SDO HMI 2014-11-21 01:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 105.51 | 763.40 | 143.02 | 1054.88 | -13.45 | 164.25 | -67.33 | 105.38 | 0.9313 | 199.6 | -180.8 | |
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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 | 1.12 | 0.00 | 1.15 | -17.29 | 172.47 | -59.11 | 111.05 | 0.8799 | 499.0 | 423.0 | |
| 3.00 | 744.87 | 3.75 | 1025.14 | -13.68 | 166.33 | -65.24 | 105.92 | 0.9192 | 255.1 | -185.7 | |
| 68.11 | -2.00 | 84.96 | -2.00 | -12.98 | 166.19 | -65.39 | 105.15 | 0.9195 | 641.2 | 999999 | |
| 17.67 | -2.00 | 26.81 | -2.00 | -14.09 | 161.90 | -69.68 | 105.71 | 0.9463 | -665.5 | 999999 | |
| 10.47 | -2.00 | 17.26 | -2.00 | -14.64 | 160.28 | -71.29 | 106.08 | 0.9551 | -262.4 | 999999 | |
| 2.14 | 3.60 | 3.47 | 5.84 | -14.01 | 160.57 | -71.00 | 105.47 | 0.9532 | -498.4 | -379.4 | |
| 1.20 | -2.00 | 2.01 | -2.00 | -14.28 | 159.98 | -71.60 | 105.67 | 0.9564 | 104.6 | 999999 | |
| 0.00 | 1.20 | 0.00 | 1.76 | -10.90 | 162.07 | -69.51 | 102.39 | 0.9432 | -363.0 | -352.9 | |
| 1.89 | -2.00 | 3.06 | -2.00 | -13.40 | 160.44 | -71.14 | 104.82 | 0.9535 | -527.9 | 999999 | |
| 1.03 | -2.00 | 1.70 | -2.00 | -13.72 | 160.21 | -71.36 | 105.12 | 0.9549 | -334.8 | 999999 | |
| 0.00 | 9.26 | 0.00 | 15.04 | -12.67 | 160.37 | -71.20 | 104.04 | 0.9534 | 14.0 | 33.0 | |
| 0.00 | 1.63 | 0.00 | 2.85 | -14.34 | 159.12 | -72.45 | 105.64 | 0.9605 | 128.0 | 127.3 | |
| 0.00 | 1.72 | 0.00 | 3.10 | -14.08 | 158.61 | -72.97 | 105.31 | 0.9628 | -97.0 | -55.7 | |
| 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. | |