SDO HMI 2014-07-09 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.15 | 193.24 | 37.53 | 200.31 | -11.99 | 267.91 | 59.66 | 254.13 | 0.8795 | 67.6 | -119.0 | |
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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 | 0.73 | 0.00 | 0.87 | -13.59 | 271.98 | 63.72 | 253.23 | 0.9120 | 240.0 | 291.1 | |
| 0.00 | 0.73 | 0.00 | 0.83 | -12.70 | 270.87 | 62.61 | 253.97 | 0.9030 | 370.0 | 365.5 | |
| 3.54 | 93.20 | 3.80 | 100.39 | -10.29 | 269.41 | 61.15 | 256.35 | 0.8888 | 783.9 | 94.4 | |
| 1.18 | 2.73 | 1.31 | 3.03 | -12.37 | 270.12 | 61.86 | 254.18 | 0.8970 | 510.3 | 404.9 | |
| 14.17 | -3.00 | 15.18 | -3.00 | -10.66 | 269.27 | 61.02 | 255.91 | 0.8882 | 730.0 | 999999 | |
| 1.09 | -3.00 | 1.14 | -3.00 | -10.56 | 268.60 | 60.34 | 255.90 | 0.8828 | 581.8 | 999999 | |
| 0.00 | 1.09 | 0.00 | 1.18 | -14.01 | 268.91 | 60.66 | 252.13 | 0.8905 | -335.0 | -239.8 | |
| 0.00 | 0.91 | 0.00 | 0.95 | -12.80 | 268.28 | 60.02 | 253.33 | 0.8837 | 387.0 | 333.2 | |
| 0.00 | 1.00 | 0.00 | 0.97 | -8.57 | 266.63 | 58.37 | 257.76 | 0.8635 | 521.0 | 478.2 | |
| 0.00 | 0.64 | 0.00 | 0.62 | -10.11 | 266.33 | 58.07 | 255.94 | 0.8633 | 414.0 | 297.9 | |
| 0.64 | 1.73 | 0.65 | 1.77 | -13.95 | 267.37 | 59.12 | 251.84 | 0.8785 | -373.7 | -239.2 | |
| 15.53 | 87.56 | 15.45 | 86.90 | -13.48 | 266.33 | 58.08 | 252.12 | 0.8692 | -812.2 | -386.7 | |
| 0.00 | 0.55 | 0.00 | 0.53 | -12.97 | 265.26 | 57.01 | 252.43 | 0.8593 | -224.0 | -220.8 | |
| 0.00 | 1.64 | 0.00 | 1.57 | -14.19 | 264.91 | 56.65 | 250.95 | 0.8588 | -511.0 | -422.2 | |
| 0.00 | 0.73 | 0.00 | 0.70 | -14.49 | 265.02 | 56.77 | 250.65 | 0.8603 | -315.0 | -294.8 | |
| 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. | |