SDO HMI 2014-01-17 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 |
| 17.69 | 62.95 | 16.69 | 58.77 | -17.67 | 31.08 | 57.77 | 252.09 | 0.8488 | 161.1 | -106.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.47 | 0.00 | 2.41 | -17.36 | 32.76 | 59.45 | 252.64 | 0.8632 | -269.0 | -197.3 | |
| 2.38 | 37.60 | 2.28 | 36.20 | -16.97 | 32.19 | 58.88 | 253.04 | 0.8581 | 533.5 | 84.0 | |
| 11.99 | -2.00 | 11.51 | -2.00 | -17.49 | 32.22 | 58.91 | 252.44 | 0.8588 | 628.2 | 999999 | |
| 0.00 | 2.21 | 0.00 | 2.09 | -17.69 | 31.60 | 58.29 | 252.15 | 0.8536 | 75.0 | 163.3 | |
| 0.00 | 0.60 | 0.00 | 0.55 | -17.04 | 30.81 | 57.50 | 252.83 | 0.8461 | 392.0 | 310.0 | |
| 0.00 | 0.94 | 0.00 | 0.86 | -17.19 | 30.77 | 57.46 | 252.64 | 0.8459 | 364.0 | 338.5 | |
| 0.00 | 1.70 | 0.00 | 1.56 | -18.81 | 30.43 | 57.12 | 250.69 | 0.8445 | -506.0 | -444.1 | |
| 0.00 | 0.51 | 0.00 | 0.45 | -17.76 | 29.17 | 55.86 | 251.78 | 0.8320 | -360.0 | -332.0 | |
| 0.51 | 1.53 | 0.45 | 1.35 | -18.23 | 28.95 | 55.64 | 251.18 | 0.8305 | -433.7 | -318.3 | |
| 1.87 | 4.17 | 1.64 | 3.65 | -18.29 | 28.59 | 55.28 | 251.07 | 0.8273 | -537.8 | -449.2 | |
| 0.94 | 5.44 | 0.81 | 4.71 | -18.29 | 28.10 | 54.79 | 251.00 | 0.8227 | -648.5 | -562.2 | |
| 0.00 | 3.23 | 0.00 | 2.78 | -18.44 | 27.69 | 54.38 | 250.76 | 0.8190 | -647.0 | -531.6 | |
| 0.00 | 1.02 | 0.00 | 0.87 | -18.43 | 27.41 | 54.10 | 250.73 | 0.8164 | -486.0 | -387.2 | |
| 0.00 | 1.53 | 0.00 | 1.29 | -18.23 | 27.06 | 53.75 | 250.91 | 0.8128 | -673.0 | -514.6 | |
| 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. | |