SDO HMI 2014-08-04 04:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.77 | 349.55 | 73.83 | 305.12 | 9.24 | 172.90 | -55.77 | 82.88 | 0.8239 | 232.7 | 144.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.83 | 11.50 | 182.85 | -45.82 | 79.77 | 0.7164 | -671.0 | -539.6 | |
| 0.00 | 1.00 | 0.00 | 0.76 | 6.71 | 178.80 | -49.87 | 86.29 | 0.7632 | -681.0 | -569.0 | |
| 0.00 | 0.90 | 0.00 | 0.69 | 7.16 | 178.68 | -49.99 | 85.69 | 0.7643 | -651.0 | -520.7 | |
| 2.80 | 34.93 | 2.18 | 27.25 | 9.86 | 177.91 | -50.76 | 82.16 | 0.7725 | -974.2 | -548.6 | |
| 3.44 | -4.00 | 2.69 | -4.00 | 10.27 | 177.62 | -51.05 | 81.63 | 0.7757 | -761.9 | 999999 | |
| 11.94 | -4.00 | 9.34 | -4.00 | 10.05 | 177.57 | -51.10 | 81.92 | 0.7762 | -740.6 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.63 | 7.99 | 177.92 | -50.75 | 84.59 | 0.7725 | -54.0 | -148.0 | |
| 0.00 | 1.09 | 0.00 | 0.85 | 6.88 | 177.85 | -50.81 | 86.02 | 0.7736 | -466.0 | -436.1 | |
| 0.00 | 1.81 | 0.00 | 1.45 | 10.40 | 176.59 | -52.08 | 81.48 | 0.7868 | -689.0 | -586.5 | |
| 2.35 | 8.51 | 1.88 | 6.82 | 9.93 | 176.45 | -52.22 | 82.08 | 0.7883 | -757.6 | -475.7 | |
| 0.00 | 3.26 | 0.00 | 2.63 | 10.18 | 176.13 | -52.53 | 81.76 | 0.7916 | -401.0 | -322.9 | |
| 0.00 | 7.33 | 0.00 | 5.96 | 10.61 | 175.77 | -52.89 | 81.22 | 0.7954 | -336.0 | -311.0 | |
| 0.00 | 1.09 | 0.00 | 0.89 | 11.00 | 175.62 | -53.04 | 80.73 | 0.7970 | -419.0 | -292.7 | |
| 1.90 | 26.15 | 1.55 | 21.53 | 10.03 | 175.50 | -53.17 | 81.95 | 0.7982 | 49.3 | 191.6 | |
| 0.00 | 2.35 | 0.00 | 1.93 | 9.75 | 175.41 | -53.26 | 82.30 | 0.7992 | 104.0 | 122.3 | |
| 0.00 | 0.81 | 0.00 | 0.67 | 6.45 | 175.62 | -53.05 | 86.44 | 0.7978 | -353.0 | -270.2 | |
| 0.00 | 2.17 | 0.00 | 1.78 | 4.74 | 175.63 | -53.03 | 88.59 | 0.7987 | -461.0 | -356.0 | |
| 1.18 | 9.50 | 0.98 | 7.93 | 10.17 | 174.52 | -54.15 | 81.78 | 0.8083 | 785.2 | 566.4 | |
| 0.00 | 1.18 | 0.00 | 1.00 | 10.80 | 173.93 | -54.74 | 81.00 | 0.8142 | 627.0 | 541.8 | |
| 0.00 | 1.45 | 0.00 | 1.25 | 11.35 | 173.18 | -55.49 | 80.33 | 0.8217 | -279.0 | -148.8 | |
| 0.00 | 1.36 | 0.00 | 1.15 | 7.07 | 174.16 | -54.50 | 85.60 | 0.8125 | 495.0 | 445.9 | |
| 0.00 | 4.80 | 0.00 | 4.11 | 9.69 | 173.57 | -55.10 | 82.36 | 0.8179 | 834.0 | 691.1 | |
| 1.45 | 7.51 | 1.25 | 6.51 | 9.47 | 173.13 | -55.54 | 82.63 | 0.8222 | 731.1 | 602.3 | |
| 0.00 | 0.63 | 0.00 | 0.56 | 11.33 | 172.63 | -56.04 | 80.36 | 0.8271 | 572.0 | 422.9 | |
| 0.00 | 1.99 | 0.00 | 1.77 | 10.80 | 172.11 | -56.56 | 81.01 | 0.8320 | 440.0 | 319.7 | |
| 2.80 | 225.75 | 2.48 | 204.38 | 9.43 | 172.36 | -56.31 | 82.66 | 0.8297 | 758.1 | 218.2 | |
| 0.36 | 1.27 | 0.32 | 1.13 | 10.96 | 171.83 | -56.83 | 80.82 | 0.8346 | 608.0 | 532.4 | |
| 11.94 | -26.00 | 10.69 | -26.00 | 9.23 | 171.79 | -56.88 | 82.89 | 0.8352 | 838.1 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.66 | 10.65 | 171.18 | -57.49 | 81.18 | 0.8408 | 425.0 | 361.1 | |
| 32.03 | -26.00 | 28.95 | -26.00 | 8.71 | 171.46 | -57.21 | 83.50 | 0.8384 | 696.3 | 999999 | |
| 5.25 | -26.00 | 4.77 | -26.00 | 9.19 | 171.29 | -57.38 | 82.93 | 0.8399 | 584.5 | 999999 | |
| 1.81 | -26.00 | 1.66 | -26.00 | 9.37 | 170.89 | -57.77 | 82.71 | 0.8436 | 402.0 | 999999 | |
| 2.99 | -26.00 | 2.75 | -26.00 | 9.05 | 170.80 | -57.87 | 83.08 | 0.8445 | 249.9 | 999999 | |
| 2.26 | -26.00 | 2.09 | -26.00 | 8.73 | 170.70 | -57.96 | 83.45 | 0.8455 | -342.7 | 999999 | |
| 0.27 | -26.00 | 0.25 | -26.00 | 8.57 | 170.62 | -58.04 | 83.64 | 0.8462 | -355.0 | 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. | |