SDO HMI 2014-12-05 08:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.25 | 0.00 | 11.85 | 13.91 | 19.49 | -23.75 | 58.89 | 0.4600 | -714.2 | -556.7 | |
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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 | 3.33 | 0.00 | 1.80 | 15.21 | 24.46 | -18.77 | 50.40 | 0.4047 | -792.0 | -623.4 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 14.88 | 21.99 | -21.25 | 54.34 | 0.4329 | -844.0 | -681.8 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 14.75 | 21.80 | -21.43 | 54.80 | 0.4342 | -785.0 | -670.4 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 14.94 | 21.45 | -21.78 | 54.86 | 0.4403 | -463.0 | -392.8 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 7.86 | 20.30 | -22.93 | 71.23 | 0.4094 | -814.0 | -689.1 | |
| 0.00 | 2.90 | 0.00 | 1.62 | 14.66 | 19.43 | -23.81 | 57.61 | 0.4644 | -766.0 | -449.1 | |
| 0.00 | 1.54 | 0.00 | 0.86 | 15.46 | 19.23 | -24.00 | 56.33 | 0.4730 | -771.0 | -528.6 | |
| 0.00 | 1.28 | 0.00 | 0.72 | 14.60 | 18.73 | -24.50 | 58.42 | 0.4731 | -638.0 | -455.9 | |
| 0.00 | 1.28 | 0.00 | 0.72 | 13.75 | 18.49 | -24.74 | 60.26 | 0.4702 | -731.0 | -612.8 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 8.93 | 17.48 | -25.76 | 70.76 | 0.4566 | -822.0 | -622.6 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 10.63 | 17.24 | -26.00 | 67.42 | 0.4685 | -852.0 | -684.1 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 10.00 | 17.06 | -26.18 | 68.82 | 0.4679 | -585.0 | -461.6 | |
| 0.00 | 1.62 | 0.00 | 0.92 | 13.32 | 16.69 | -26.55 | 62.63 | 0.4917 | -652.0 | -518.3 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 20.16 | 15.42 | -27.81 | 52.20 | 0.5564 | -602.0 | -488.4 | |
| 0.00 | 0.85 | 0.00 | 0.49 | 15.70 | 15.69 | -27.55 | 59.20 | 0.5204 | -596.0 | -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. | |