SDO HMI 2014-09-30 05:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.76 | 33.00 | 0.89 | 16.73 | 7.76 | 207.73 | 12.56 | 275.52 | 0.2176 | 21.9 | 229.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.59 | 0.00 | 0.82 | 7.58 | 210.62 | 15.45 | 273.98 | 0.2658 | -866.0 | -769.3 | |
| 0.00 | 2.03 | 0.00 | 1.04 | 7.71 | 210.25 | 15.08 | 274.54 | 0.2597 | -807.0 | -818.0 | |
| 0.00 | 1.15 | 0.00 | 0.59 | 7.71 | 210.09 | 14.92 | 274.59 | 0.2571 | -838.0 | -764.2 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 6.22 | 209.73 | 14.56 | 268.69 | 0.2510 | -793.0 | -642.0 | |
| 0.00 | 1.15 | 0.00 | 0.59 | 7.22 | 209.51 | 14.34 | 272.70 | 0.2471 | -760.0 | -520.9 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 6.61 | 208.81 | 13.63 | 270.14 | 0.2352 | -884.0 | -611.7 | |
| 0.00 | 1.85 | 0.00 | 0.94 | 6.59 | 208.37 | 13.20 | 270.02 | 0.2278 | -1079.0 | -886.6 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 6.73 | 207.97 | 12.80 | 270.56 | 0.2210 | -884.0 | -695.3 | |
| 0.00 | 1.68 | 0.00 | 0.85 | 8.51 | 207.38 | 12.20 | 279.00 | 0.2126 | 613.0 | 483.2 | |
| 0.00 | 10.94 | 0.00 | 5.53 | 8.10 | 207.05 | 11.88 | 277.21 | 0.2063 | 824.0 | 805.0 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 7.84 | 206.67 | 11.50 | 276.09 | 0.1995 | 976.0 | 780.2 | |
| 0.79 | 2.73 | 0.40 | 1.38 | 8.65 | 206.67 | 11.49 | 280.13 | 0.2010 | 1016.6 | 802.8 | |
| 0.00 | 2.12 | 0.00 | 1.07 | 7.03 | 206.47 | 11.29 | 272.04 | 0.1953 | 1092.0 | 823.4 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 7.61 | 206.39 | 11.21 | 275.00 | 0.1944 | 773.0 | 523.8 | |
| 0.97 | 2.38 | 0.49 | 1.20 | 8.36 | 206.38 | 11.20 | 278.86 | 0.1954 | 1045.2 | 776.9 | |
| 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. | |