SDO HMI 2011-12-09 11:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.03 | 99.69 | 19.92 | 50.87 | 7.91 | 43.00 | -11.22 | 53.62 | 0.2398 | 197.4 | 7.0 | |
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back to the solar disc SDO HMI 2011-12-09 11:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.58 | 10.99 | 3.84 | 5.56 | 7.68 | 45.27 | -8.95 | 48.55 | 0.2066 | -1078.3 | -820.6 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 8.15 | 44.90 | -9.32 | 48.00 | 0.2168 | -820.0 | -638.0 | |
| 3.58 | 26.84 | 1.81 | 13.60 | 7.20 | 44.71 | -9.51 | 52.04 | 0.2089 | -966.4 | -738.2 | |
| 4.94 | -3.00 | 2.51 | -3.00 | 7.71 | 44.70 | -9.52 | 50.19 | 0.2144 | -1003.5 | 999999 | |
| 0.00 | 3.75 | 0.00 | 1.90 | 8.15 | 44.36 | -9.87 | 49.60 | 0.2238 | -543.0 | -721.4 | |
| 0.00 | 3.92 | 0.00 | 1.99 | 8.15 | 43.96 | -10.26 | 50.69 | 0.2290 | -958.0 | -657.4 | |
| 2.90 | 5.62 | 1.48 | 2.88 | 8.42 | 42.53 | -11.70 | 53.38 | 0.2510 | 1127.5 | 758.7 | |
| 0.00 | 2.47 | 0.00 | 1.27 | 8.57 | 42.25 | -11.98 | 53.54 | 0.2563 | 843.0 | 683.2 | |
| 0.77 | 3.15 | 0.39 | 1.61 | 8.16 | 42.17 | -12.05 | 55.07 | 0.2533 | 831.0 | 795.0 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 7.68 | 41.97 | -12.25 | 57.08 | 0.2517 | 903.0 | 685.0 | |
| 0.00 | 2.47 | 0.00 | 1.27 | 9.38 | 41.76 | -12.46 | 52.14 | 0.2709 | 483.0 | 471.8 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 7.32 | 41.77 | -12.46 | 58.72 | 0.2515 | 825.0 | 674.8 | |
| 8.10 | 36.90 | 4.15 | 18.96 | 7.89 | 41.36 | -12.87 | 57.65 | 0.2624 | 1136.1 | 779.3 | |
| 11.16 | -13.00 | 5.74 | -13.00 | 8.10 | 41.07 | -13.15 | 57.53 | 0.2682 | 983.9 | 999999 | |
| 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. | |