SDO HMI 2014-08-11 16:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.17 | 58.27 | 8.54 | 37.61 | -17.80 | 161.63 | 32.12 | 232.06 | 0.6444 | 622.3 | 495.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.54 | 0.00 | 0.37 | -19.23 | 164.39 | 34.88 | 232.51 | 0.6828 | 638.0 | 476.8 | |
| 12.72 | 39.25 | 8.25 | 25.37 | -17.04 | 162.48 | 32.97 | 233.77 | 0.6472 | 902.6 | 576.6 | |
| 0.00 | 2.44 | 0.00 | 1.58 | -18.63 | 161.40 | 31.89 | 230.84 | 0.6479 | 858.0 | 700.3 | |
| 0.00 | 1.89 | 0.00 | 1.20 | -17.31 | 160.58 | 31.07 | 231.81 | 0.6290 | 660.0 | 576.9 | |
| 0.00 | 0.81 | 0.00 | 0.53 | -20.09 | 160.66 | 31.15 | 228.38 | 0.6520 | 635.0 | 612.3 | |
| 0.00 | 3.43 | 0.00 | 2.22 | -19.71 | 160.50 | 30.99 | 228.71 | 0.6474 | 683.0 | 607.0 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -19.87 | 160.38 | 30.87 | 228.41 | 0.6475 | 562.0 | 562.7 | |
| 0.45 | 1.71 | 0.29 | 1.10 | -19.52 | 160.12 | 30.61 | 228.60 | 0.6420 | 744.8 | 663.8 | |
| 0.00 | 1.08 | 0.00 | 0.70 | -19.47 | 159.88 | 30.37 | 228.45 | 0.6392 | 667.0 | 655.2 | |
| 0.00 | 1.17 | 0.00 | 0.76 | -20.57 | 159.63 | 30.12 | 226.88 | 0.6459 | 687.0 | 512.3 | |
| 0.00 | 1.26 | 0.00 | 0.80 | -18.75 | 159.11 | 29.60 | 228.63 | 0.6254 | 318.0 | 394.0 | |
| 0.00 | 0.90 | 0.00 | 0.57 | -18.52 | 158.62 | 29.11 | 228.46 | 0.6185 | 684.0 | 555.0 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -20.25 | 157.63 | 28.12 | 225.35 | 0.6238 | -597.0 | -426.2 | |
| 0.00 | 2.53 | 0.00 | 1.60 | -20.60 | 157.22 | 27.71 | 224.52 | 0.6230 | -799.0 | -603.0 | |
| 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. | |