SDO HMI 2014-10-01 13:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89.11 | 508.01 | 125.59 | 720.81 | -11.45 | 244.95 | 67.35 | 255.00 | 0.9345 | 79.3 | 123.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.25 | 232.07 | 61.05 | 376.39 | -10.74 | 248.19 | 70.59 | 256.46 | 0.9545 | 209.4 | 106.5 | |
| 11.27 | -1.00 | 17.41 | -1.00 | -11.04 | 246.99 | 69.39 | 255.92 | 0.9486 | 769.6 | 999999 | |
| 4.40 | 44.65 | 6.34 | 63.40 | -11.09 | 245.49 | 67.89 | 255.56 | 0.9403 | 513.9 | 432.1 | |
| 0.00 | 3.96 | 0.00 | 6.28 | -13.76 | 246.91 | 69.31 | 253.10 | 0.9511 | 448.0 | 396.8 | |
| 0.53 | -3.00 | 0.75 | -3.00 | -10.74 | 245.16 | 67.56 | 255.85 | 0.9380 | 493.5 | 999999 | |
| 0.62 | 18.94 | 0.95 | 29.44 | -13.56 | 246.52 | 68.92 | 253.22 | 0.9488 | 61.7 | 209.3 | |
| 0.00 | 3.70 | 0.00 | 5.54 | -13.05 | 245.95 | 68.36 | 253.62 | 0.9452 | 135.0 | 129.4 | |
| 1.94 | 54.87 | 2.98 | 86.25 | -13.94 | 246.33 | 68.74 | 252.78 | 0.9483 | 486.6 | 338.3 | |
| 5.28 | -8.00 | 8.27 | -8.00 | -14.38 | 246.53 | 68.93 | 252.37 | 0.9499 | 456.2 | 999999 | |
| 0.00 | 6.43 | 0.00 | 9.30 | -13.03 | 245.19 | 67.59 | 253.48 | 0.9410 | 59.0 | 153.4 | |
| 0.00 | 0.97 | 0.00 | 1.41 | -13.41 | 245.25 | 67.65 | 253.09 | 0.9418 | -187.0 | -133.6 | |
| 0.00 | 1.41 | 0.00 | 1.98 | -12.38 | 244.67 | 67.08 | 254.04 | 0.9372 | 318.0 | 272.4 | |
| 1.23 | 7.13 | 1.62 | 9.37 | -11.38 | 243.34 | 65.74 | 254.79 | 0.9278 | -72.8 | 2.5 | |
| 1.23 | -13.00 | 1.61 | -13.00 | -11.65 | 243.16 | 65.56 | 254.47 | 0.9270 | -227.9 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.91 | -11.42 | 243.05 | 65.46 | 254.69 | 0.9261 | -569.0 | -519.4 | |
| 0.00 | 1.76 | 0.00 | 2.23 | -13.80 | 241.85 | 64.26 | 251.89 | 0.9220 | 171.0 | 136.1 | |
| 0.00 | 0.62 | 0.00 | 0.73 | -14.29 | 239.94 | 62.34 | 250.88 | 0.9102 | 131.0 | 148.9 | |
| 0.00 | 1.06 | 0.00 | 1.21 | -13.79 | 239.18 | 61.58 | 251.21 | 0.9040 | 285.0 | 234.0 | |
| 0.00 | 1.06 | 0.00 | 1.15 | -11.32 | 238.11 | 60.51 | 253.60 | 0.8916 | -151.0 | -158.7 | |
| 0.00 | 1.67 | 0.00 | 1.76 | -12.02 | 237.00 | 59.41 | 252.54 | 0.8845 | -352.0 | -272.4 | |
| 0.00 | 1.14 | 0.00 | 1.19 | -12.26 | 236.61 | 59.01 | 252.16 | 0.8819 | -147.0 | -155.3 | |
| 17.61 | 98.82 | 17.19 | 96.77 | -10.57 | 234.77 | 57.17 | 253.52 | 0.8635 | -766.0 | -130.4 | |
| 0.00 | 0.97 | 0.00 | 0.95 | -12.10 | 234.68 | 57.08 | 251.79 | 0.8661 | -416.0 | -376.0 | |
| 2.73 | 4.58 | 2.65 | 4.44 | -11.77 | 234.29 | 56.69 | 252.03 | 0.8621 | -542.7 | -386.3 | |
| 3.17 | 5.46 | 3.03 | 5.23 | -11.02 | 233.95 | 56.35 | 252.78 | 0.8575 | -719.6 | -528.5 | |
| 0.00 | 0.88 | 0.00 | 0.84 | -11.28 | 233.75 | 56.15 | 252.43 | 0.8564 | -619.0 | -555.4 | |
| 0.00 | 0.62 | 0.00 | 0.58 | -10.27 | 233.30 | 55.70 | 253.44 | 0.8501 | -508.0 | -445.0 | |
| 0.00 | 1.85 | 0.00 | 1.72 | -10.00 | 233.12 | 55.52 | 253.69 | 0.8479 | -245.0 | -229.6 | |
| 1.85 | 4.23 | 1.74 | 3.99 | -11.18 | 233.39 | 55.79 | 252.43 | 0.8530 | -699.5 | -535.5 | |
| 0.00 | 0.88 | 0.00 | 0.80 | -9.79 | 232.53 | 54.93 | 253.77 | 0.8421 | -516.0 | -460.9 | |
| 0.00 | 2.55 | 0.00 | 2.33 | -10.17 | 232.30 | 54.70 | 253.26 | 0.8410 | -674.0 | -567.2 | |
| 0.00 | 1.50 | 0.00 | 1.35 | -9.47 | 232.13 | 54.53 | 254.02 | 0.8378 | -519.0 | -440.5 | |
| 0.00 | 0.97 | 0.00 | 0.86 | -8.63 | 231.84 | 54.24 | 254.90 | 0.8331 | -489.0 | -422.2 | |
| 0.00 | 1.06 | 0.00 | 0.96 | -10.72 | 232.18 | 54.58 | 252.59 | 0.8413 | -626.0 | -528.9 | |
| 0.00 | 1.50 | 0.00 | 1.45 | -16.01 | 232.90 | 55.30 | 246.86 | 0.8614 | -435.0 | -312.8 | |
| 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. | |