SDO HMI 2011-11-14 17:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.80 | 232.56 | 16.97 | 137.04 | 28.33 | 42.18 | 21.76 | 322.95 | 0.5436 | -767.0 | -404.0 | |
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back to the solar disc SDO HMI 2011-11-14 17:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.52 | 0.00 | 0.33 | 35.16 | 45.58 | 25.16 | 327.09 | 0.6421 | -505.0 | -412.0 | |
| 8.68 | 218.89 | 5.13 | 129.07 | 28.41 | 42.48 | 22.06 | 322.68 | 0.5471 | -1131.1 | -430.7 | |
| 14.27 | -2.00 | 8.40 | -2.00 | 28.09 | 42.41 | 21.99 | 322.35 | 0.5430 | -1324.9 | 999999 | |
| 1.55 | -2.00 | 0.91 | -2.00 | 28.42 | 42.01 | 21.59 | 323.25 | 0.5431 | -897.4 | 999999 | |
| 2.75 | -2.00 | 1.62 | -2.00 | 28.62 | 42.05 | 21.63 | 323.45 | 0.5456 | -819.2 | 999999 | |
| 1.55 | -2.00 | 0.91 | -2.00 | 28.66 | 41.84 | 21.42 | 323.74 | 0.5441 | -798.8 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 29.71 | 42.00 | 21.59 | 324.84 | 0.5570 | -484.0 | -397.8 | |
| 0.00 | 1.55 | 0.00 | 0.92 | 29.52 | 41.89 | 21.47 | 324.74 | 0.5539 | -684.0 | -528.6 | |
| 0.00 | 1.03 | 0.00 | 0.62 | 30.31 | 42.03 | 21.61 | 325.52 | 0.5638 | 673.0 | 545.5 | |
| 0.00 | 0.86 | 0.00 | 0.54 | 35.36 | 42.39 | 21.97 | 330.49 | 0.6218 | -569.0 | -494.7 | |
| 0.00 | 1.89 | 0.00 | 1.11 | 29.78 | 40.23 | 19.81 | 327.07 | 0.5432 | -716.0 | -670.1 | |
| 0.00 | 1.46 | 0.00 | 0.86 | 30.16 | 39.40 | 18.98 | 328.55 | 0.5411 | -663.0 | -578.4 | |
| 0.00 | 3.01 | 0.00 | 1.69 | 26.61 | 36.42 | 16.00 | 328.57 | 0.4746 | 545.0 | 644.5 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 23.83 | 35.64 | 15.23 | 326.15 | 0.4332 | 767.0 | 573.2 | |
| 0.00 | 1.46 | 0.00 | 0.82 | 26.94 | 36.02 | 15.60 | 329.59 | 0.4756 | 752.0 | 538.9 | |
| 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. | |