SDO HMI 2014-01-03 10:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.24 | 55.27 | 11.00 | 35.73 | -12.63 | 118.58 | -39.10 | 105.92 | 0.6417 | 487.5 | 339.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.06 | 0.00 | 1.84 | -15.38 | 124.84 | -32.83 | 112.67 | 0.5687 | 611.0 | 513.5 | |
| 0.00 | 1.19 | 0.00 | 0.72 | -15.46 | 124.32 | -33.35 | 112.53 | 0.5759 | 670.0 | 518.6 | |
| 0.00 | 0.76 | 0.00 | 0.45 | -8.53 | 124.61 | -33.06 | 100.55 | 0.5510 | 699.0 | 606.7 | |
| 0.00 | 3.14 | 0.00 | 1.96 | -12.80 | 121.26 | -36.41 | 106.92 | 0.6073 | 711.0 | 558.8 | |
| 0.00 | 0.68 | 0.00 | 0.44 | -15.11 | 119.24 | -38.43 | 109.86 | 0.6403 | 571.0 | 485.5 | |
| 0.00 | 0.68 | 0.00 | 0.44 | -14.38 | 119.09 | -38.59 | 108.69 | 0.6401 | 739.0 | 552.2 | |
| 0.00 | 1.02 | 0.00 | 0.66 | -14.67 | 119.02 | -38.65 | 109.13 | 0.6418 | 677.0 | 497.9 | |
| 0.00 | 1.61 | 0.00 | 1.05 | -15.33 | 118.68 | -38.99 | 110.00 | 0.6481 | 548.0 | 433.3 | |
| 0.00 | 1.27 | 0.00 | 0.82 | -13.79 | 118.85 | -38.82 | 107.73 | 0.6415 | 645.0 | 611.0 | |
| 14.19 | 18.61 | 9.04 | 11.85 | -11.23 | 119.20 | -38.47 | 103.84 | 0.6308 | 919.4 | 602.5 | |
| 0.00 | 1.02 | 0.00 | 0.65 | -12.41 | 118.88 | -38.79 | 105.61 | 0.6376 | 787.0 | 627.8 | |
| 0.00 | 1.10 | 0.00 | 0.71 | -11.49 | 118.92 | -38.75 | 104.18 | 0.6349 | 583.0 | 448.5 | |
| 0.00 | 1.27 | 0.00 | 0.86 | -18.78 | 117.23 | -40.44 | 114.52 | 0.6773 | 574.0 | 541.5 | |
| 0.59 | 4.33 | 0.38 | 2.80 | -12.64 | 118.57 | -39.10 | 105.88 | 0.6422 | 875.6 | 603.3 | |
| 1.70 | 3.91 | 1.09 | 2.52 | -12.34 | 118.58 | -39.09 | 105.42 | 0.6413 | 950.3 | 726.1 | |
| 0.76 | -14.00 | 0.49 | -14.00 | -12.58 | 118.38 | -39.29 | 105.72 | 0.6444 | 583.1 | 999999 | |
| 0.00 | 1.10 | 0.00 | 0.71 | -11.53 | 118.34 | -39.34 | 104.10 | 0.6427 | 566.0 | 421.2 | |
| 0.00 | 1.36 | 0.00 | 0.88 | -12.32 | 118.04 | -39.63 | 105.25 | 0.6483 | 589.0 | 466.9 | |
| 0.00 | 1.36 | 0.00 | 0.88 | -11.12 | 117.74 | -39.93 | 103.33 | 0.6496 | 731.0 | 608.1 | |
| 0.00 | 0.76 | 0.00 | 0.50 | -11.20 | 117.57 | -40.10 | 103.42 | 0.6520 | 563.0 | 491.7 | |
| 0.00 | 1.27 | 0.00 | 0.85 | -12.38 | 116.44 | -41.24 | 104.95 | 0.6687 | -574.0 | -466.7 | |
| 0.00 | 1.02 | 0.00 | 0.69 | -13.05 | 114.95 | -42.72 | 105.58 | 0.6885 | -554.0 | -436.0 | |
| 0.00 | 0.85 | 0.00 | 0.61 | -13.88 | 111.65 | -46.03 | 106.03 | 0.7293 | -693.0 | -696.8 | |
| 0.00 | 1.27 | 0.00 | 0.92 | -14.11 | 111.54 | -46.13 | 106.33 | 0.7309 | -692.0 | -590.7 | |
| 0.00 | 0.93 | 0.00 | 0.68 | -13.66 | 111.44 | -46.23 | 105.69 | 0.7313 | -722.0 | -623.5 | |
| 0.00 | 1.02 | 0.00 | 0.74 | -13.77 | 111.23 | -46.44 | 105.80 | 0.7338 | -539.0 | -442.2 | |
| 0.00 | 0.68 | 0.00 | 0.50 | -12.27 | 110.50 | -47.17 | 103.64 | 0.7398 | -366.0 | -372.4 | |
| 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. | |