SDO HMI 2014-08-04 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.55 | 319.68 | 76.49 | 295.62 | 9.23 | 172.97 | -57.90 | 82.84 | 0.8442 | 329.0 | 120.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.54 | 0.00 | 0.41 | 3.94 | 182.06 | -48.81 | 90.01 | 0.7530 | -508.0 | -437.5 | |
| 0.00 | 0.90 | 0.00 | 0.72 | 7.13 | 178.74 | -52.12 | 85.63 | 0.7877 | -481.0 | -380.3 | |
| 0.00 | 1.99 | 0.00 | 1.60 | 6.73 | 178.71 | -52.16 | 86.13 | 0.7883 | -555.0 | -456.8 | |
| 1.27 | 33.37 | 1.03 | 27.27 | 9.85 | 177.91 | -52.96 | 82.16 | 0.7960 | -991.6 | -567.0 | |
| 4.43 | -4.00 | 3.63 | -4.00 | 10.20 | 177.67 | -53.19 | 81.72 | 0.7985 | -769.1 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.68 | 12.34 | 176.99 | -53.87 | 79.07 | 0.8058 | -239.0 | -258.4 | |
| 6.87 | -4.00 | 5.65 | -4.00 | 9.94 | 177.53 | -53.34 | 82.04 | 0.8000 | -756.7 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.11 | 9.61 | 177.55 | -53.31 | 82.47 | 0.7998 | -463.0 | -428.0 | |
| 0.00 | 0.54 | 0.00 | 0.44 | 7.02 | 177.80 | -53.07 | 85.72 | 0.7978 | -362.0 | -365.2 | |
| 0.00 | 1.18 | 0.00 | 0.99 | 10.36 | 176.58 | -54.28 | 81.53 | 0.8097 | -523.0 | -532.4 | |
| 2.62 | 7.14 | 2.21 | 6.04 | 9.89 | 176.43 | -54.43 | 82.11 | 0.8112 | -629.4 | -410.5 | |
| 0.00 | 2.17 | 0.00 | 1.84 | 10.23 | 176.13 | -54.73 | 81.69 | 0.8142 | -378.0 | -349.7 | |
| 0.00 | 1.09 | 0.00 | 0.93 | 10.95 | 175.56 | -55.30 | 80.81 | 0.8199 | -373.0 | -257.8 | |
| 3.62 | 31.83 | 3.13 | 27.61 | 10.05 | 175.42 | -55.45 | 81.91 | 0.8213 | -19.2 | 82.0 | |
| 0.00 | 1.54 | 0.00 | 1.33 | 9.71 | 175.45 | -55.42 | 82.32 | 0.8210 | -35.0 | -18.3 | |
| 0.45 | 8.32 | 0.40 | 7.33 | 10.09 | 174.47 | -56.40 | 81.85 | 0.8305 | 832.0 | 584.1 | |
| 0.00 | 0.36 | 0.00 | 0.32 | 10.03 | 174.20 | -56.67 | 81.91 | 0.8331 | 372.0 | 295.2 | |
| 0.00 | 0.90 | 0.00 | 0.81 | 9.79 | 173.81 | -57.06 | 82.21 | 0.8368 | 543.0 | 414.0 | |
| 0.00 | 5.43 | 0.00 | 4.90 | 9.56 | 173.64 | -57.23 | 82.48 | 0.8384 | 769.0 | 596.7 | |
| 0.00 | 2.44 | 0.00 | 2.24 | 11.27 | 173.09 | -57.78 | 80.44 | 0.8434 | 80.0 | 68.7 | |
| 0.00 | 0.99 | 0.00 | 0.92 | 11.25 | 172.56 | -58.30 | 80.46 | 0.8483 | 483.0 | 387.8 | |
| 2.71 | 7.87 | 2.50 | 7.25 | 9.53 | 172.95 | -57.91 | 82.50 | 0.8448 | 667.3 | 522.3 | |
| 0.00 | 0.36 | 0.00 | 0.33 | 6.49 | 173.28 | -57.59 | 86.12 | 0.8428 | 469.0 | 452.5 | |
| 0.00 | 4.79 | 0.00 | 4.53 | 10.86 | 171.97 | -58.90 | 80.92 | 0.8536 | 604.0 | 488.7 | |
| 4.70 | 200.78 | 4.41 | 193.20 | 9.34 | 172.23 | -58.63 | 82.70 | 0.8514 | 690.4 | 190.6 | |
| 1.90 | -25.00 | 1.79 | -25.00 | 9.21 | 172.09 | -58.77 | 82.86 | 0.8528 | 770.8 | 999999 | |
| 2.35 | -25.00 | 2.23 | -25.00 | 9.38 | 171.98 | -58.88 | 82.65 | 0.8537 | 771.4 | 999999 | |
| 0.00 | 2.26 | 0.00 | 2.12 | 7.99 | 172.21 | -58.65 | 84.30 | 0.8520 | 196.0 | 147.3 | |
| 18.36 | -25.00 | 17.43 | -25.00 | 9.00 | 171.85 | -59.02 | 83.09 | 0.8550 | 815.8 | 999999 | |
| 7.14 | -25.00 | 6.79 | -25.00 | 8.56 | 171.78 | -59.09 | 83.60 | 0.8558 | 737.3 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.70 | 10.64 | 171.19 | -59.68 | 81.17 | 0.8606 | 298.0 | 322.8 | |
| 2.89 | -25.00 | 2.78 | -25.00 | 8.47 | 171.44 | -59.43 | 83.70 | 0.8588 | 677.0 | 999999 | |
| 4.07 | -25.00 | 3.93 | -25.00 | 9.13 | 171.20 | -59.66 | 82.92 | 0.8607 | 521.9 | 999999 | |
| 16.73 | -25.00 | 16.19 | -25.00 | 8.61 | 171.22 | -59.65 | 83.53 | 0.8607 | 528.6 | 999999 | |
| 2.44 | -25.00 | 2.39 | -25.00 | 9.00 | 170.80 | -60.06 | 83.06 | 0.8642 | 289.8 | 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. | |