SDO HMI 2014-03-14 13:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 83.55 | 315.72 | 79.18 | 295.32 | 5.63 | 10.90 | 56.75 | 281.26 | 0.8503 | 297.8 | 93.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.12 | 10.51 | 7.94 | 11.71 | 4.87 | 16.74 | 62.58 | 279.08 | 0.8976 | -546.1 | -271.2 | |
| 0.00 | 0.61 | 0.00 | 0.67 | 4.35 | 16.46 | 62.31 | 278.57 | 0.8947 | -454.0 | -432.9 | |
| 0.00 | 0.69 | 0.00 | 0.76 | 4.54 | 16.30 | 62.14 | 278.82 | 0.8938 | -620.0 | -558.8 | |
| 0.00 | 2.26 | 0.00 | 2.39 | 5.20 | 15.14 | 60.98 | 279.79 | 0.8857 | -413.0 | -332.8 | |
| 0.00 | 3.13 | 0.00 | 3.26 | 4.20 | 14.86 | 60.70 | 278.73 | 0.8819 | -669.0 | -547.0 | |
| 0.00 | 1.65 | 0.00 | 1.72 | 4.97 | 14.67 | 60.51 | 279.63 | 0.8815 | -659.0 | -555.8 | |
| 1.22 | 3.56 | 1.24 | 3.62 | 5.58 | 13.86 | 59.70 | 280.49 | 0.8759 | -584.5 | -513.6 | |
| 7.64 | 12.51 | 7.79 | 12.76 | 6.03 | 13.76 | 59.60 | 281.01 | 0.8759 | -559.8 | -290.7 | |
| 0.00 | 2.69 | 0.00 | 2.75 | 6.45 | 13.72 | 59.56 | 281.50 | 0.8763 | -93.0 | -135.2 | |
| 0.00 | 1.74 | 0.00 | 1.66 | 4.72 | 11.81 | 57.66 | 279.98 | 0.8570 | 293.0 | 183.7 | |
| 1.30 | 275.33 | 1.23 | 253.07 | 3.75 | 11.53 | 57.37 | 278.93 | 0.8528 | -447.9 | 146.6 | |
| 5.73 | -11.00 | 5.38 | -11.00 | 4.41 | 11.22 | 57.06 | 279.77 | 0.8511 | -619.7 | 999999 | |
| 23.28 | -11.00 | 21.60 | -11.00 | 5.71 | 10.57 | 56.41 | 281.42 | 0.8478 | 680.2 | 999999 | |
| 1.82 | -11.00 | 1.68 | -11.00 | 5.15 | 10.38 | 56.22 | 280.81 | 0.8449 | 525.7 | 999999 | |
| 5.04 | -11.00 | 4.68 | -11.00 | 6.16 | 10.48 | 56.32 | 281.96 | 0.8478 | 566.4 | 999999 | |
| 6.69 | -11.00 | 6.05 | -11.00 | 4.90 | 9.81 | 55.65 | 280.67 | 0.8392 | 730.8 | 999999 | |
| 23.71 | -11.00 | 21.59 | -11.00 | 6.20 | 9.73 | 55.58 | 282.20 | 0.8411 | 872.6 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.95 | 8.01 | 9.48 | 55.32 | 284.37 | 0.8428 | 399.0 | 288.8 | |
| 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. | |