SDO HMI 2014-10-07 19:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.96 | 14.28 | 0.65 | 9.82 | -13.61 | 56.06 | -39.07 | 117.61 | 0.6907 | -96.4 | -80.7 | |
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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 | 1.58 | 0.00 | 1.00 | -13.24 | 61.68 | -33.45 | 120.65 | 0.6259 | 865.0 | 690.2 | |
| 0.00 | 1.05 | 0.00 | 0.69 | -13.49 | 59.39 | -35.74 | 119.35 | 0.6539 | 486.0 | 371.4 | |
| 0.00 | 1.05 | 0.00 | 0.70 | -13.80 | 58.45 | -36.67 | 119.16 | 0.6665 | -628.0 | -556.2 | |
| 0.00 | 1.93 | 0.00 | 1.27 | -12.11 | 58.32 | -36.80 | 116.76 | 0.6583 | 671.0 | 482.7 | |
| 0.00 | 0.70 | 0.00 | 0.47 | -13.43 | 57.82 | -37.30 | 118.26 | 0.6715 | -658.0 | -476.0 | |
| 0.00 | 1.93 | 0.00 | 1.29 | -13.55 | 57.57 | -37.56 | 118.25 | 0.6750 | -719.0 | -643.2 | |
| 0.96 | 2.19 | 0.65 | 1.47 | -13.33 | 57.49 | -37.63 | 117.91 | 0.6747 | -760.0 | -621.6 | |
| 0.00 | 0.96 | 0.00 | 0.67 | -15.30 | 55.74 | -39.39 | 119.41 | 0.7050 | 693.0 | 569.9 | |
| 0.00 | 1.05 | 0.00 | 0.80 | -16.84 | 50.75 | -44.37 | 118.54 | 0.7642 | -544.0 | -371.2 | |
| 0.00 | 1.23 | 0.00 | 0.92 | -12.08 | 49.80 | -45.32 | 112.24 | 0.7535 | -192.0 | -206.6 | |
| 0.00 | 0.61 | 0.00 | 0.54 | -14.51 | 42.84 | -52.29 | 112.34 | 0.8302 | -507.0 | -439.9 | |
| 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. | |