SDO HMI 2014-03-12 00:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.34 | 371.58 | 96.67 | 497.20 | 14.16 | 52.83 | 65.19 | 288.54 | 0.9280 | -18.6 | -3.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.88 | 125.40 | 19.36 | 200.76 | 13.57 | 57.34 | 69.70 | 286.79 | 0.9537 | -73.7 | -18.6 | |
| 0.00 | 1.30 | 0.00 | 2.02 | 12.79 | 56.58 | 68.95 | 286.16 | 0.9489 | -272.0 | -302.8 | |
| 0.00 | 0.95 | 0.00 | 1.47 | 12.92 | 56.41 | 68.77 | 286.33 | 0.9482 | -408.0 | -387.2 | |
| 17.43 | -1.00 | 26.99 | -1.00 | 13.67 | 56.36 | 68.72 | 287.11 | 0.9488 | -470.6 | 999999 | |
| 1.21 | 1.99 | 1.82 | 2.98 | 13.00 | 55.78 | 68.15 | 286.56 | 0.9449 | -538.4 | -518.4 | |
| 0.00 | 0.52 | 0.00 | 0.74 | 11.86 | 54.83 | 67.19 | 285.59 | 0.9381 | -442.0 | -441.7 | |
| 0.00 | 1.13 | 0.00 | 1.68 | 13.23 | 55.58 | 67.95 | 286.84 | 0.9441 | -524.0 | -539.4 | |
| 0.00 | 5.29 | 0.00 | 7.66 | 13.11 | 55.10 | 67.47 | 286.82 | 0.9413 | -479.0 | -467.2 | |
| 0.00 | 2.34 | 0.00 | 3.42 | 14.50 | 54.89 | 67.25 | 288.31 | 0.9420 | -344.0 | -316.4 | |
| 0.00 | 1.30 | 0.00 | 1.79 | 14.93 | 53.51 | 65.88 | 289.10 | 0.9348 | 66.0 | 54.0 | |
| 0.00 | 1.39 | 0.00 | 1.92 | 15.16 | 53.58 | 65.94 | 289.32 | 0.9355 | 157.0 | 117.1 | |
| 7.37 | 116.55 | 9.48 | 147.13 | 13.74 | 52.17 | 64.54 | 288.19 | 0.9248 | 271.7 | -70.7 | |
| 9.71 | -12.00 | 12.28 | -12.00 | 14.07 | 51.56 | 63.93 | 288.70 | 0.9215 | 432.6 | 999999 | |
| 1.30 | -12.00 | 1.63 | -12.00 | 14.58 | 51.34 | 63.70 | 289.29 | 0.9210 | -582.2 | 999999 | |
| 0.95 | -12.00 | 1.17 | -12.00 | 13.76 | 50.78 | 63.14 | 288.58 | 0.9159 | -347.2 | 999999 | |
| 3.90 | -12.00 | 4.88 | -12.00 | 14.81 | 51.11 | 63.48 | 289.59 | 0.9199 | -356.0 | 999999 | |
| 1.13 | -12.00 | 1.35 | -12.00 | 13.66 | 50.19 | 62.55 | 288.63 | 0.9118 | 152.5 | 999999 | |
| 0.69 | 20.03 | 0.85 | 24.40 | 15.08 | 50.43 | 62.79 | 290.06 | 0.9160 | -568.8 | -288.2 | |
| 0.52 | 2.34 | 0.63 | 2.82 | 14.76 | 50.13 | 62.49 | 289.81 | 0.9134 | -367.2 | -403.8 | |
| 0.00 | 1.47 | 0.00 | 1.75 | 14.74 | 49.72 | 62.08 | 289.91 | 0.9106 | -454.0 | -460.5 | |
| 0.00 | 1.30 | 0.00 | 1.56 | 16.01 | 49.65 | 62.02 | 291.26 | 0.9126 | 307.0 | 232.7 | |
| 0.00 | 1.99 | 0.00 | 2.24 | 14.50 | 48.11 | 60.48 | 290.11 | 0.8990 | 351.0 | 261.3 | |
| 0.00 | 0.95 | 0.00 | 1.12 | 16.27 | 48.87 | 61.24 | 291.77 | 0.9079 | 105.0 | 85.0 | |
| 0.00 | 1.82 | 0.00 | 2.07 | 15.28 | 48.30 | 60.66 | 290.89 | 0.9019 | -234.0 | -204.0 | |
| 0.43 | 4.77 | 0.49 | 5.38 | 14.97 | 48.08 | 60.45 | 290.62 | 0.8997 | 409.8 | 192.0 | |
| 0.00 | 0.87 | 0.00 | 0.96 | 14.59 | 47.84 | 60.21 | 290.29 | 0.8972 | 403.0 | 363.8 | |
| 0.00 | 3.90 | 0.00 | 4.44 | 15.59 | 48.26 | 60.63 | 291.23 | 0.9023 | -154.0 | -147.6 | |
| 0.00 | 2.34 | 0.00 | 2.70 | 16.25 | 48.48 | 60.84 | 291.87 | 0.9052 | 356.0 | 272.7 | |
| 1.73 | 5.38 | 1.96 | 6.07 | 15.81 | 47.93 | 60.29 | 291.56 | 0.9005 | 322.5 | 174.4 | |
| 0.00 | 8.59 | 0.00 | 9.46 | 15.39 | 47.28 | 59.65 | 291.31 | 0.8949 | -333.0 | 202.1 | |
| 0.00 | 0.87 | 0.00 | 0.95 | 15.12 | 47.16 | 59.52 | 291.06 | 0.8934 | 495.0 | 475.7 | |
| 0.78 | 33.47 | 0.84 | 35.34 | 14.99 | 46.55 | 58.92 | 291.11 | 0.8887 | 436.0 | 437.4 | |
| 3.21 | -32.00 | 3.38 | -32.00 | 14.75 | 46.15 | 58.51 | 290.98 | 0.8851 | 734.2 | 999999 | |
| 1.82 | -32.00 | 1.93 | -32.00 | 15.22 | 46.12 | 58.48 | 291.50 | 0.8860 | 567.3 | 999999 | |
| 7.28 | 23.33 | 7.63 | 24.37 | 15.55 | 45.62 | 57.98 | 292.01 | 0.8830 | 640.6 | 452.2 | |
| 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. | |