SDO HMI 2014-01-02 10:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.60 | 44.00 | 15.53 | 37.43 | -11.94 | 116.69 | -54.15 | 102.47 | 0.8120 | 438.3 | 233.0 | |
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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 | 0.93 | 0.00 | 0.66 | -14.75 | 125.92 | -44.92 | 107.57 | 0.7186 | 585.0 | 442.6 | |
| 0.00 | 0.59 | 0.00 | 0.42 | -9.76 | 125.90 | -44.94 | 100.63 | 0.7106 | 596.0 | 483.4 | |
| 0.00 | 1.27 | 0.00 | 0.99 | -10.23 | 120.54 | -50.30 | 100.66 | 0.7728 | 446.0 | 347.4 | |
| 10.62 | 21.93 | 8.50 | 17.53 | -11.34 | 119.22 | -51.62 | 101.95 | 0.7879 | 812.6 | 551.1 | |
| 0.00 | 1.44 | 0.00 | 1.18 | -13.68 | 118.50 | -52.34 | 104.81 | 0.7979 | 609.0 | 465.8 | |
| 6.71 | 9.18 | 5.69 | 7.78 | -12.34 | 116.79 | -54.06 | 102.94 | 0.8137 | 590.2 | 284.1 | |
| 0.00 | 1.36 | 0.00 | 1.26 | -12.46 | 113.40 | -57.44 | 102.75 | 0.8460 | 450.0 | 273.4 | |
| 0.00 | 0.76 | 0.00 | 0.73 | -13.79 | 112.08 | -58.76 | 104.19 | 0.8586 | -524.0 | -496.7 | |
| 0.59 | 1.70 | 0.57 | 1.64 | -12.69 | 111.81 | -59.03 | 102.89 | 0.8602 | -599.0 | -530.4 | |
| 0.00 | 0.59 | 0.00 | 0.58 | -11.57 | 111.15 | -59.70 | 101.55 | 0.8654 | -419.0 | -389.4 | |
| 0.00 | 1.19 | 0.00 | 1.17 | -11.71 | 110.97 | -59.87 | 101.71 | 0.8669 | -461.0 | -375.4 | |
| 0.68 | 2.04 | 0.77 | 2.32 | -12.89 | 106.58 | -64.26 | 102.78 | 0.9023 | -373.4 | -295.8 | |
| 0.00 | 1.02 | 0.00 | 1.17 | -12.78 | 106.28 | -64.56 | 102.65 | 0.9044 | -168.0 | -119.9 | |
| 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. | |