SDO HMI 2011-07-05 07:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.82 | 104.77 | 22.85 | 97.24 | 15.48 | 26.64 | 57.35 | 286.26 | 0.8470 | -250.0 | -168.8 | |
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back to the solar disc SDO HMI 2011-07-05 07:59:11 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.45 | 77.96 | 14.68 | 74.02 | 15.33 | 27.57 | 58.28 | 285.96 | 0.8553 | -743.3 | -311.9 | |
| 0.82 | -1.00 | 0.77 | -1.00 | 14.97 | 27.17 | 57.88 | 285.59 | 0.8515 | -817.2 | 999999 | |
| 0.36 | -1.00 | 0.34 | -1.00 | 15.11 | 26.88 | 57.58 | 285.78 | 0.8490 | -781.5 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.91 | 15.37 | 25.99 | 56.70 | 286.20 | 0.8413 | -275.0 | -279.5 | |
| 0.00 | 1.18 | 0.00 | 1.06 | 15.23 | 25.59 | 56.29 | 286.08 | 0.8375 | 421.0 | 264.7 | |
| 0.00 | 1.09 | 0.00 | 0.99 | 16.86 | 25.72 | 56.43 | 288.00 | 0.8405 | -470.0 | -334.7 | |
| 1.73 | 10.72 | 1.49 | 9.26 | 15.78 | 23.85 | 54.55 | 286.98 | 0.8218 | 335.1 | 377.7 | |
| 2.73 | -7.00 | 2.35 | -7.00 | 15.98 | 23.65 | 54.36 | 287.25 | 0.8202 | 653.0 | 999999 | |
| 1.00 | 4.82 | 0.86 | 4.15 | 16.33 | 23.63 | 54.34 | 287.67 | 0.8205 | 504.7 | 504.9 | |
| 2.73 | 3.00 | 2.36 | 2.59 | 16.64 | 23.70 | 54.41 | 288.04 | 0.8216 | 556.6 | 292.2 | |
| 0.00 | 3.09 | 0.00 | 2.63 | 15.65 | 23.25 | 53.96 | 286.91 | 0.8159 | 482.0 | 470.0 | |
| 0.00 | 0.55 | 0.00 | 0.47 | 16.44 | 23.18 | 53.89 | 287.88 | 0.8164 | 513.0 | 463.8 | |
| 0.00 | 1.36 | 0.00 | 1.16 | 16.20 | 22.92 | 53.63 | 287.63 | 0.8135 | 672.0 | 585.1 | |
| 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. | |