SDO HMI 2014-10-01 22:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.91 | 340.41 | 99.61 | 620.23 | -10.93 | 244.90 | 72.27 | 256.50 | 0.9590 | 122.8 | 86.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.94 | 0.00 | 5.22 | -10.48 | 250.46 | 77.82 | 257.97 | 0.9836 | -140.0 | -142.6 | |
| 0.00 | 0.97 | 0.00 | 2.55 | -11.56 | 250.12 | 77.48 | 256.83 | 0.9831 | -173.0 | -197.6 | |
| 27.82 | 184.42 | 62.00 | 405.62 | -10.73 | 248.09 | 75.46 | 257.33 | 0.9758 | 206.2 | 131.8 | |
| 9.42 | -3.00 | 19.53 | -3.00 | -10.96 | 247.05 | 74.42 | 256.93 | 0.9719 | 769.7 | 999999 | |
| 0.00 | 2.73 | 0.00 | 5.26 | -11.82 | 245.87 | 73.23 | 255.85 | 0.9677 | 463.0 | 416.4 | |
| 0.00 | 13.64 | 0.00 | 28.03 | -12.97 | 246.63 | 73.99 | 254.82 | 0.9717 | 193.0 | 273.1 | |
| 0.00 | 15.32 | 0.00 | 27.00 | -10.46 | 244.59 | 71.95 | 257.00 | 0.9608 | 622.0 | 371.2 | |
| 0.00 | 7.83 | 0.00 | 14.05 | -10.98 | 244.79 | 72.16 | 256.51 | 0.9622 | 574.0 | 457.6 | |
| 0.00 | 0.26 | 0.00 | 0.55 | -13.52 | 246.51 | 73.88 | 254.24 | 0.9716 | 186.0 | 160.7 | |
| 0.00 | 0.70 | 0.00 | 1.36 | -13.03 | 245.58 | 72.94 | 254.56 | 0.9674 | 116.0 | 100.2 | |
| 0.00 | 1.41 | 0.00 | 2.78 | -13.57 | 245.89 | 73.26 | 254.07 | 0.9692 | -105.0 | -46.5 | |
| 0.53 | 2.29 | 0.86 | 3.74 | -11.76 | 242.94 | 70.31 | 255.35 | 0.9541 | -217.2 | -175.5 | |
| 0.00 | 0.88 | 0.00 | 1.37 | -14.95 | 241.32 | 68.69 | 251.73 | 0.9493 | 77.0 | 178.2 | |
| 0.00 | 1.50 | 0.00 | 1.88 | -11.91 | 237.19 | 64.55 | 253.97 | 0.9210 | -42.0 | -118.2 | |
| 0.00 | 0.70 | 0.00 | 0.97 | -15.08 | 238.55 | 65.92 | 250.95 | 0.9342 | -200.0 | -202.0 | |
| 0.00 | 1.58 | 0.00 | 2.15 | -15.22 | 238.33 | 65.69 | 250.76 | 0.9330 | -187.0 | -189.7 | |
| 14.26 | 81.78 | 16.29 | 93.70 | -10.68 | 234.83 | 62.20 | 254.71 | 0.9029 | -664.0 | -178.5 | |
| 0.00 | 1.41 | 0.00 | 1.61 | -11.77 | 234.52 | 61.88 | 253.46 | 0.9025 | -384.0 | -405.0 | |
| 0.00 | 1.50 | 0.00 | 1.70 | -11.82 | 234.34 | 61.71 | 253.36 | 0.9013 | -402.0 | -354.3 | |
| 0.00 | 3.17 | 0.00 | 3.53 | -11.18 | 233.90 | 61.27 | 253.95 | 0.8970 | -488.0 | -401.7 | |
| 0.00 | 1.23 | 0.00 | 1.32 | -9.69 | 233.09 | 60.46 | 255.37 | 0.8882 | -164.0 | -206.0 | |
| 0.88 | 3.79 | 0.93 | 3.97 | -9.40 | 232.64 | 60.00 | 255.58 | 0.8841 | 91.2 | -130.0 | |
| 0.00 | 2.99 | 0.00 | 3.25 | -11.17 | 233.20 | 60.57 | 253.78 | 0.8917 | -403.0 | -392.9 | |
| 0.00 | 1.94 | 0.00 | 2.01 | -9.79 | 232.20 | 59.57 | 255.04 | 0.8814 | -488.0 | -416.2 | |
| 0.00 | 3.17 | 0.00 | 3.30 | -10.18 | 232.14 | 59.50 | 254.58 | 0.8817 | -501.0 | -489.5 | |
| 0.00 | 2.38 | 0.00 | 2.48 | -10.74 | 232.07 | 59.44 | 253.96 | 0.8822 | -288.0 | -355.7 | |
| 0.00 | 0.88 | 0.00 | 0.83 | -16.71 | 226.63 | 54.00 | 245.62 | 0.8528 | -232.0 | -254.7 | |
| 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. | |