SDO HMI 2011-11-13 20:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.28 | 371.39 | 31.30 | 221.94 | 16.15 | 63.83 | 31.88 | 294.88 | 0.5615 | -840.9 | -340.2 | |
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back to the solar disc SDO HMI 2011-11-13 20:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.86 | 356.85 | 0.51 | 213.65 | 15.52 | 64.16 | 32.22 | 293.55 | 0.5625 | -939.4 | -372.0 | |
| 0.00 | 1.29 | 0.00 | 0.79 | 18.97 | 64.77 | 32.83 | 298.85 | 0.5876 | -707.0 | -572.5 | |
| 50.39 | -1.00 | 30.18 | -1.00 | 16.04 | 64.11 | 32.16 | 294.46 | 0.5642 | -1254.5 | 999999 | |
| 1.03 | -1.00 | 0.61 | -1.00 | 15.72 | 63.68 | 31.74 | 294.14 | 0.5571 | -1342.4 | 999999 | |
| 0.00 | 1.72 | 0.00 | 1.01 | 14.14 | 62.42 | 30.48 | 292.08 | 0.5329 | -774.0 | -603.0 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 18.00 | 58.07 | 26.13 | 302.14 | 0.4967 | 660.0 | 600.7 | |
| 0.00 | 1.98 | 0.00 | 1.14 | 19.51 | 58.19 | 26.24 | 304.69 | 0.5090 | 600.0 | 455.3 | |
| 0.00 | 1.63 | 0.00 | 0.92 | 18.18 | 56.86 | 24.91 | 303.58 | 0.4824 | 818.0 | 690.6 | |
| 0.00 | 1.81 | 0.00 | 1.03 | 21.23 | 56.11 | 24.17 | 309.67 | 0.4978 | 647.0 | 577.8 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 20.36 | 54.75 | 22.81 | 309.67 | 0.4742 | 714.0 | 629.7 | |
| 0.00 | 0.95 | 0.00 | 0.54 | 22.33 | 54.87 | 22.93 | 312.83 | 0.4934 | 766.0 | 649.3 | |
| 0.00 | 1.55 | 0.00 | 0.87 | 21.70 | 54.52 | 22.58 | 312.22 | 0.4837 | 892.0 | 707.6 | |
| 0.00 | 2.41 | 0.00 | 1.31 | 20.25 | 50.24 | 18.30 | 315.36 | 0.4210 | 812.0 | 674.5 | |
| 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. | |