| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.14 | 420.89 | 39.88 | 220.55 | 12.51 | 13.64 | -2.13 | 6.46 | 0.3252 | -997.0 | -378.6 | |
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back to the solar disc SDO HMI 2014-04-06 04:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.32 | 0.00 | 0.70 | 14.35 | 15.25 | -0.52 | 1.43 | 0.3535 | 837.0 | 695.1 | |
| 75.17 | 398.80 | 39.37 | 209.02 | 12.57 | 13.75 | -2.02 | 6.09 | 0.3259 | -1477.2 | -424.5 | |
| 0.00 | 0.62 | 0.00 | 0.32 | 10.27 | 13.09 | -2.68 | 9.19 | 0.2894 | 792.0 | 666.4 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 3.76 | 13.03 | -2.74 | 15.34 | 0.1811 | 803.0 | 597.8 | |
| 0.00 | 1.32 | 0.00 | 0.68 | 9.52 | 12.61 | -3.16 | 11.32 | 0.2784 | 925.0 | 782.2 | |
| 0.00 | 1.67 | 0.00 | 0.88 | 12.96 | 12.48 | -3.29 | 9.65 | 0.3351 | -601.0 | -506.5 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 12.67 | 12.48 | -3.28 | 9.78 | 0.3304 | -698.0 | -602.1 | |
| 0.00 | 1.94 | 0.00 | 1.00 | 9.90 | 12.42 | -3.35 | 11.69 | 0.2853 | 879.0 | 629.6 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 11.85 | 11.94 | -3.83 | 11.88 | 0.3188 | -707.0 | -629.4 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 12.36 | 11.59 | -4.17 | 12.57 | 0.3282 | -587.0 | -492.3 | |
| 0.00 | 2.46 | 0.00 | 1.29 | 11.42 | 11.18 | -4.59 | 14.50 | 0.3146 | 860.0 | 728.8 | |
| 0.97 | 3.08 | 0.51 | 1.62 | 12.65 | 10.94 | -4.83 | 14.23 | 0.3354 | 1031.9 | 783.9 | |
| 0.00 | 1.94 | 0.00 | 1.01 | 11.90 | 10.62 | -5.15 | 15.77 | 0.3247 | 1042.0 | 799.0 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 9.56 | 9.22 | -6.55 | 22.48 | 0.2956 | 711.0 | 486.9 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 11.84 | 8.18 | -7.59 | 22.65 | 0.3370 | 657.0 | 510.5 | |
| 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. | |