SDO HMI 2014-10-13 12:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.03 | 0.00 | 10.84 | 14.75 | 358.20 | -21.62 | 65.20 | 0.3892 | -565.7 | -519.4 | |
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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 | 1.75 | 0.00 | 0.90 | 10.88 | 4.96 | -14.86 | 70.60 | 0.2683 | -536.0 | -603.8 | |
| 0.00 | 0.52 | 0.00 | 0.27 | 12.03 | 4.04 | -15.78 | 67.70 | 0.2888 | -504.0 | -637.8 | |
| 0.00 | 1.49 | 0.00 | 0.78 | 14.42 | 3.40 | -16.42 | 61.14 | 0.3140 | -830.0 | -714.6 | |
| 0.00 | 3.76 | 0.00 | 1.96 | 14.38 | 3.08 | -16.74 | 61.68 | 0.3183 | -1006.0 | -856.4 | |
| 0.00 | 1.66 | 0.00 | 0.88 | 14.05 | 0.12 | -19.70 | 65.91 | 0.3598 | -741.0 | -479.7 | |
| 0.00 | 1.66 | 0.00 | 0.88 | 14.49 | 359.82 | -20.00 | 65.05 | 0.3669 | -944.0 | -813.8 | |
| 0.00 | 2.01 | 0.00 | 1.07 | 14.79 | 359.66 | -20.16 | 64.45 | 0.3710 | -929.0 | -698.0 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 15.86 | 358.89 | -20.93 | 62.61 | 0.3888 | -724.0 | -541.2 | |
| 0.00 | 1.84 | 0.00 | 0.98 | 14.85 | 358.76 | -21.06 | 65.15 | 0.3845 | -708.0 | -620.7 | |
| 0.00 | 1.49 | 0.00 | 0.81 | 15.95 | 356.36 | -23.47 | 64.66 | 0.4254 | -709.0 | -482.6 | |
| 0.00 | 0.44 | 0.00 | 0.25 | 15.38 | 352.30 | -27.52 | 68.60 | 0.4805 | -663.0 | -569.4 | |
| 0.00 | 2.01 | 0.00 | 1.28 | 17.08 | 341.84 | -37.99 | 70.05 | 0.6282 | 571.0 | 468.5 | |
| 0.00 | 0.26 | 0.00 | 0.17 | 21.12 | 340.56 | -39.26 | 64.39 | 0.6570 | 369.0 | 480.0 | |
| 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. | |