SDO HMI 2011-10-24 10:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.20 | 0.00 | 10.28 | 24.08 | 330.33 | 29.16 | 306.99 | 0.5593 | -703.5 | -572.2 | |
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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 |
| 0.00 | 1.65 | 0.00 | 1.01 | 24.73 | 332.25 | 31.09 | 306.50 | 0.5857 | -578.0 | -398.3 | |
| 0.00 | 1.30 | 0.00 | 0.78 | 22.15 | 331.10 | 29.94 | 303.32 | 0.5553 | -776.0 | -548.1 | |
| 0.00 | 1.30 | 0.00 | 0.78 | 22.96 | 331.26 | 30.10 | 304.50 | 0.5625 | -881.0 | -628.7 | |
| 0.00 | 1.30 | 0.00 | 0.77 | 23.45 | 330.22 | 29.06 | 306.08 | 0.5535 | -848.0 | -725.5 | |
| 0.00 | 1.04 | 0.00 | 0.62 | 24.49 | 330.33 | 29.17 | 307.63 | 0.5621 | -653.0 | -530.2 | |
| 0.00 | 0.35 | 0.00 | 0.21 | 23.77 | 330.08 | 28.91 | 306.71 | 0.5540 | -545.0 | -577.8 | |
| 0.00 | 1.22 | 0.00 | 0.72 | 24.05 | 330.11 | 28.94 | 307.13 | 0.5564 | -769.0 | -611.2 | |
| 0.00 | 1.04 | 0.00 | 0.62 | 23.55 | 329.95 | 28.78 | 306.47 | 0.5510 | -725.0 | -623.4 | |
| 0.00 | 2.17 | 0.00 | 1.30 | 24.66 | 329.93 | 28.76 | 308.23 | 0.5588 | -697.0 | -496.2 | |
| 0.00 | 2.26 | 0.00 | 1.34 | 23.85 | 329.69 | 28.52 | 307.15 | 0.5501 | -838.0 | -759.6 | |
| 0.00 | 1.83 | 0.00 | 1.09 | 24.42 | 329.75 | 28.59 | 307.99 | 0.5550 | -618.0 | -550.6 | |
| 0.00 | 1.04 | 0.00 | 0.62 | 25.06 | 329.72 | 28.56 | 309.00 | 0.5594 | -572.0 | -376.2 | |
| 0.00 | 0.70 | 0.00 | 0.42 | 26.22 | 329.39 | 28.22 | 311.05 | 0.5647 | -646.0 | -547.2 | |
| 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. | |