SDO HMI 2014-10-04 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.58 | 188.45 | 34.11 | 114.09 | -12.47 | 163.01 | 29.40 | 236.83 | 0.5745 | 211.2 | 146.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.78 | -11.30 | 167.59 | 33.99 | 242.33 | 0.6212 | 675.0 | 565.1 | |
| 0.00 | 1.05 | 0.00 | 0.77 | -24.42 | 170.29 | 36.69 | 227.76 | 0.7371 | 486.0 | 369.4 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -13.87 | 166.27 | 32.67 | 237.70 | 0.6223 | 755.0 | 581.3 | |
| 0.00 | 2.28 | 0.00 | 1.43 | -13.24 | 165.88 | 32.28 | 238.27 | 0.6135 | 678.0 | 622.6 | |
| 0.35 | 1.23 | 0.22 | 0.76 | -11.76 | 165.42 | 31.82 | 240.06 | 0.5979 | -335.5 | -180.8 | |
| 8.44 | 111.59 | 5.19 | 68.36 | -12.45 | 164.83 | 31.23 | 238.57 | 0.5955 | 947.9 | 388.9 | |
| 0.00 | 0.53 | 0.00 | 0.33 | -14.78 | 164.95 | 31.35 | 235.36 | 0.6137 | 697.0 | 635.3 | |
| 15.11 | -6.00 | 9.26 | -6.00 | -12.21 | 164.55 | 30.94 | 238.69 | 0.5904 | 1041.1 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.75 | -11.15 | 164.27 | 30.67 | 240.05 | 0.5798 | 717.0 | 583.4 | |
| 4.83 | -6.00 | 2.94 | -6.00 | -11.69 | 164.26 | 30.66 | 239.24 | 0.5834 | 913.8 | 999999 | |
| 0.53 | -6.00 | 0.32 | -6.00 | -11.87 | 164.14 | 30.54 | 238.87 | 0.5832 | 853.7 | 999999 | |
| 2.02 | -6.00 | 1.22 | -6.00 | -11.48 | 163.92 | 30.32 | 239.27 | 0.5777 | 967.7 | 999999 | |
| 7.91 | 11.16 | 4.82 | 6.80 | -12.45 | 163.86 | 30.26 | 237.76 | 0.5840 | 908.5 | 638.3 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -11.21 | 163.68 | 30.08 | 239.47 | 0.5729 | 308.0 | 280.7 | |
| 2.02 | -6.00 | 1.22 | -6.00 | -11.78 | 163.71 | 30.11 | 238.63 | 0.5773 | 884.9 | 999999 | |
| 0.00 | 1.85 | 0.00 | 1.11 | -10.70 | 163.51 | 29.91 | 240.12 | 0.5673 | -292.0 | -298.0 | |
| 0.97 | 2.28 | 0.58 | 1.37 | -10.59 | 163.29 | 29.69 | 240.10 | 0.5638 | -725.0 | -566.8 | |
| 0.00 | 2.99 | 0.00 | 1.81 | -12.30 | 163.38 | 29.78 | 237.58 | 0.5771 | 917.0 | 796.9 | |
| 0.00 | 2.28 | 0.00 | 1.36 | -10.24 | 163.11 | 29.51 | 240.51 | 0.5591 | -690.0 | -645.4 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -10.23 | 162.90 | 29.30 | 240.35 | 0.5564 | -632.0 | -528.7 | |
| 0.70 | 3.25 | 0.42 | 1.93 | -10.68 | 162.63 | 29.03 | 239.40 | 0.5562 | -859.0 | -687.7 | |
| 0.00 | 1.32 | 0.00 | 0.78 | -10.95 | 162.38 | 28.78 | 238.76 | 0.5550 | -740.0 | -590.2 | |
| 0.70 | 2.37 | 0.40 | 1.36 | -10.68 | 158.72 | 25.12 | 235.61 | 0.5076 | -683.1 | -556.7 | |
| 0.00 | 1.76 | 0.00 | 1.03 | -14.09 | 159.07 | 25.47 | 230.69 | 0.5413 | -626.0 | -398.9 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -13.56 | 158.84 | 25.24 | 231.21 | 0.5340 | -644.0 | -522.9 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -14.64 | 158.73 | 25.13 | 229.49 | 0.5425 | -649.0 | -621.5 | |
| 0.00 | 2.46 | 0.00 | 1.44 | -14.29 | 158.65 | 25.05 | 229.92 | 0.5384 | -751.0 | -678.6 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -13.28 | 158.30 | 24.70 | 231.03 | 0.5252 | -580.0 | -420.1 | |
| 0.00 | 1.49 | 0.00 | 0.88 | -15.21 | 158.49 | 24.89 | 228.41 | 0.5451 | -263.0 | -245.9 | |
| 0.35 | 1.58 | 0.21 | 0.92 | -13.82 | 158.29 | 24.69 | 230.20 | 0.5300 | -670.0 | -531.6 | |
| 1.05 | 7.73 | 0.61 | 4.50 | -13.62 | 158.10 | 24.50 | 230.28 | 0.5260 | -893.3 | -669.8 | |
| 1.76 | 3.25 | 1.02 | 1.88 | -13.42 | 157.84 | 24.24 | 230.29 | 0.5212 | -835.8 | -684.2 | |
| 0.00 | 1.32 | 0.00 | 0.76 | -12.38 | 157.46 | 23.86 | 231.45 | 0.5073 | -832.0 | -636.5 | |
| 9.84 | 13.88 | 5.68 | 8.01 | -13.21 | 157.48 | 23.88 | 230.19 | 0.5151 | -1017.1 | -719.5 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -20.57 | 157.82 | 24.22 | 220.72 | 0.5911 | 574.0 | 404.4 | |
| 0.00 | 1.58 | 0.00 | 0.91 | -17.70 | 151.58 | 17.98 | 215.96 | 0.5027 | -435.0 | -317.1 | |
| 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. | |