SDO HMI 2014-10-05 02:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.96 | 0.00 | 12.38 | -18.19 | 103.68 | -27.17 | 133.56 | 0.5998 | 42.7 | 28.0 | |
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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 | 1.49 | 0.00 | 0.90 | -22.74 | 112.71 | -18.13 | 149.32 | 0.5647 | 783.0 | 493.5 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -13.97 | 111.34 | -19.50 | 136.71 | 0.4744 | 654.0 | 551.7 | |
| 0.00 | 1.23 | 0.00 | 0.70 | -15.20 | 110.93 | -19.91 | 137.90 | 0.4923 | 749.0 | 585.1 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -22.86 | 109.76 | -21.09 | 145.58 | 0.5887 | 612.0 | 470.5 | |
| 0.00 | 1.41 | 0.00 | 0.89 | -23.80 | 107.22 | -23.63 | 143.54 | 0.6194 | 745.0 | 629.6 | |
| 0.00 | 2.46 | 0.00 | 1.48 | -17.47 | 105.95 | -24.90 | 134.65 | 0.5667 | 474.0 | 495.1 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -23.30 | 104.76 | -26.09 | 140.32 | 0.6349 | 549.0 | 414.2 | |
| 0.00 | 1.49 | 0.00 | 0.88 | -15.04 | 105.90 | -24.94 | 131.27 | 0.5440 | 877.0 | 697.1 | |
| 0.00 | 1.41 | 0.00 | 0.90 | -17.30 | 99.59 | -31.26 | 128.09 | 0.6317 | -762.0 | -674.1 | |
| 0.00 | 0.62 | 0.00 | 0.39 | -17.36 | 99.17 | -31.67 | 127.81 | 0.6366 | -699.0 | -640.4 | |
| 0.00 | 0.79 | 0.00 | 0.51 | -17.55 | 98.80 | -32.04 | 127.73 | 0.6420 | -671.0 | -547.0 | |
| 0.00 | 0.97 | 0.00 | 0.63 | -17.36 | 98.21 | -32.64 | 126.99 | 0.6468 | -632.0 | -528.4 | |
| 0.00 | 3.08 | 0.00 | 1.99 | -17.03 | 98.16 | -32.69 | 126.54 | 0.6449 | -767.0 | -613.7 | |
| 0.00 | 0.97 | 0.00 | 0.63 | -17.10 | 97.17 | -33.68 | 125.82 | 0.6559 | -625.0 | -502.7 | |
| 0.00 | 0.88 | 0.00 | 0.58 | -16.11 | 95.89 | -34.95 | 123.57 | 0.6629 | -646.0 | -544.0 | |
| 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. | |