| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.79 | 224.35 | 34.69 | 127.68 | -13.15 | 120.84 | -22.10 | 132.01 | 0.4947 | 518.8 | 247.0 | |
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back to the solar disc SDO HMI 2014-10-04 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 |
| 31.06 | 190.83 | 17.56 | 108.06 | -13.01 | 121.68 | -21.26 | 132.85 | 0.4839 | 1224.5 | 370.3 | |
| 5.19 | -1.00 | 2.93 | -1.00 | -12.55 | 121.42 | -21.52 | 131.78 | 0.4821 | 999.7 | 999999 | |
| 8.09 | -1.00 | 4.61 | -1.00 | -13.43 | 120.94 | -22.00 | 132.51 | 0.4963 | 886.9 | 999999 | |
| 3.43 | -1.00 | 1.96 | -1.00 | -13.38 | 120.65 | -22.29 | 132.06 | 0.4991 | 707.3 | 999999 | |
| 1.32 | -1.00 | 0.76 | -1.00 | -13.55 | 120.36 | -22.58 | 131.96 | 0.5039 | 763.3 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.81 | -13.55 | 119.73 | -23.21 | 131.16 | 0.5111 | -662.0 | -429.6 | |
| 0.00 | 2.20 | 0.00 | 1.27 | -12.89 | 118.79 | -24.16 | 129.04 | 0.5157 | 862.0 | 684.3 | |
| 0.79 | 1.85 | 0.47 | 1.09 | -15.30 | 118.03 | -24.91 | 131.72 | 0.5465 | -884.3 | -724.2 | |
| 0.00 | 0.35 | 0.00 | 0.21 | -14.08 | 117.94 | -25.00 | 129.87 | 0.5362 | -629.0 | -595.2 | |
| 1.67 | 25.60 | 0.98 | 15.00 | -13.68 | 117.64 | -25.30 | 128.94 | 0.5359 | -954.3 | -693.4 | |
| 0.35 | 1.23 | 0.21 | 0.73 | -15.23 | 117.45 | -25.49 | 130.98 | 0.5522 | -741.5 | -591.8 | |
| 2.20 | -10.00 | 1.29 | -10.00 | -13.66 | 117.48 | -25.46 | 128.72 | 0.5376 | -914.6 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -12.57 | 117.46 | -25.48 | 127.07 | 0.5283 | -719.0 | -524.5 | |
| 6.69 | -10.00 | 3.92 | -10.00 | -13.28 | 117.31 | -25.63 | 127.99 | 0.5362 | -999.1 | 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. | |