SDO HMI 2014-10-09 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.58 | 31.76 | 6.24 | 17.26 | -13.19 | 60.72 | -14.61 | 143.48 | 0.4133 | 554.5 | 208.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.48 | -14.62 | 63.09 | -12.24 | 149.93 | 0.4111 | 607.0 | 525.3 | |
| 2.81 | 17.46 | 1.51 | 9.42 | -12.83 | 61.96 | -13.37 | 145.20 | 0.3967 | 1168.5 | 809.4 | |
| 4.39 | -2.00 | 2.37 | -2.00 | -13.09 | 61.91 | -13.42 | 145.48 | 0.4005 | 998.9 | 999999 | |
| 2.19 | -2.00 | 1.18 | -2.00 | -12.84 | 61.77 | -13.56 | 144.83 | 0.3985 | 1036.1 | 999999 | |
| 2.19 | -2.00 | 1.18 | -2.00 | -12.84 | 61.58 | -13.75 | 144.46 | 0.4004 | 887.6 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -13.01 | 61.35 | -13.98 | 144.25 | 0.4046 | 652.0 | 538.6 | |
| 0.00 | 1.67 | 0.00 | 0.91 | -14.13 | 60.83 | -14.50 | 144.89 | 0.4239 | 809.0 | 595.5 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -14.03 | 60.17 | -15.16 | 143.52 | 0.4286 | 915.0 | 695.6 | |
| 0.00 | 4.65 | 0.00 | 2.52 | -11.95 | 59.66 | -15.66 | 139.44 | 0.4080 | -1049.0 | -851.6 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -14.38 | 58.99 | -16.34 | 141.96 | 0.4442 | 777.0 | 587.8 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -14.14 | 58.36 | -16.97 | 140.57 | 0.4475 | -849.0 | -664.8 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -15.15 | 57.17 | -18.16 | 140.11 | 0.4710 | 701.0 | 614.5 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -15.28 | 56.96 | -18.37 | 139.98 | 0.4746 | 662.0 | 445.8 | |
| 0.00 | 0.26 | 0.00 | 0.16 | -12.79 | 46.28 | -29.04 | 123.49 | 0.5699 | -622.0 | -537.7 | |
| 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. | |