SDO HMI 2014-01-13 06:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.01 | 159.01 | 21.42 | 81.11 | -17.97 | 30.17 | 2.01 | 187.99 | 0.2400 | 244.4 | 137.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.34 | 78.48 | 10.89 | 40.08 | -17.98 | 31.53 | 3.37 | 193.36 | 0.2431 | 1304.0 | 476.3 | |
| 1.19 | -1.00 | 0.61 | -1.00 | -18.31 | 31.20 | 3.03 | 191.77 | 0.2474 | 954.7 | 999999 | |
| 0.94 | -1.00 | 0.48 | -1.00 | -18.25 | 31.04 | 2.88 | 191.23 | 0.2458 | 969.4 | 999999 | |
| 1.62 | 4.68 | 0.82 | 2.38 | -17.37 | 31.00 | 2.83 | 191.84 | 0.2310 | 1164.9 | 840.5 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -17.71 | 30.97 | 2.81 | 191.43 | 0.2365 | 1018.0 | 840.8 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -16.95 | 30.87 | 2.70 | 191.70 | 0.2235 | 892.0 | 655.6 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -17.77 | 30.69 | 2.53 | 190.28 | 0.2366 | 930.0 | 668.6 | |
| 0.00 | 9.01 | 0.00 | 4.60 | -17.92 | 30.51 | 2.34 | 189.43 | 0.2387 | 617.0 | 729.8 | |
| 0.00 | 5.02 | 0.00 | 2.56 | -18.28 | 30.26 | 2.10 | 188.23 | 0.2441 | 708.0 | 623.1 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -17.68 | 29.64 | 1.48 | 186.08 | 0.2326 | -656.0 | -492.2 | |
| 0.00 | 1.79 | 0.00 | 0.91 | -18.38 | 29.12 | 0.95 | 183.73 | 0.2437 | -1002.0 | -774.7 | |
| 0.00 | 6.29 | 0.00 | 3.21 | -18.10 | 28.99 | 0.83 | 183.31 | 0.2389 | -959.0 | -784.4 | |
| 15.64 | 46.42 | 7.97 | 23.65 | -17.89 | 28.12 | -0.04 | 179.83 | 0.2349 | -1217.1 | -556.4 | |
| 1.28 | -13.00 | 0.65 | -13.00 | -18.19 | 27.94 | -0.23 | 179.09 | 0.2401 | -887.1 | 999999 | |
| 0.00 | 2.72 | 0.00 | 1.39 | -18.38 | 27.81 | -0.35 | 178.62 | 0.2432 | -765.0 | -633.2 | |
| 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. | |