SDO HMI 2014-09-02 19:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.68 | 55.15 | 13.22 | 39.28 | -17.82 | 158.18 | -38.96 | 123.54 | 0.7201 | 183.1 | -8.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.94 | 26.46 | 9.74 | 18.48 | -17.56 | 159.34 | -37.80 | 123.99 | 0.7070 | 826.7 | 402.5 | |
| 0.00 | 4.47 | 0.00 | 3.12 | -17.06 | 159.06 | -38.08 | 123.18 | 0.7067 | 563.0 | 485.8 | |
| 0.00 | 1.34 | 0.00 | 0.95 | -18.33 | 158.53 | -38.60 | 124.37 | 0.7199 | -177.0 | -151.9 | |
| 0.00 | 1.61 | 0.00 | 1.12 | -16.28 | 158.88 | -38.25 | 122.10 | 0.7039 | 398.0 | 431.3 | |
| 0.00 | 0.80 | 0.00 | 0.58 | -17.53 | 157.72 | -39.42 | 122.88 | 0.7232 | -219.0 | -146.7 | |
| 0.00 | 0.89 | 0.00 | 0.64 | -17.56 | 157.42 | -39.71 | 122.72 | 0.7263 | 503.0 | 428.2 | |
| 1.34 | 3.58 | 0.98 | 2.60 | -18.23 | 156.95 | -40.19 | 123.22 | 0.7349 | -798.9 | -454.3 | |
| 0.00 | 0.45 | 0.00 | 0.33 | -18.98 | 156.73 | -40.40 | 123.97 | 0.7414 | -699.0 | -626.6 | |
| 0.72 | 2.95 | 0.52 | 2.16 | -18.61 | 156.67 | -40.47 | 123.51 | 0.7399 | -797.1 | -728.4 | |
| 0.00 | 1.70 | 0.00 | 1.26 | -18.91 | 156.37 | -40.76 | 123.67 | 0.7445 | -439.0 | -337.8 | |
| 0.00 | 1.43 | 0.00 | 1.05 | -18.43 | 156.51 | -40.62 | 123.19 | 0.7404 | -831.0 | -645.9 | |
| 1.79 | 4.20 | 1.32 | 3.10 | -18.52 | 156.28 | -40.86 | 123.15 | 0.7432 | -605.0 | -480.2 | |
| 0.89 | 3.04 | 0.66 | 2.24 | -18.22 | 156.28 | -40.86 | 122.79 | 0.7415 | -796.7 | -589.7 | |
| 0.00 | 2.23 | 0.00 | 1.65 | -18.13 | 156.09 | -41.04 | 122.58 | 0.7428 | -561.0 | -458.8 | |
| 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. | |