SDO HMI 2011-11-28 17:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.09 | 141.80 | 17.60 | 82.63 | 17.98 | 223.45 | 27.57 | 303.44 | 0.5298 | -468.6 | -365.8 | |
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back to the solar disc SDO HMI 2011-11-28 17:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.77 | 0.00 | 0.46 | 19.79 | 225.63 | 29.74 | 304.50 | 0.5687 | 786.0 | 609.8 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 18.06 | 224.65 | 28.76 | 302.54 | 0.5449 | 70.0 | 24.4 | |
| 9.83 | 27.44 | 5.78 | 16.11 | 17.84 | 224.43 | 28.55 | 302.37 | 0.5407 | -911.9 | -584.2 | |
| 0.00 | 3.42 | 0.00 | 2.00 | 17.39 | 223.96 | 28.08 | 301.99 | 0.5318 | -920.0 | -675.3 | |
| 20.26 | 92.22 | 11.82 | 53.80 | 18.10 | 223.52 | 27.64 | 303.55 | 0.5313 | -1109.1 | -441.9 | |
| 0.00 | 0.26 | 0.00 | 0.15 | 15.80 | 223.05 | 27.17 | 300.00 | 0.5095 | 320.0 | 377.3 | |
| 0.00 | 5.98 | 0.00 | 3.44 | 16.26 | 222.95 | 27.07 | 300.90 | 0.5112 | -99.0 | -183.6 | |
| 0.00 | 1.20 | 0.00 | 0.69 | 16.08 | 222.82 | 26.94 | 300.69 | 0.5082 | 529.0 | 463.9 | |
| 0.00 | 1.28 | 0.00 | 0.73 | 15.19 | 222.62 | 26.74 | 299.27 | 0.4998 | 941.0 | 832.2 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 20.41 | 222.81 | 26.93 | 307.92 | 0.5402 | -733.0 | -566.8 | |
| 0.00 | 0.85 | 0.00 | 0.49 | 18.93 | 221.32 | 25.44 | 306.97 | 0.5107 | -524.0 | -441.1 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 18.44 | 220.11 | 24.23 | 307.39 | 0.4920 | 641.0 | 532.3 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 13.13 | 218.95 | 23.06 | 298.57 | 0.4363 | 832.0 | 676.2 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 18.66 | 219.46 | 23.58 | 308.47 | 0.4861 | 664.0 | 522.6 | |
| 0.00 | 1.37 | 0.00 | 0.78 | 20.98 | 218.42 | 22.54 | 313.48 | 0.4952 | 772.0 | 615.8 | |
| 0.00 | 2.05 | 0.00 | 1.16 | 21.31 | 217.20 | 21.32 | 315.49 | 0.4852 | 293.0 | 430.2 | |
| 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. | |