SDO HMI 2014-11-04 23:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.52 | 181.71 | 29.89 | 91.28 | -4.91 | 86.77 | 3.16 | 199.70 | 0.1701 | 206.6 | 45.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.54 | 29.98 | 1.78 | 15.09 | -4.34 | 89.87 | 6.26 | 216.89 | 0.1819 | 889.8 | 737.6 | |
| 12.27 | -1.00 | 6.17 | -1.00 | -4.22 | 89.66 | 6.05 | 216.36 | 0.1781 | 1126.4 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -4.76 | 89.64 | 6.02 | 214.51 | 0.1854 | 865.0 | 699.5 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -4.97 | 89.58 | 5.96 | 213.61 | 0.1878 | 717.0 | 592.0 | |
| 8.90 | 33.35 | 4.47 | 16.74 | -4.00 | 88.58 | 4.97 | 211.85 | 0.1645 | 1168.0 | 758.8 | |
| 0.00 | 3.02 | 0.00 | 1.52 | -4.57 | 88.35 | 4.73 | 208.91 | 0.1709 | 853.0 | 698.8 | |
| 0.00 | 1.73 | 0.00 | 0.87 | -4.87 | 88.32 | 4.70 | 207.93 | 0.1752 | 706.0 | 589.2 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -6.23 | 88.24 | 4.62 | 204.30 | 0.1956 | 896.0 | 738.3 | |
| 9.16 | -5.00 | 4.60 | -5.00 | -4.03 | 88.20 | 4.58 | 209.71 | 0.1615 | 1215.9 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -5.26 | 88.14 | 4.53 | 206.04 | 0.1799 | 768.0 | 574.0 | |
| 0.00 | 2.51 | 0.00 | 1.26 | -4.75 | 87.93 | 4.31 | 206.25 | 0.1703 | 1009.0 | 867.5 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -6.16 | 87.70 | 4.08 | 201.87 | 0.1910 | 868.0 | 681.9 | |
| 0.00 | 1.38 | 0.00 | 0.69 | -4.36 | 87.69 | 4.07 | 205.99 | 0.1624 | 377.0 | 274.9 | |
| 0.00 | 2.51 | 0.00 | 1.26 | -4.54 | 87.69 | 4.07 | 205.52 | 0.1652 | 998.0 | 861.1 | |
| 0.60 | 7.43 | 0.30 | 3.73 | -3.79 | 87.57 | 3.95 | 206.92 | 0.1526 | 955.3 | 857.5 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -6.10 | 87.49 | 3.87 | 200.96 | 0.1887 | 670.0 | 544.8 | |
| 2.16 | 3.37 | 1.08 | 1.69 | -4.66 | 87.39 | 3.78 | 203.57 | 0.1649 | 751.8 | 499.3 | |
| 0.00 | 1.81 | 0.00 | 0.91 | -3.84 | 87.18 | 3.56 | 204.45 | 0.1506 | 76.0 | 83.0 | |
| 0.00 | 0.78 | 0.00 | 0.39 | -5.55 | 86.53 | 2.91 | 196.95 | 0.1743 | -767.0 | -554.9 | |
| 0.35 | 4.49 | 0.17 | 2.25 | -3.93 | 86.46 | 2.85 | 199.76 | 0.1473 | 1040.2 | 747.1 | |
| 0.00 | 1.64 | 0.00 | 0.82 | -4.02 | 85.90 | 2.28 | 195.89 | 0.1458 | 1009.0 | 797.8 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -3.51 | 85.75 | 2.13 | 195.86 | 0.1365 | 923.0 | 695.4 | |
| 0.00 | 1.90 | 0.00 | 0.95 | -5.31 | 85.75 | 2.14 | 192.92 | 0.1668 | -470.0 | -206.9 | |
| 0.00 | 1.90 | 0.00 | 0.95 | -5.22 | 85.51 | 1.90 | 191.62 | 0.1644 | -736.0 | -445.2 | |
| 1.12 | 65.92 | 0.56 | 33.11 | -5.76 | 85.36 | 1.75 | 190.15 | 0.1731 | -908.3 | -748.4 | |
| 7.17 | -25.00 | 3.60 | -25.00 | -5.61 | 85.18 | 1.57 | 189.27 | 0.1700 | -1283.7 | 999999 | |
| 4.49 | -25.00 | 2.26 | -25.00 | -5.76 | 85.18 | 1.57 | 189.13 | 0.1726 | -918.5 | 999999 | |
| 5.87 | -25.00 | 2.95 | -25.00 | -5.43 | 85.00 | 1.39 | 188.38 | 0.1664 | -1306.2 | 999999 | |
| 1.04 | -25.00 | 0.52 | -25.00 | -5.04 | 84.86 | 1.24 | 187.81 | 0.1594 | -1022.2 | 999999 | |
| 0.86 | -25.00 | 0.43 | -25.00 | -5.31 | 84.83 | 1.21 | 187.41 | 0.1639 | -1216.6 | 999999 | |
| 1.99 | -25.00 | 1.00 | -25.00 | -5.22 | 84.59 | 0.97 | 186.02 | 0.1619 | -1214.7 | 999999 | |
| 0.00 | 3.37 | 0.00 | 1.70 | -7.54 | 81.83 | -1.78 | 171.23 | 0.2034 | -1017.0 | -788.6 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -7.15 | 81.08 | -2.53 | 167.23 | 0.1992 | -786.0 | -500.0 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -7.03 | 80.99 | -2.62 | 166.66 | 0.1975 | -970.0 | -779.2 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -7.24 | 80.48 | -3.13 | 164.46 | 0.2032 | -724.0 | -619.2 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -8.76 | 79.90 | -3.72 | 163.82 | 0.2310 | -861.0 | -661.3 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -7.15 | 79.55 | -4.06 | 160.03 | 0.2067 | -929.0 | -767.7 | |
| 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. | |