SDO HMI 2011-12-07 13:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.35 | 22.68 | 3.06 | 18.25 | 18.24 | 128.70 | 49.22 | 293.91 | 0.7821 | 170.7 | -2.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.73 | 0.00 | 2.76 | 16.96 | 138.82 | 59.33 | 289.47 | 0.8747 | -230.0 | -160.5 | |
| 0.00 | 1.02 | 0.00 | 1.04 | 17.18 | 138.87 | 59.39 | 289.71 | 0.8754 | -184.0 | -163.6 | |
| 0.00 | 1.96 | 0.00 | 1.93 | 17.40 | 137.60 | 58.12 | 290.20 | 0.8654 | -259.0 | -229.7 | |
| 0.00 | 1.11 | 0.00 | 1.06 | 16.56 | 136.78 | 57.30 | 289.41 | 0.8573 | 585.0 | 448.3 | |
| 0.00 | 1.28 | 0.00 | 0.97 | 18.12 | 126.35 | 46.87 | 294.07 | 0.7620 | -573.0 | -418.4 | |
| 0.00 | 1.70 | 0.00 | 1.30 | 18.36 | 126.35 | 46.87 | 294.38 | 0.7628 | -695.0 | -563.2 | |
| 0.00 | 1.11 | 0.00 | 0.86 | 20.43 | 126.77 | 47.29 | 296.81 | 0.7738 | -417.0 | -413.2 | |
| 0.00 | 1.02 | 0.00 | 0.77 | 19.68 | 125.06 | 45.57 | 296.52 | 0.7539 | -701.0 | -572.1 | |
| 4.35 | 6.99 | 3.06 | 4.92 | 18.27 | 121.67 | 42.19 | 296.09 | 0.7125 | 862.8 | 675.5 | |
| 0.00 | 0.94 | 0.00 | 0.66 | 18.74 | 121.61 | 42.12 | 296.74 | 0.7136 | 598.0 | 449.5 | |
| 0.00 | 0.43 | 0.00 | 0.30 | 20.50 | 121.33 | 41.84 | 299.18 | 0.7181 | 407.0 | 384.8 | |
| 0.00 | 1.11 | 0.00 | 0.78 | 20.12 | 121.16 | 41.68 | 298.76 | 0.7146 | 512.0 | 501.3 | |
| 0.00 | 0.43 | 0.00 | 0.30 | 20.81 | 121.01 | 41.53 | 299.74 | 0.7161 | 509.0 | 414.8 | |
| 0.00 | 0.85 | 0.00 | 0.60 | 20.91 | 120.83 | 41.35 | 299.95 | 0.7146 | 550.0 | 498.2 | |
| 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. | |