SDO HMI 2011-12-07 20:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.19 | 187.75 | 20.74 | 110.41 | 18.49 | 102.97 | 27.35 | 305.97 | 0.5404 | -332.4 | -237.6 | |
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back to the solar disc SDO HMI 2011-12-07 20:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.77 | 7.07 | 2.81 | 4.16 | 17.01 | 104.02 | 28.40 | 302.65 | 0.5423 | 763.8 | 645.9 | |
| 2.47 | 3.58 | 1.45 | 2.10 | 17.07 | 103.46 | 27.85 | 303.22 | 0.5359 | 716.8 | 593.5 | |
| 23.61 | 139.34 | 13.96 | 82.47 | 18.78 | 103.48 | 27.86 | 305.95 | 0.5487 | -1203.7 | -342.6 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 17.88 | 102.20 | 26.58 | 305.68 | 0.5265 | -695.0 | -544.4 | |
| 0.00 | 1.45 | 0.00 | 0.84 | 17.72 | 102.07 | 26.46 | 305.55 | 0.5237 | -691.0 | -530.0 | |
| 1.70 | 2.39 | 0.99 | 1.38 | 17.60 | 101.85 | 26.23 | 305.56 | 0.5200 | 679.5 | 398.8 | |
| 0.00 | 1.53 | 0.00 | 0.88 | 17.57 | 101.39 | 25.77 | 305.95 | 0.5142 | 778.0 | 586.0 | |
| 2.64 | 19.01 | 1.53 | 10.98 | 18.31 | 101.34 | 25.72 | 307.23 | 0.5195 | -1061.9 | -356.6 | |
| 0.00 | 2.13 | 0.00 | 1.23 | 18.47 | 100.88 | 25.26 | 307.94 | 0.5154 | 613.0 | 492.6 | |
| 0.00 | 2.05 | 0.00 | 1.14 | 14.62 | 99.44 | 23.82 | 302.73 | 0.4665 | 849.0 | 615.7 | |
| 0.00 | 3.24 | 0.00 | 1.83 | 16.36 | 99.45 | 23.83 | 305.89 | 0.4806 | 882.0 | 678.3 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 15.50 | 99.34 | 23.73 | 304.46 | 0.4722 | 631.0 | 591.2 | |
| 0.00 | 1.36 | 0.00 | 0.77 | 16.46 | 99.19 | 23.58 | 306.33 | 0.4781 | 527.0 | 587.3 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 20.03 | 99.48 | 23.86 | 311.93 | 0.5129 | 756.0 | 622.2 | |
| 0.00 | 1.70 | 0.00 | 0.97 | 19.31 | 98.00 | 22.38 | 312.52 | 0.4896 | 701.0 | 510.4 | |
| 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. | |