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 |
| 14.87 | 66.19 | 8.86 | 39.66 | 8.21 | 346.45 | -33.96 | 79.69 | 0.5640 | -23.1 | 128.3 | |
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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 | 1.63 | 0.00 | 0.93 | 7.43 | 351.53 | -28.89 | 79.99 | 0.4884 | -869.0 | -680.8 | |
| 0.00 | 1.29 | 0.00 | 0.75 | 8.23 | 349.18 | -31.24 | 79.02 | 0.5249 | 288.0 | 261.7 | |
| 0.00 | 0.95 | 0.00 | 0.55 | 8.53 | 349.16 | -31.26 | 78.46 | 0.5259 | 648.0 | 551.2 | |
| 3.27 | 10.23 | 1.90 | 5.96 | 7.90 | 349.04 | -31.38 | 79.69 | 0.5264 | -933.1 | -682.4 | |
| 1.80 | -4.00 | 1.05 | -4.00 | 8.07 | 348.88 | -31.54 | 79.39 | 0.5290 | -849.3 | 999999 | |
| 1.03 | 1.63 | 0.60 | 0.95 | 7.80 | 348.73 | -31.69 | 79.94 | 0.5307 | -752.1 | -684.7 | |
| 0.00 | 1.72 | 0.00 | 1.00 | 7.98 | 348.57 | -31.85 | 79.65 | 0.5333 | -695.0 | -495.2 | |
| 0.00 | 0.95 | 0.00 | 0.56 | 7.36 | 347.95 | -32.47 | 80.92 | 0.5413 | -597.0 | -484.8 | |
| 0.00 | 1.89 | 0.00 | 1.12 | 7.29 | 347.60 | -32.82 | 81.11 | 0.5463 | -748.0 | -607.7 | |
| 0.52 | 5.84 | 0.31 | 3.52 | 8.17 | 345.94 | -34.48 | 79.87 | 0.5715 | 905.2 | 810.8 | |
| 1.80 | 33.09 | 1.09 | 20.06 | 8.19 | 345.68 | -34.74 | 79.89 | 0.5751 | 897.3 | 377.0 | |
| 6.02 | -11.00 | 3.65 | -11.00 | 8.34 | 345.44 | -34.97 | 79.69 | 0.5787 | 887.7 | 999999 | |
| 0.43 | 2.15 | 0.26 | 1.31 | 8.77 | 344.92 | -35.50 | 79.06 | 0.5868 | -555.2 | -349.6 | |
| 0.00 | 1.12 | 0.00 | 0.68 | 8.40 | 344.70 | -35.72 | 79.72 | 0.5892 | -502.0 | -469.5 | |
| 0.00 | 1.46 | 0.00 | 0.89 | 8.67 | 344.64 | -35.78 | 79.28 | 0.5905 | -802.0 | -672.1 | |
| 0.00 | 1.12 | 0.00 | 0.69 | 9.24 | 343.60 | -36.82 | 78.55 | 0.6058 | 543.0 | 518.4 | |
| 0.00 | 1.12 | 0.00 | 0.69 | 8.88 | 343.60 | -36.81 | 79.14 | 0.6051 | 664.0 | 536.5 | |
| 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. | |