SDO HMI 2011-07-24 11:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.34 | 34.19 | 4.90 | 17.95 | 23.96 | 79.00 | 3.33 | 350.36 | 0.3311 | -505.6 | -327.0 | |
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back to the solar disc SDO HMI 2011-07-24 11:59:11 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.26 | 7.80 | 3.28 | 4.09 | 23.51 | 81.14 | 5.47 | 344.51 | 0.3287 | -889.1 | -699.1 | |
| 0.00 | 6.35 | 0.00 | 3.33 | 23.58 | 80.67 | 5.01 | 345.82 | 0.3278 | -1133.0 | -895.9 | |
| 3.08 | 3.72 | 1.62 | 1.95 | 23.61 | 80.24 | 4.57 | 347.02 | 0.3267 | -961.2 | -719.1 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 22.59 | 80.04 | 4.37 | 346.79 | 0.3095 | -873.0 | -659.1 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 22.56 | 79.81 | 4.14 | 347.45 | 0.3081 | -870.0 | -710.9 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 22.47 | 79.71 | 4.04 | 347.67 | 0.3062 | -686.0 | -650.1 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 22.75 | 79.42 | 3.75 | 348.73 | 0.3099 | -970.0 | -693.8 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 23.04 | 79.23 | 3.56 | 349.48 | 0.3140 | -942.0 | -795.6 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 23.53 | 79.01 | 3.34 | 350.39 | 0.3213 | -976.0 | -663.8 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 23.88 | 78.25 | 2.58 | 352.70 | 0.3253 | -815.0 | -584.2 | |
| 0.00 | 1.72 | 0.00 | 0.90 | 24.24 | 76.65 | 0.98 | 357.26 | 0.3289 | 851.0 | 669.5 | |
| 0.00 | 3.99 | 0.00 | 2.13 | 27.20 | 74.28 | -1.39 | 3.28 | 0.3777 | 697.0 | 621.1 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 24.53 | 73.34 | -2.33 | 6.35 | 0.3354 | 869.0 | 647.4 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 24.59 | 72.97 | -2.70 | 7.33 | 0.3371 | 777.0 | 686.2 | |
| 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. | |