SDO HMI 2014-12-09 01:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.83 | 0.00 | 10.07 | 14.18 | 18.70 | 24.35 | 302.51 | 0.4783 | -473.2 | -335.1 | |
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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 | 0.43 | 0.00 | 0.25 | 9.64 | 26.80 | 32.45 | 287.73 | 0.5576 | -562.0 | -500.6 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 16.84 | 26.48 | 32.13 | 299.78 | 0.5888 | -667.0 | -572.5 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 12.93 | 25.68 | 31.34 | 293.97 | 0.5569 | -758.0 | -637.8 | |
| 0.00 | 1.02 | 0.00 | 0.60 | 15.12 | 23.50 | 29.16 | 299.17 | 0.5408 | -609.0 | -534.0 | |
| 0.00 | 1.88 | 0.00 | 1.07 | 12.65 | 21.44 | 27.10 | 296.41 | 0.4983 | -695.0 | -458.2 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 6.27 | 20.23 | 25.88 | 284.35 | 0.4498 | -725.0 | -568.1 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 14.02 | 20.93 | 26.58 | 299.33 | 0.5001 | -580.0 | -476.2 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 9.85 | 20.19 | 25.84 | 291.92 | 0.4648 | -813.0 | -679.2 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 12.65 | 18.62 | 24.27 | 298.83 | 0.4598 | -808.0 | -655.6 | |
| 0.00 | 2.64 | 0.00 | 1.47 | 14.08 | 17.61 | 23.26 | 302.60 | 0.4567 | -695.0 | -393.1 | |
| 0.00 | 2.39 | 0.00 | 1.34 | 15.24 | 17.68 | 23.33 | 304.70 | 0.4667 | -754.0 | -584.5 | |
| 0.00 | 2.39 | 0.00 | 1.30 | 18.39 | 10.22 | 15.87 | 320.73 | 0.4117 | 824.0 | 631.8 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 20.59 | 5.96 | 11.61 | 331.94 | 0.4023 | 690.0 | 560.3 | |
| 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. | |