SDO HMI 2014-04-03 20:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.57 | 0.00 | 7.58 | -28.33 | 74.17 | 27.60 | 225.83 | 0.5658 | -564.4 | -484.3 | |
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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 | 0.61 | 0.00 | 0.46 | -21.97 | 94.57 | 48.00 | 246.30 | 0.7550 | 461.0 | 400.6 | |
| 0.00 | 0.44 | 0.00 | 0.28 | -27.72 | 80.74 | 34.17 | 232.56 | 0.6285 | -641.0 | -563.4 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -29.09 | 76.73 | 30.16 | 227.75 | 0.5954 | -578.0 | -451.1 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -28.90 | 76.62 | 30.06 | 227.94 | 0.5929 | -693.0 | -553.2 | |
| 0.00 | 1.23 | 0.00 | 0.76 | -29.56 | 76.52 | 29.95 | 226.92 | 0.5969 | -573.0 | -461.4 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -29.33 | 76.41 | 29.84 | 227.14 | 0.5940 | -669.0 | -478.2 | |
| 0.00 | 1.41 | 0.00 | 0.85 | -28.02 | 75.22 | 28.66 | 228.05 | 0.5714 | -820.0 | -656.5 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -26.12 | 72.45 | 25.88 | 228.45 | 0.5258 | -782.0 | -628.3 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -31.63 | 71.07 | 24.50 | 219.08 | 0.5623 | -693.0 | -637.3 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -27.67 | 68.49 | 21.92 | 221.80 | 0.4981 | -698.0 | -539.5 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -29.68 | 67.75 | 21.18 | 218.00 | 0.5119 | -532.0 | -469.5 | |
| 0.00 | 1.23 | 0.00 | 0.70 | -27.92 | 67.01 | 20.45 | 219.62 | 0.4861 | -591.0 | -555.1 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -30.22 | 67.46 | 20.89 | 216.92 | 0.5150 | -528.0 | -453.0 | |
| 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. | |