SDO HMI 2014-09-03 18:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.90 | 73.87 | 12.74 | 45.13 | -17.86 | 158.70 | -25.78 | 134.92 | 0.5864 | 230.5 | 100.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.89 | 0.00 | 0.53 | -19.47 | 162.96 | -21.52 | 141.89 | 0.5626 | 587.0 | 399.7 | |
| 0.00 | 0.98 | 0.00 | 0.59 | -17.45 | 161.24 | -23.24 | 137.28 | 0.5570 | 742.0 | 601.1 | |
| 0.00 | 1.52 | 0.00 | 0.90 | -17.32 | 161.08 | -23.40 | 136.93 | 0.5573 | 506.0 | 583.1 | |
| 0.00 | 1.97 | 0.00 | 1.17 | -16.83 | 161.05 | -23.44 | 136.25 | 0.5526 | 771.0 | 655.5 | |
| 0.89 | 14.83 | 0.53 | 8.90 | -17.51 | 160.68 | -23.81 | 136.68 | 0.5632 | 904.8 | 724.5 | |
| 8.22 | -5.00 | 4.94 | -5.00 | -17.81 | 160.60 | -23.88 | 136.97 | 0.5671 | 895.4 | 999999 | |
| 0.00 | 2.14 | 0.00 | 1.29 | -17.84 | 160.07 | -24.41 | 136.39 | 0.5725 | 945.0 | 730.5 | |
| 0.00 | 1.07 | 0.00 | 0.65 | -18.52 | 159.97 | -24.51 | 137.11 | 0.5802 | 483.0 | 498.4 | |
| 0.00 | 5.63 | 0.00 | 3.38 | -17.31 | 160.01 | -24.47 | 135.64 | 0.5679 | 678.0 | 580.6 | |
| 0.00 | 0.98 | 0.00 | 0.60 | -18.13 | 159.78 | -24.70 | 136.41 | 0.5781 | 439.0 | 478.3 | |
| 0.00 | 1.07 | 0.00 | 0.65 | -17.96 | 159.77 | -24.71 | 136.19 | 0.5766 | 715.0 | 527.4 | |
| 0.00 | 0.27 | 0.00 | 0.16 | -17.83 | 159.72 | -24.76 | 135.97 | 0.5758 | 279.0 | 315.3 | |
| 0.00 | 0.36 | 0.00 | 0.22 | -17.87 | 159.58 | -24.90 | 135.85 | 0.5776 | 360.0 | 415.2 | |
| 0.00 | 1.52 | 0.00 | 0.93 | -18.60 | 159.04 | -25.44 | 136.16 | 0.5901 | 277.0 | 261.4 | |
| 1.79 | 4.91 | 1.08 | 2.98 | -17.66 | 159.12 | -25.36 | 135.07 | 0.5802 | 810.6 | 571.3 | |
| 0.00 | 1.34 | 0.00 | 0.82 | -18.22 | 158.71 | -25.77 | 135.33 | 0.5896 | 612.0 | 486.0 | |
| 0.00 | 1.70 | 0.00 | 1.03 | -16.55 | 158.41 | -26.08 | 132.84 | 0.5768 | 390.0 | 305.1 | |
| 0.00 | 1.07 | 0.00 | 0.65 | -16.75 | 158.31 | -26.18 | 133.00 | 0.5798 | 685.0 | 650.4 | |
| 0.00 | 1.25 | 0.00 | 0.77 | -17.64 | 157.81 | -26.67 | 133.62 | 0.5931 | -258.0 | -313.1 | |
| 0.00 | 0.89 | 0.00 | 0.56 | -18.72 | 157.56 | -26.92 | 134.71 | 0.6057 | -254.0 | -314.5 | |
| 2.23 | 3.57 | 1.38 | 2.22 | -18.45 | 157.53 | -26.95 | 134.36 | 0.6034 | -856.2 | -744.7 | |
| 0.00 | 4.02 | 0.00 | 2.51 | -18.91 | 157.20 | -27.28 | 134.57 | 0.6109 | -826.0 | -666.6 | |
| 3.57 | 5.63 | 2.18 | 3.43 | -16.22 | 157.29 | -27.19 | 131.22 | 0.5855 | -853.9 | -700.7 | |
| 3.13 | 11.53 | 1.96 | 7.24 | -18.81 | 156.57 | -27.91 | 133.81 | 0.6163 | -866.8 | -616.9 | |
| 1.07 | 2.86 | 0.67 | 1.78 | -17.91 | 156.55 | -27.93 | 132.67 | 0.6084 | -715.8 | -632.2 | |
| 0.00 | 0.80 | 0.00 | 0.51 | -18.70 | 156.19 | -28.29 | 133.30 | 0.6190 | -661.0 | -571.9 | |
| 0.00 | 1.07 | 0.00 | 0.66 | -15.97 | 155.44 | -29.05 | 129.04 | 0.6032 | 521.0 | 401.2 | |
| 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. | |