SDO HMI 2014-04-06 03:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.45 | 408.16 | 39.02 | 213.97 | 12.52 | 13.62 | -2.69 | 8.14 | 0.3267 | -979.0 | -401.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.92 | 388.01 | 38.74 | 203.45 | 12.59 | 13.74 | -2.57 | 7.73 | 0.3275 | -1421.5 | -436.4 | |
| 0.00 | 1.85 | 0.00 | 0.93 | 3.76 | 13.01 | -3.31 | 18.34 | 0.1840 | 972.0 | 681.0 | |
| 0.00 | 2.29 | 0.00 | 1.20 | 12.95 | 12.44 | -3.87 | 11.32 | 0.3369 | -656.0 | -526.8 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 12.67 | 12.20 | -4.11 | 12.19 | 0.3331 | -559.0 | -454.2 | |
| 0.00 | 0.97 | 0.00 | 0.50 | 9.80 | 12.24 | -4.08 | 14.22 | 0.2865 | 781.0 | 616.1 | |
| 0.00 | 2.02 | 0.00 | 1.06 | 11.85 | 12.00 | -4.32 | 13.35 | 0.3206 | -808.0 | -632.6 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 12.36 | 11.62 | -4.70 | 14.07 | 0.3303 | -510.0 | -444.3 | |
| 0.00 | 2.02 | 0.00 | 1.06 | 12.04 | 11.32 | -5.00 | 15.20 | 0.3265 | -343.0 | -217.1 | |
| 0.00 | 1.67 | 0.00 | 0.87 | 11.41 | 11.21 | -5.11 | 16.06 | 0.3169 | 778.0 | 703.7 | |
| 0.53 | 1.50 | 0.28 | 0.79 | 12.65 | 11.06 | -5.26 | 15.44 | 0.3372 | 878.0 | 734.3 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 12.46 | 10.82 | -5.50 | 16.27 | 0.3354 | 843.0 | 706.6 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 11.93 | 10.61 | -5.70 | 17.33 | 0.3279 | 974.0 | 820.9 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 10.68 | 9.41 | -6.91 | 22.13 | 0.3152 | 784.0 | 589.7 | |
| 0.00 | 1.76 | 0.00 | 0.92 | 9.70 | 8.42 | -7.90 | 26.32 | 0.3070 | 761.0 | 517.8 | |
| 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. | |