SDO HMI 2013-07-25 20:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 83.52 | 363.75 | 48.82 | 211.91 | -7.08 | 158.39 | 29.27 | 247.21 | 0.5277 | -143.7 | -67.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.79 | -9.14 | 163.73 | 34.61 | 247.42 | 0.6096 | 630.0 | 559.4 | |
| 0.00 | 1.81 | 0.00 | 1.13 | -9.54 | 163.59 | 34.47 | 246.72 | 0.6099 | 566.0 | 494.1 | |
| 1.54 | 72.11 | 0.94 | 43.90 | -7.25 | 162.92 | 33.80 | 249.91 | 0.5897 | 644.3 | 661.3 | |
| 1.45 | -3.00 | 0.88 | -3.00 | -6.75 | 162.84 | 33.72 | 250.68 | 0.5864 | 826.6 | 999999 | |
| 16.67 | -3.00 | 10.16 | -3.00 | -7.11 | 162.57 | 33.45 | 249.94 | 0.5845 | 1050.8 | 999999 | |
| 1.72 | 3.17 | 1.06 | 1.95 | -8.89 | 162.59 | 33.47 | 247.11 | 0.5936 | 736.2 | 578.6 | |
| 0.00 | 1.00 | 0.00 | 0.61 | -9.23 | 162.48 | 33.36 | 246.51 | 0.5940 | 362.0 | 335.7 | |
| 0.36 | 1.54 | 0.22 | 0.93 | -8.11 | 161.56 | 32.44 | 247.70 | 0.5761 | 896.8 | 739.0 | |
| 0.00 | 0.82 | 0.00 | 0.48 | -7.50 | 159.88 | 30.76 | 247.63 | 0.5504 | 660.0 | 489.8 | |
| 0.00 | 1.36 | 0.00 | 0.82 | -10.46 | 160.12 | 31.00 | 242.95 | 0.5709 | 580.0 | 478.5 | |
| 11.51 | 38.14 | 6.78 | 22.36 | -6.62 | 159.67 | 30.55 | 249.01 | 0.5430 | 867.1 | 722.5 | |
| 1.63 | -11.00 | 0.95 | -11.00 | -6.18 | 159.04 | 29.92 | 249.36 | 0.5320 | 925.1 | 999999 | |
| 0.00 | 2.08 | 0.00 | 1.22 | -7.45 | 158.92 | 29.80 | 247.05 | 0.5371 | -585.0 | -468.7 | |
| 0.00 | 1.90 | 0.00 | 1.11 | -5.79 | 158.63 | 29.51 | 249.79 | 0.5243 | 375.0 | 546.9 | |
| 0.54 | 3.35 | 0.32 | 1.94 | -5.72 | 158.45 | 29.33 | 249.79 | 0.5214 | 965.8 | 750.1 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -9.76 | 158.69 | 29.57 | 242.98 | 0.5480 | 716.0 | 624.9 | |
| 0.00 | 2.63 | 0.00 | 1.53 | -7.27 | 158.44 | 29.32 | 247.02 | 0.5297 | -709.0 | -481.8 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -6.27 | 158.38 | 29.26 | 248.75 | 0.5233 | 278.0 | 274.6 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -5.70 | 158.13 | 29.01 | 249.61 | 0.5169 | 387.0 | 346.0 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -8.29 | 158.27 | 29.15 | 245.13 | 0.5334 | -486.0 | -325.2 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -7.47 | 158.11 | 28.99 | 246.42 | 0.5263 | -666.0 | -506.8 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -7.84 | 158.03 | 28.91 | 245.72 | 0.5274 | -818.0 | -664.2 | |
| 0.00 | 0.91 | 0.00 | 0.53 | -8.00 | 157.97 | 28.85 | 245.41 | 0.5275 | -605.0 | -519.0 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -8.24 | 157.74 | 28.62 | 244.81 | 0.5259 | -670.0 | -587.4 | |
| 0.00 | 2.26 | 0.00 | 1.30 | -6.21 | 157.60 | 28.48 | 248.33 | 0.5122 | -438.0 | -392.6 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -6.39 | 157.44 | 28.32 | 247.88 | 0.5109 | -808.0 | -574.9 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -7.25 | 157.28 | 28.17 | 246.21 | 0.5138 | -30.0 | -108.7 | |
| 0.00 | 2.26 | 0.00 | 1.30 | -6.06 | 157.18 | 28.06 | 248.29 | 0.5055 | -514.0 | -530.0 | |
| 2.54 | 215.44 | 1.46 | 123.22 | -6.68 | 157.11 | 27.99 | 247.10 | 0.5080 | -690.1 | -455.7 | |
| 2.26 | -29.00 | 1.29 | -29.00 | -6.51 | 156.68 | 27.56 | 247.10 | 0.5011 | -881.9 | 999999 | |
| 1.72 | -29.00 | 0.98 | -29.00 | -6.35 | 156.67 | 27.55 | 247.38 | 0.5000 | -799.9 | 999999 | |
| 35.33 | -29.00 | 20.22 | -29.00 | -7.21 | 156.48 | 27.36 | 245.64 | 0.5026 | -1174.0 | 999999 | |
| 2.26 | -29.00 | 1.29 | -29.00 | -6.67 | 156.17 | 27.05 | 246.40 | 0.4950 | -1154.9 | 999999 | |
| 2.72 | -29.00 | 1.55 | -29.00 | -7.45 | 156.12 | 27.00 | 244.92 | 0.4990 | -883.3 | 999999 | |
| 1.27 | -29.00 | 0.72 | -29.00 | -6.48 | 156.06 | 26.94 | 246.66 | 0.4922 | -1101.6 | 999999 | |
| 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. | |