SDO HMI 2014-09-24 22:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.42 | 0.00 | 13.23 | -15.55 | 246.90 | -18.11 | 141.64 | 0.4842 | -711.8 | -599.8 | |
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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 | 1.24 | 0.00 | 0.68 | -15.69 | 252.88 | -12.13 | 152.16 | 0.4348 | 796.0 | 646.1 | |
| 0.00 | 3.18 | 0.00 | 1.80 | -16.10 | 247.09 | -17.92 | 142.58 | 0.4886 | -695.0 | -580.8 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -15.68 | 247.06 | -17.95 | 141.99 | 0.4838 | -950.0 | -763.7 | |
| 0.00 | 1.15 | 0.00 | 0.65 | -15.03 | 247.12 | -17.89 | 141.21 | 0.4756 | -714.0 | -606.5 | |
| 0.00 | 3.71 | 0.00 | 2.09 | -15.26 | 247.07 | -17.94 | 141.44 | 0.4788 | -1016.0 | -788.3 | |
| 0.00 | 1.59 | 0.00 | 0.90 | -15.82 | 246.88 | -18.13 | 141.90 | 0.4871 | -898.0 | -717.7 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -15.98 | 246.80 | -18.21 | 141.99 | 0.4898 | -651.0 | -532.8 | |
| 0.00 | 0.62 | 0.00 | 0.35 | -15.50 | 246.78 | -18.23 | 141.32 | 0.4843 | -725.0 | -602.7 | |
| 0.00 | 1.86 | 0.00 | 1.05 | -15.70 | 246.66 | -18.35 | 141.41 | 0.4877 | -749.0 | -573.6 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -15.11 | 246.03 | -18.98 | 139.66 | 0.4870 | -887.0 | -751.8 | |
| 0.00 | 1.59 | 0.00 | 0.91 | -15.96 | 245.91 | -19.10 | 140.63 | 0.4979 | -744.0 | -565.1 | |
| 0.00 | 2.65 | 0.00 | 1.50 | -15.27 | 245.91 | -19.10 | 139.71 | 0.4901 | -867.0 | -689.9 | |
| 0.00 | 1.33 | 0.00 | 0.75 | -14.98 | 245.94 | -19.07 | 139.35 | 0.4864 | -880.0 | -589.8 | |
| 0.00 | 1.50 | 0.00 | 0.85 | -15.41 | 245.70 | -19.31 | 139.59 | 0.4937 | -985.0 | -789.8 | |
| 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. | |