SDO HMI 2014-03-08 13:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.17 | 34.99 | 12.69 | 48.63 | -18.62 | 322.90 | -70.32 | 107.22 | 0.9354 | 15.9 | -53.9 | |
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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 |
| 0.95 | 6.15 | 1.19 | 7.66 | -18.26 | 325.60 | -67.63 | 106.82 | 0.9191 | 572.2 | 455.9 | |
| 1.99 | -1.00 | 2.49 | -1.00 | -18.07 | 325.50 | -67.72 | 106.60 | 0.9197 | 500.7 | 999999 | |
| 0.00 | 1.56 | 0.00 | 2.07 | -19.10 | 323.91 | -69.31 | 107.73 | 0.9297 | -419.0 | -381.8 | |
| 0.00 | 0.52 | 0.00 | 0.68 | -18.41 | 324.44 | -68.78 | 106.98 | 0.9265 | -164.0 | -168.2 | |
| 0.00 | 0.61 | 0.00 | 0.79 | -18.21 | 324.54 | -68.69 | 106.76 | 0.9259 | 267.0 | 280.9 | |
| 0.00 | 2.16 | 0.00 | 2.94 | -19.23 | 323.42 | -69.80 | 107.87 | 0.9327 | -364.0 | -244.8 | |
| 0.00 | 1.30 | 0.00 | 1.74 | -18.83 | 323.71 | -69.51 | 107.44 | 0.9309 | -544.0 | -476.5 | |
| 0.00 | 1.30 | 0.00 | 1.72 | -18.28 | 324.12 | -69.11 | 106.84 | 0.9285 | -64.0 | -83.1 | |
| 0.43 | 1.21 | 0.57 | 1.60 | -18.07 | 324.21 | -69.02 | 106.62 | 0.9279 | 143.6 | 102.0 | |
| 0.00 | 0.78 | 0.00 | 1.02 | -17.90 | 324.35 | -68.87 | 106.43 | 0.9270 | 375.0 | 357.4 | |
| 1.73 | 5.63 | 2.37 | 7.73 | -18.90 | 323.27 | -69.95 | 107.52 | 0.9335 | -199.1 | 2.3 | |
| 0.00 | 0.69 | 0.00 | 0.97 | -19.21 | 322.69 | -70.54 | 107.86 | 0.9369 | 301.0 | 266.8 | |
| 1.21 | 5.37 | 1.88 | 8.33 | -19.60 | 320.43 | -72.80 | 108.31 | 0.9493 | -272.9 | -164.1 | |
| 0.78 | 2.60 | 1.17 | 3.90 | -18.75 | 321.17 | -72.05 | 107.39 | 0.9455 | -439.2 | -405.8 | |
| 0.00 | 0.52 | 0.00 | 0.80 | -19.25 | 320.62 | -72.60 | 107.93 | 0.9483 | -317.0 | -297.3 | |
| 2.08 | 4.59 | 3.02 | 6.68 | -17.31 | 321.91 | -71.32 | 105.84 | 0.9416 | 252.9 | 78.0 | |
| 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. | |