.00 | 0.85 | 8.87 | 138.95 | -50.71 | 73.21 | 0.8009 | -511.0 | -443.9 | |
| 6.54 | 110.22 | 6.34 | 107.93 | 8.85 | 132.37 | -57.29 | 75.25 | 0.8618 | 794.0 | 183.5 | |
| 0.86 | -6.00 | 0.82 | -6.00 | 7.69 | 132.63 | -57.03 | 76.49 | 0.8571 | 726.4 | 999999 | |
| 0.43 | 1.55 | 0.41 | 1.47 | 6.87 | 132.62 | -57.03 | 77.43 | 0.8555 | -415.0 | -309.4 | |
| 0.69 | -6.00 | 0.68 | -6.00 | 8.77 | 131.93 | -57.72 | 75.45 | 0.8653 | 407.5 | 999999 | |
| 0.00 | 2.75 | 0.00 | 2.65 | 7.09 | 132.25 | -57.41 | 77.27 | 0.8592 | 316.0 | 202.6 | |
| 11.19 | -6.00 | 10.93 | -6.00 | 8.22 | 131.95 | -57.70 | 76.07 | 0.8640 | 647.7 | 999999 | |
| 0.77 | -6.00 | 0.76 | -6.00 | 8.56 | 131.87 | -57.78 | 75.70 | 0.8654 | 462.9 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.26 | 9.16 | 131.49 | -58.16 | 75.14 | 0.8697 | -220.0 | -183.7 | |
| 0.00 | 0.86 | 0.00 | 0.85 | 7.24 | 131.42 | -58.23 | 77.31 | 0.8665 | 501.0 | 468.5 | |
| 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. | |