SDO HMI 2014-09-26 08:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.10 | 20.85 | 2.11 | 13.98 | 8.82 | 288.59 | 42.27 | 275.27 | 0.6676 | -349.4 | -339.8 | |
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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 | 0.44 | 0.00 | 0.34 | 8.38 | 296.79 | 50.47 | 275.16 | 0.7685 | -597.0 | -530.6 | |
| 0.80 | 2.39 | 0.57 | 1.72 | 5.16 | 292.99 | 46.67 | 270.55 | 0.7268 | -563.1 | -448.6 | |
| 0.00 | 0.97 | 0.00 | 0.70 | 5.26 | 292.83 | 46.51 | 270.67 | 0.7247 | -643.0 | -605.2 | |
| 0.00 | 0.71 | 0.00 | 0.50 | 8.01 | 292.55 | 46.23 | 274.46 | 0.7196 | -595.0 | -534.9 | |
| 0.00 | 0.88 | 0.00 | 0.63 | 10.32 | 292.81 | 46.49 | 277.68 | 0.7223 | -558.0 | -482.7 | |
| 0.00 | 0.97 | 0.00 | 0.69 | 10.00 | 292.66 | 46.34 | 277.23 | 0.7205 | -722.0 | -581.5 | |
| 0.00 | 0.80 | 0.00 | 0.56 | 7.59 | 292.09 | 45.77 | 273.86 | 0.7142 | -502.0 | -422.9 | |
| 2.30 | 4.33 | 1.54 | 2.90 | 10.89 | 288.95 | 42.63 | 278.59 | 0.6749 | -764.3 | -580.2 | |
| 0.00 | 1.06 | 0.00 | 0.70 | 6.67 | 288.31 | 41.99 | 272.28 | 0.6673 | 717.0 | 574.8 | |
| 0.00 | 1.68 | 0.00 | 1.11 | 11.62 | 288.17 | 41.85 | 279.73 | 0.6654 | -617.0 | -542.4 | |
| 0.00 | 3.80 | 0.00 | 2.50 | 11.98 | 287.87 | 41.55 | 280.29 | 0.6617 | -703.0 | -593.3 | |
| 0.00 | 1.41 | 0.00 | 0.89 | 4.54 | 284.29 | 37.97 | 268.50 | 0.6158 | 468.0 | 405.4 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 4.25 | 264.88 | 18.56 | 262.76 | 0.3214 | 669.0 | 551.6 | |
| 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. | |