SDO HMI 2011-07-24 15:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.59 | 33.18 | 7.68 | 17.48 | 24.05 | 79.49 | 6.03 | 343.31 | 0.3411 | -698.9 | -454.3 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.80 | 8.25 | 3.05 | 4.34 | 23.46 | 81.17 | 7.71 | 338.65 | 0.3394 | -910.3 | -632.6 | |
| 5.53 | 6.16 | 2.91 | 3.24 | 23.59 | 80.70 | 7.25 | 339.96 | 0.3388 | -882.7 | -619.0 | |
| 3.26 | 3.54 | 1.72 | 1.86 | 23.59 | 80.24 | 6.78 | 341.15 | 0.3363 | -957.6 | -703.0 | |
| 0.00 | 2.27 | 0.00 | 1.18 | 22.03 | 79.76 | 6.30 | 340.71 | 0.3095 | -714.0 | -538.0 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 22.70 | 79.43 | 5.97 | 342.38 | 0.3183 | -902.0 | -627.7 | |
| 0.00 | 1.81 | 0.00 | 0.95 | 23.06 | 79.24 | 5.79 | 343.23 | 0.3229 | -962.0 | -816.8 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 23.41 | 79.09 | 5.63 | 343.97 | 0.3278 | -949.0 | -694.9 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 24.91 | 77.58 | 4.12 | 349.10 | 0.3458 | -841.0 | -643.9 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 26.86 | 77.54 | 4.08 | 350.26 | 0.3771 | -797.0 | -634.4 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 24.94 | 77.24 | 3.78 | 349.98 | 0.3454 | -1026.0 | -822.7 | |
| 0.00 | 1.90 | 0.00 | 1.02 | 26.73 | 77.26 | 3.81 | 350.85 | 0.3743 | -752.0 | -688.1 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 24.33 | 76.72 | 3.26 | 351.03 | 0.3341 | 744.0 | 614.9 | |
| 0.00 | 1.81 | 0.00 | 0.97 | 27.30 | 74.99 | 1.53 | 356.40 | 0.3793 | 834.0 | 644.2 | |
| 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. | |