SDO HMI 2014-02-26 01:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.34 | 22.91 | 4.01 | 17.24 | 6.39 | 124.53 | -46.99 | 74.93 | 0.7548 | -349.9 | -253.8 | |
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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 | 0.95 | 0.00 | 0.69 | 9.90 | 127.52 | -44.00 | 69.26 | 0.7341 | -696.0 | -606.4 | |
| 0.00 | 0.69 | 0.00 | 0.50 | 8.73 | 127.50 | -44.03 | 70.79 | 0.7298 | -621.0 | -549.6 | |
| 0.00 | 0.95 | 0.00 | 0.68 | 7.86 | 127.28 | -44.24 | 72.01 | 0.7290 | -687.0 | -580.3 | |
| 0.00 | 1.89 | 0.00 | 1.37 | 8.12 | 127.08 | -44.45 | 71.75 | 0.7323 | -531.0 | -468.8 | |
| 0.00 | 1.03 | 0.00 | 0.74 | 6.85 | 126.99 | -44.53 | 73.46 | 0.7287 | -646.0 | -553.2 | |
| 0.00 | 1.46 | 0.00 | 1.06 | 7.25 | 126.90 | -44.63 | 72.97 | 0.7312 | -731.0 | -621.7 | |
| 0.00 | 1.64 | 0.00 | 1.21 | 8.24 | 125.83 | -45.70 | 72.12 | 0.7466 | -538.0 | -443.9 | |
| 0.00 | 2.07 | 0.00 | 1.53 | 8.09 | 125.81 | -45.72 | 72.32 | 0.7463 | -536.0 | -427.9 | |
| 5.34 | 7.58 | 4.01 | 5.69 | 3.97 | 124.04 | -47.49 | 78.25 | 0.7534 | -692.3 | -431.1 | |
| 0.00 | 1.29 | 0.00 | 1.00 | 4.96 | 122.51 | -49.01 | 77.45 | 0.7728 | 726.0 | 618.9 | |
| 0.00 | 0.95 | 0.00 | 0.76 | 5.18 | 120.86 | -50.66 | 77.66 | 0.7908 | 619.0 | 534.9 | |
| 0.00 | 0.69 | 0.00 | 0.62 | 14.11 | 118.89 | -52.64 | 67.75 | 0.8350 | -480.0 | -454.6 | |
| 0.00 | 1.12 | 0.00 | 0.90 | 5.02 | 120.64 | -50.88 | 77.92 | 0.7927 | 518.0 | 462.5 | |
| 0.00 | 0.60 | 0.00 | 0.49 | 5.53 | 120.16 | -51.37 | 77.44 | 0.7989 | 428.0 | 384.1 | |
| 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. | |