SDO HMI 2011-06-13 13:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.53 | 35.62 | 3.95 | 18.84 | -15.55 | 244.54 | -12.65 | 143.27 | 0.3532 | -52.6 | -146.1 | |
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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 | 1.45 | 0.00 | 0.76 | -14.68 | 247.95 | -9.25 | 149.77 | 0.3101 | 733.0 | 637.4 | |
| 0.00 | 1.63 | 0.00 | 0.85 | -15.60 | 247.46 | -9.74 | 150.00 | 0.3272 | 984.0 | 845.3 | |
| 5.26 | 10.87 | 2.75 | 5.70 | -14.66 | 246.03 | -11.16 | 144.87 | 0.3269 | 1073.4 | 738.1 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -14.60 | 245.52 | -11.67 | 143.56 | 0.3310 | 683.0 | 540.3 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -14.85 | 245.16 | -12.04 | 143.18 | 0.3380 | 655.0 | 421.1 | |
| 0.00 | 0.63 | 0.00 | 0.34 | -19.14 | 243.75 | -13.45 | 147.17 | 0.4071 | 709.0 | 503.6 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -15.96 | 243.86 | -13.34 | 142.39 | 0.3651 | -892.0 | -743.1 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -16.12 | 243.68 | -13.51 | 142.32 | 0.3688 | -846.0 | -699.6 | |
| 2.27 | 7.88 | 1.20 | 4.19 | -15.68 | 243.45 | -13.74 | 141.07 | 0.3656 | -1022.4 | -870.2 | |
| 0.00 | 1.18 | 0.00 | 0.63 | -16.60 | 243.09 | -14.11 | 141.97 | 0.3807 | -875.0 | -634.0 | |
| 0.00 | 2.36 | 0.00 | 1.26 | -16.48 | 242.97 | -14.23 | 141.52 | 0.3804 | -802.0 | -637.7 | |
| 0.00 | 0.91 | 0.00 | 0.48 | -15.93 | 242.98 | -14.22 | 140.59 | 0.3737 | -762.0 | -609.7 | |
| 0.00 | 0.91 | 0.00 | 0.48 | -16.00 | 242.61 | -14.58 | 140.01 | 0.3782 | -793.0 | -523.0 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -15.81 | 242.46 | -14.73 | 139.39 | 0.3775 | -846.0 | -749.9 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -18.08 | 241.18 | -16.01 | 140.94 | 0.4179 | -565.0 | -487.4 | |
| 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. | |