SDO HMI 2014-07-09 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.52 | 0.00 | 9.75 | 17.67 | 198.58 | -13.52 | 41.78 | 0.3321 | -459.5 | -377.2 | |
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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 | 0.73 | 0.00 | 0.37 | 17.18 | 202.86 | -9.23 | 33.30 | 0.2804 | -660.0 | -536.6 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 18.09 | 201.81 | -10.29 | 34.31 | 0.3025 | -898.0 | -655.2 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 15.98 | 200.95 | -11.14 | 41.07 | 0.2840 | -759.0 | -484.8 | |
| 0.00 | 1.91 | 0.00 | 1.00 | 18.13 | 200.50 | -11.60 | 37.40 | 0.3159 | -1028.0 | -817.1 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 16.53 | 200.53 | -11.56 | 40.78 | 0.2955 | -705.0 | -503.7 | |
| 0.00 | 3.54 | 0.00 | 1.85 | 17.82 | 200.32 | -11.77 | 38.46 | 0.3137 | -1000.0 | -858.0 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 16.22 | 200.26 | -11.84 | 42.17 | 0.2947 | -743.0 | -570.1 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 17.72 | 200.10 | -12.00 | 39.17 | 0.3148 | -878.0 | -733.0 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 18.06 | 199.19 | -12.90 | 40.47 | 0.3286 | -661.0 | -465.3 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 17.48 | 198.15 | -13.95 | 43.85 | 0.3333 | -763.0 | -593.8 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 18.70 | 194.23 | -17.86 | 48.04 | 0.3924 | 848.0 | 775.1 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 18.54 | 194.08 | -18.01 | 48.59 | 0.3926 | 714.0 | 493.2 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 18.39 | 189.89 | -22.21 | 54.31 | 0.4434 | 559.0 | 414.7 | |
| 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. | |