SDO HMI 2014-08-15 07:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.87 | 44.00 | 8.86 | 26.18 | -17.54 | 105.22 | 23.64 | 223.64 | 0.5559 | 438.7 | 426.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.26 | 0.00 | 0.76 | -17.45 | 106.25 | 24.66 | 224.98 | 0.5653 | 528.0 | 444.9 | |
| 4.96 | 13.80 | 2.96 | 8.24 | -17.15 | 106.03 | 24.45 | 225.14 | 0.5600 | 960.7 | 729.6 | |
| 1.44 | -2.00 | 0.86 | -2.00 | -17.51 | 106.01 | 24.43 | 224.64 | 0.5634 | 768.6 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.70 | -17.46 | 105.76 | 24.18 | 224.41 | 0.5604 | 854.0 | 779.3 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -17.93 | 105.83 | 24.24 | 223.88 | 0.5658 | 470.0 | 342.8 | |
| 0.00 | 0.72 | 0.00 | 0.43 | -17.76 | 105.73 | 24.15 | 223.99 | 0.5631 | 640.0 | 623.8 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -17.42 | 105.55 | 23.96 | 224.21 | 0.5578 | 886.0 | 819.8 | |
| 2.25 | 3.79 | 1.36 | 2.28 | -18.39 | 105.61 | 24.03 | 223.05 | 0.5682 | 781.4 | 574.3 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -17.71 | 105.45 | 23.86 | 223.71 | 0.5598 | 757.0 | 571.2 | |
| 0.45 | 12.90 | 0.27 | 7.67 | -17.60 | 105.22 | 23.64 | 223.59 | 0.5564 | 973.0 | 714.0 | |
| 4.24 | -10.00 | 2.52 | -10.00 | -17.76 | 105.04 | 23.45 | 223.16 | 0.5561 | 924.1 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -18.48 | 104.16 | 22.58 | 221.18 | 0.5552 | -408.0 | -318.3 | |
| 0.00 | 1.53 | 0.00 | 0.91 | -18.35 | 103.56 | 21.97 | 220.57 | 0.5480 | -792.0 | -659.6 | |
| 1.53 | 3.52 | 0.89 | 2.05 | -16.61 | 103.27 | 21.68 | 222.45 | 0.5266 | -887.3 | -662.8 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -17.04 | 102.50 | 20.92 | 220.87 | 0.5237 | -811.0 | -664.3 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -17.89 | 102.12 | 20.54 | 219.28 | 0.5295 | -753.0 | -551.1 | |
| 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. | |