SDO HMI 2011-11-30 05:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.74 | 160.54 | 39.24 | 214.02 | -20.29 | 109.93 | -66.17 | 112.38 | 0.9290 | 176.4 | 146.1 | |
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back to the solar disc SDO HMI 2011-11-30 05:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.85 | 0.00 | 1.03 | -22.76 | 113.04 | -63.07 | 115.62 | 0.9135 | -187.0 | -196.3 | |
| 5.13 | 52.06 | 6.76 | 68.86 | -23.38 | 110.77 | -65.34 | 115.82 | 0.9283 | 645.4 | 259.1 | |
| 0.77 | -2.00 | 1.00 | -2.00 | -23.09 | 110.97 | -65.14 | 115.55 | 0.9268 | 916.9 | 999999 | |
| 1.03 | -2.00 | 1.37 | -2.00 | -23.22 | 110.44 | -65.66 | 115.59 | 0.9300 | 316.2 | 999999 | |
| 0.77 | 1.71 | 1.05 | 2.33 | -22.46 | 109.82 | -66.28 | 114.67 | 0.9327 | 215.7 | 159.7 | |
| 0.00 | 1.20 | 0.00 | 1.64 | -22.63 | 109.66 | -66.44 | 114.82 | 0.9338 | 151.0 | 143.7 | |
| 0.00 | 1.11 | 0.00 | 1.58 | -23.03 | 108.85 | -67.25 | 115.09 | 0.9387 | 28.0 | -3.0 | |
| 0.00 | 0.34 | 0.00 | 0.54 | -22.84 | 106.48 | -69.62 | 114.51 | 0.9509 | -574.0 | -535.0 | |
| 11.97 | 73.18 | 14.73 | 90.00 | -16.88 | 111.34 | -64.76 | 108.97 | 0.9170 | 659.5 | 247.7 | |
| 6.16 | 16.76 | 9.69 | 26.62 | -22.01 | 106.39 | -69.71 | 113.63 | 0.9506 | -480.9 | -187.7 | |
| 0.00 | 5.21 | 0.00 | 8.53 | -22.54 | 105.70 | -70.41 | 114.07 | 0.9544 | -253.0 | -231.4 | |
| 2.91 | 8.12 | 4.64 | 12.89 | -21.50 | 106.01 | -70.09 | 113.05 | 0.9520 | -507.6 | -409.5 | |
| 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. | |