SDO HMI 2014-08-04 16:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.16 | 25.44 | 2.40 | 14.55 | -19.33 | 238.29 | 16.22 | 211.64 | 0.5026 | -118.3 | -160.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.72 | 0.00 | 1.03 | -20.75 | 243.81 | 21.74 | 218.00 | 0.5647 | 439.0 | 371.8 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -17.72 | 242.13 | 20.06 | 219.49 | 0.5158 | 880.0 | 757.8 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -18.06 | 242.14 | 20.07 | 219.07 | 0.5196 | 659.0 | 501.9 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -18.46 | 240.55 | 18.48 | 216.31 | 0.5098 | 564.0 | 499.9 | |
| 4.16 | 5.97 | 2.40 | 3.44 | -19.12 | 240.25 | 18.18 | 215.08 | 0.5150 | 955.7 | 671.9 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -19.80 | 239.45 | 17.38 | 213.11 | 0.5165 | 701.0 | 629.9 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -19.64 | 237.78 | 15.71 | 210.71 | 0.5013 | -547.0 | -443.1 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -19.20 | 237.67 | 15.60 | 211.02 | 0.4948 | -641.0 | -506.0 | |
| 0.00 | 2.17 | 0.00 | 1.25 | -20.58 | 237.23 | 15.16 | 208.87 | 0.5092 | -710.0 | -579.3 | |
| 0.00 | 0.54 | 0.00 | 0.30 | -18.11 | 236.77 | 14.70 | 210.76 | 0.4736 | -868.0 | -771.5 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -19.21 | 236.67 | 14.60 | 209.37 | 0.4872 | -388.0 | -296.1 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -19.73 | 236.25 | 14.18 | 208.13 | 0.4911 | -834.0 | -574.3 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -19.73 | 236.05 | 13.98 | 207.80 | 0.4896 | -783.0 | -646.8 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -20.02 | 234.51 | 12.44 | 204.87 | 0.4832 | -558.0 | -494.2 | |
| 0.00 | 1.99 | 0.00 | 1.11 | -18.63 | 234.08 | 12.01 | 205.42 | 0.4612 | -818.0 | -670.9 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -19.17 | 233.89 | 11.82 | 204.56 | 0.4673 | -862.0 | -702.1 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -18.83 | 233.76 | 11.69 | 204.65 | 0.4618 | -704.0 | -505.5 | |
| 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. | |