SDO HMI 2014-10-06 04:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.33 | 0.00 | 12.69 | 13.57 | 60.07 | -56.48 | 77.96 | 0.8303 | -234.2 | -212.2 | |
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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 | 0.70 | 0.00 | 0.56 | 13.13 | 64.91 | -51.65 | 78.34 | 0.7821 | -136.0 | -154.6 | |
| 0.00 | 0.88 | 0.00 | 0.69 | 12.59 | 64.96 | -51.59 | 79.03 | 0.7813 | -577.0 | -491.0 | |
| 0.00 | 0.88 | 0.00 | 0.73 | 14.27 | 62.59 | -53.96 | 77.01 | 0.8065 | -469.0 | -423.1 | |
| 0.00 | 1.23 | 0.00 | 1.03 | 14.07 | 62.34 | -54.21 | 77.28 | 0.8089 | -366.0 | -284.2 | |
| 0.00 | 0.70 | 0.00 | 0.61 | 13.88 | 60.56 | -55.99 | 77.59 | 0.8262 | -527.0 | -491.9 | |
| 0.00 | 2.02 | 0.00 | 1.79 | 13.15 | 60.04 | -56.51 | 78.47 | 0.8310 | -469.0 | -377.6 | |
| 0.00 | 0.97 | 0.00 | 0.86 | 13.00 | 59.98 | -56.57 | 78.67 | 0.8315 | -340.0 | -223.5 | |
| 0.00 | 0.62 | 0.00 | 0.55 | 13.55 | 59.72 | -56.83 | 78.00 | 0.8340 | -328.0 | -250.3 | |
| 0.00 | 0.35 | 0.00 | 0.32 | 14.06 | 59.19 | -57.36 | 77.41 | 0.8391 | -255.0 | -221.0 | |
| 0.00 | 0.97 | 0.00 | 0.87 | 13.01 | 59.41 | -57.14 | 78.66 | 0.8369 | -113.0 | -91.2 | |
| 0.00 | 1.41 | 0.00 | 1.31 | 14.24 | 58.24 | -58.32 | 77.22 | 0.8479 | -466.0 | -346.1 | |
| 0.00 | 1.93 | 0.00 | 1.82 | 14.51 | 57.83 | -58.73 | 76.91 | 0.8516 | -361.0 | -291.7 | |
| 0.00 | 0.79 | 0.00 | 0.73 | 12.89 | 58.17 | -58.38 | 78.82 | 0.8482 | 532.0 | 458.6 | |
| 0.00 | 0.88 | 0.00 | 0.82 | 12.65 | 58.20 | -58.35 | 79.10 | 0.8479 | 596.0 | 539.1 | |
| 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. | |