SDO HMI 2014-03-15 15:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.21 | 238.40 | 78.80 | 388.90 | 5.35 | 11.45 | 71.57 | 277.94 | 0.9548 | 164.2 | -1.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.04 | 0.00 | 2.56 | 4.63 | 17.54 | 77.67 | 276.24 | 0.9805 | -148.0 | -151.8 | |
| 0.00 | 1.04 | 0.00 | 2.62 | 5.07 | 17.73 | 77.85 | 276.67 | 0.9813 | -125.0 | -79.8 | |
| 3.74 | 19.03 | 7.15 | 36.47 | 6.30 | 13.84 | 73.96 | 278.52 | 0.9671 | -227.0 | -49.4 | |
| 0.00 | 1.04 | 0.00 | 1.81 | 2.69 | 12.84 | 72.96 | 274.97 | 0.9599 | 280.0 | 234.3 | |
| 7.21 | 46.83 | 12.39 | 79.15 | 3.62 | 12.50 | 72.62 | 275.98 | 0.9590 | -454.8 | -298.0 | |
| 1.39 | -5.00 | 2.37 | -5.00 | 3.22 | 12.42 | 72.54 | 275.57 | 0.9583 | -270.9 | 999999 | |
| 8.77 | 165.59 | 14.57 | 260.23 | 5.10 | 11.67 | 71.80 | 277.64 | 0.9560 | -169.1 | 93.9 | |
| 0.00 | 0.70 | 0.00 | 1.21 | 6.84 | 12.26 | 72.38 | 279.33 | 0.9603 | -44.0 | -43.4 | |
| 10.25 | -7.00 | 16.40 | -7.00 | 6.03 | 10.81 | 70.93 | 278.75 | 0.9523 | 405.6 | 999999 | |
| 0.00 | 1.30 | 0.00 | 1.99 | 5.09 | 10.09 | 70.21 | 277.90 | 0.9476 | 495.0 | 455.5 | |
| 11.73 | -7.00 | 18.28 | -7.00 | 6.36 | 10.27 | 70.39 | 279.18 | 0.9498 | 669.4 | 999999 | |
| 1.91 | -7.00 | 2.85 | -7.00 | 4.61 | 9.61 | 69.74 | 277.47 | 0.9446 | 576.9 | 999999 | |
| 3.21 | -7.00 | 4.79 | -7.00 | 4.96 | 9.52 | 69.64 | 277.86 | 0.9444 | 637.6 | 999999 | |
| 0.00 | 0.70 | 0.00 | 1.05 | 7.11 | 9.46 | 69.58 | 280.12 | 0.9461 | 463.0 | 388.0 | |
| 0.00 | 1.13 | 0.00 | 1.81 | 10.79 | 9.92 | 70.04 | 283.84 | 0.9523 | -56.0 | -59.3 | |
| 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. | |