SDO HMI 2011-07-05 05:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.90 | 104.31 | 22.36 | 94.32 | 15.50 | 26.76 | 56.38 | 286.41 | 0.8383 | -292.3 | -220.0 | |
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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 | 1.09 | 0.00 | 1.06 | 17.03 | 29.24 | 58.85 | 287.88 | 0.8618 | -224.0 | -165.3 | |
| 0.00 | 1.00 | 0.00 | 0.96 | 17.09 | 28.71 | 58.32 | 288.01 | 0.8574 | -443.0 | -331.2 | |
| 14.81 | 78.69 | 13.66 | 72.34 | 15.34 | 27.54 | 57.15 | 286.11 | 0.8454 | -750.5 | -370.2 | |
| 2.45 | -3.00 | 2.24 | -3.00 | 14.95 | 27.14 | 56.76 | 285.70 | 0.8414 | -789.1 | 999999 | |
| 0.55 | -3.00 | 0.49 | -3.00 | 15.12 | 26.87 | 56.48 | 285.93 | 0.8391 | -846.2 | 999999 | |
| 0.00 | 1.73 | 0.00 | 1.59 | 17.34 | 27.39 | 57.01 | 288.48 | 0.8462 | -521.0 | -360.3 | |
| 0.00 | 1.09 | 0.00 | 0.96 | 15.24 | 25.61 | 55.23 | 286.24 | 0.8276 | 401.0 | 272.0 | |
| 2.00 | 9.99 | 1.69 | 8.42 | 15.82 | 23.93 | 53.54 | 287.19 | 0.8121 | 404.5 | 453.6 | |
| 1.82 | -8.00 | 1.53 | -8.00 | 16.02 | 23.73 | 53.35 | 287.46 | 0.8105 | 665.9 | 999999 | |
| 2.36 | 3.45 | 1.99 | 2.92 | 16.65 | 23.77 | 53.38 | 288.22 | 0.8118 | 513.6 | 332.4 | |
| 0.91 | 1.64 | 0.76 | 1.37 | 16.34 | 23.65 | 53.26 | 287.87 | 0.8101 | 547.8 | 554.1 | |
| 0.00 | 1.54 | 0.00 | 1.29 | 15.66 | 23.38 | 53.00 | 287.07 | 0.8066 | 614.0 | 522.4 | |
| 0.00 | 2.27 | 0.00 | 1.91 | 16.22 | 23.60 | 53.21 | 287.72 | 0.8095 | 773.0 | 601.6 | |
| 0.00 | 1.82 | 0.00 | 1.50 | 16.15 | 22.88 | 52.50 | 287.76 | 0.8024 | 666.0 | 581.7 | |
| 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. | |