SDO HMI 2014-03-15 20:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.15 | 158.26 | 40.71 | 299.22 | 11.25 | 10.04 | 72.92 | 283.76 | 0.9658 | 7.2 | -131.1 | |
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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 |
| 4.00 | 53.68 | 9.02 | 117.67 | 11.85 | 12.57 | 75.45 | 283.90 | 0.9768 | -38.1 | -151.8 | |
| 1.04 | -1.00 | 2.28 | -1.00 | 11.82 | 12.05 | 74.93 | 283.96 | 0.9749 | -404.2 | 999999 | |
| 1.04 | -1.00 | 2.25 | -1.00 | 11.96 | 11.93 | 74.81 | 284.12 | 0.9746 | -327.2 | 999999 | |
| 0.00 | 13.29 | 0.00 | 25.56 | 11.23 | 10.27 | 73.15 | 283.69 | 0.9673 | -603.0 | -553.5 | |
| 0.00 | 2.08 | 0.00 | 3.75 | 10.16 | 9.40 | 72.28 | 282.77 | 0.9626 | -211.0 | -202.5 | |
| 0.00 | 0.87 | 0.00 | 1.57 | 10.88 | 9.42 | 72.30 | 283.49 | 0.9633 | -569.0 | -542.1 | |
| 0.00 | 1.04 | 0.00 | 1.96 | 11.67 | 9.83 | 72.71 | 284.22 | 0.9658 | -305.0 | -325.3 | |
| 2.26 | 87.30 | 3.99 | 148.71 | 11.12 | 8.87 | 71.75 | 283.84 | 0.9610 | -537.0 | -13.8 | |
| 0.69 | -8.00 | 1.22 | -8.00 | 10.95 | 8.77 | 71.65 | 283.69 | 0.9604 | -273.6 | 999999 | |
| 5.99 | -8.00 | 10.11 | -8.00 | 10.40 | 8.26 | 71.14 | 283.22 | 0.9574 | 507.4 | 999999 | |
| 1.48 | -8.00 | 2.53 | -8.00 | 10.76 | 8.46 | 71.34 | 283.56 | 0.9587 | 3.9 | 999999 | |
| 1.82 | -8.00 | 3.07 | -8.00 | 11.17 | 8.04 | 70.91 | 284.06 | 0.9571 | -319.0 | 999999 | |
| 2.35 | -8.00 | 3.83 | -8.00 | 10.81 | 7.55 | 70.43 | 283.78 | 0.9543 | 466.3 | 999999 | |
| 1.48 | -8.00 | 2.41 | -8.00 | 11.43 | 7.35 | 70.23 | 284.47 | 0.9539 | 223.9 | 999999 | |
| 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. | |