SDO HMI 2011-12-09 08:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75.26 | 508.17 | 66.22 | 441.23 | -22.79 | 107.95 | 52.09 | 242.03 | 0.8255 | 545.3 | 296.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.19 | 9.63 | 1.10 | 8.84 | -17.67 | 111.55 | 55.68 | 248.99 | 0.8451 | 539.4 | 542.3 | |
| 1.36 | -1.00 | 1.25 | -1.00 | -17.61 | 111.24 | 55.38 | 248.99 | 0.8424 | 802.1 | 999999 | |
| 1.45 | -1.00 | 1.33 | -1.00 | -17.83 | 111.29 | 55.43 | 248.75 | 0.8432 | 754.7 | 999999 | |
| 0.00 | 1.28 | 0.00 | 1.06 | -19.42 | 106.73 | 50.87 | 245.65 | 0.8052 | -377.0 | -305.6 | |
| 0.00 | 1.88 | 0.00 | 1.59 | -20.62 | 107.27 | 51.41 | 244.39 | 0.8135 | -90.0 | -156.9 | |
| 67.94 | 463.02 | 59.66 | 403.73 | -22.94 | 108.15 | 52.29 | 241.93 | 0.8278 | 965.1 | 334.4 | |
| 0.00 | 1.36 | 0.00 | 1.23 | -24.17 | 108.86 | 52.99 | 240.75 | 0.8372 | -171.0 | -136.2 | |
| 1.70 | -6.00 | 1.49 | -6.00 | -23.49 | 107.88 | 52.01 | 241.21 | 0.8270 | 542.2 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.77 | -20.12 | 105.94 | 50.08 | 244.57 | 0.7997 | -460.0 | -419.1 | |
| 0.00 | 0.68 | 0.00 | 0.55 | -20.05 | 105.47 | 49.61 | 244.49 | 0.7950 | -527.0 | -470.9 | |
| 0.43 | -6.00 | 0.36 | -6.00 | -23.07 | 106.87 | 51.01 | 241.36 | 0.8170 | 952.0 | 999999 | |
| 1.19 | 2.13 | 1.03 | 1.84 | -24.27 | 106.90 | 51.04 | 239.98 | 0.8209 | 410.4 | 470.8 | |
| 0.00 | 1.11 | 0.00 | 0.90 | -20.72 | 105.08 | 49.22 | 243.56 | 0.7933 | -521.0 | -444.1 | |
| 0.00 | 0.85 | 0.00 | 0.68 | -20.49 | 104.65 | 48.78 | 243.68 | 0.7884 | -637.0 | -578.9 | |
| 0.00 | 1.79 | 0.00 | 1.55 | -24.85 | 106.77 | 50.91 | 239.26 | 0.8216 | 155.0 | 142.4 | |
| 0.00 | 2.81 | 0.00 | 2.41 | -24.69 | 106.52 | 50.66 | 239.36 | 0.8190 | 596.0 | 428.7 | |
| 0.00 | 1.70 | 0.00 | 1.41 | -22.98 | 105.46 | 49.59 | 240.98 | 0.8040 | 552.0 | 413.5 | |
| 0.00 | 1.36 | 0.00 | 1.08 | -20.68 | 104.11 | 48.24 | 243.26 | 0.7838 | -544.0 | -413.9 | |
| 0.00 | 0.85 | 0.00 | 0.69 | -22.40 | 104.44 | 48.58 | 241.30 | 0.7927 | -176.0 | -136.8 | |
| 0.00 | 1.11 | 0.00 | 0.88 | -21.13 | 103.77 | 47.91 | 242.59 | 0.7820 | -566.0 | -482.3 | |
| 0.00 | 1.36 | 0.00 | 1.11 | -22.82 | 104.49 | 48.63 | 240.82 | 0.7946 | -335.0 | -233.9 | |
| 0.00 | 0.77 | 0.00 | 0.62 | -22.40 | 104.25 | 48.38 | 241.23 | 0.7909 | -431.0 | -385.6 | |
| 0.00 | 0.77 | 0.00 | 0.59 | -19.96 | 102.87 | 47.01 | 243.70 | 0.7692 | -632.0 | -564.1 | |
| 0.00 | 1.70 | 0.00 | 1.32 | -20.62 | 102.86 | 46.99 | 242.87 | 0.7713 | -594.0 | -544.8 | |
| 0.00 | 1.28 | 0.00 | 0.97 | -19.93 | 101.90 | 46.03 | 243.37 | 0.7593 | -597.0 | -500.8 | |
| 0.00 | 0.60 | 0.00 | 0.45 | -20.28 | 102.03 | 46.17 | 242.99 | 0.7618 | -483.0 | -478.6 | |
| 0.00 | 1.11 | 0.00 | 0.87 | -22.05 | 102.76 | 46.89 | 241.08 | 0.7754 | -139.0 | -264.5 | |
| 0.00 | 0.85 | 0.00 | 0.64 | -19.99 | 101.69 | 45.83 | 243.21 | 0.7574 | -781.0 | -644.2 | |
| 0.00 | 0.85 | 0.00 | 0.67 | -22.75 | 102.55 | 46.69 | 240.14 | 0.7760 | -584.0 | -450.7 | |
| 0.00 | 1.96 | 0.00 | 1.53 | -22.91 | 102.48 | 46.62 | 239.92 | 0.7760 | -434.0 | -289.6 | |
| 0.00 | 0.34 | 0.00 | 0.26 | -20.46 | 101.38 | 45.51 | 242.49 | 0.7559 | -680.0 | -652.2 | |
| 0.00 | 1.19 | 0.00 | 0.88 | -20.50 | 100.05 | 44.18 | 241.91 | 0.7424 | -473.0 | -343.6 | |
| 0.00 | 1.36 | 0.00 | 1.00 | -20.24 | 99.91 | 44.05 | 242.17 | 0.7400 | -699.0 | -579.6 | |
| 0.00 | 0.51 | 0.00 | 0.37 | -20.81 | 99.11 | 43.25 | 241.09 | 0.7340 | -739.0 | -615.3 | |
| 0.00 | 1.02 | 0.00 | 0.74 | -21.96 | 98.62 | 42.75 | 239.41 | 0.7338 | -410.0 | -308.4 | |
| 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. | |