SDO HMI 2014-12-05 11:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.65 | 0.00 | 9.16 | -15.90 | 37.94 | -3.66 | 166.99 | 0.2916 | -103.1 | -65.2 | |
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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 | 1.37 | 0.00 | 0.71 | -16.21 | 42.51 | 0.91 | 183.07 | 0.2865 | 949.0 | 851.2 | |
| 0.00 | 1.96 | 0.00 | 1.02 | -18.01 | 42.08 | 0.48 | 181.46 | 0.3163 | 863.0 | 553.4 | |
| 0.00 | 0.43 | 0.00 | 0.22 | -17.32 | 40.69 | -0.91 | 177.14 | 0.3051 | 468.0 | 527.8 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -18.48 | 40.37 | -1.23 | 176.39 | 0.3245 | 666.0 | 542.4 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -19.54 | 40.23 | -1.36 | 176.22 | 0.3422 | 693.0 | 499.7 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -14.92 | 38.47 | -3.13 | 168.66 | 0.2696 | 770.0 | 520.7 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -19.85 | 37.40 | -4.20 | 168.72 | 0.3534 | 733.0 | 579.3 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -14.28 | 36.77 | -4.83 | 162.07 | 0.2663 | -847.0 | -721.4 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -14.09 | 36.68 | -4.92 | 161.54 | 0.2639 | -783.0 | -648.8 | |
| 0.00 | 2.13 | 0.00 | 1.09 | -11.82 | 36.70 | -4.90 | 158.33 | 0.2275 | -883.0 | -536.3 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -13.97 | 36.29 | -5.31 | 160.02 | 0.2641 | -769.0 | -578.2 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -15.22 | 35.67 | -5.93 | 159.61 | 0.2874 | -839.0 | -629.2 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -15.07 | 34.75 | -6.85 | 156.57 | 0.2908 | -984.0 | -741.3 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -15.35 | 34.25 | -7.35 | 155.46 | 0.2984 | -947.0 | -768.8 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -15.50 | 34.24 | -7.36 | 155.66 | 0.3008 | -637.0 | -588.4 | |
| 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. | |