SDO HMI 2014-03-01 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 |
| 23.55 | 67.81 | 12.95 | 37.06 | -7.64 | 150.58 | 25.13 | 267.42 | 0.4230 | 610.7 | 415.6 | |
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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 |
| 11.56 | 52.89 | 6.37 | 29.09 | -7.77 | 151.58 | 26.13 | 267.04 | 0.4388 | 995.3 | 541.5 | |
| 11.39 | -1.00 | 6.25 | -1.00 | -7.74 | 151.18 | 25.73 | 267.14 | 0.4326 | 1172.1 | 999999 | |
| 0.60 | 1.47 | 0.33 | 0.80 | -7.42 | 150.33 | 24.88 | 267.90 | 0.4193 | 994.9 | 869.8 | |
| 0.00 | 3.45 | 0.00 | 1.88 | -7.19 | 150.25 | 24.80 | 268.47 | 0.4181 | 739.0 | 512.4 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -7.37 | 149.57 | 24.12 | 268.06 | 0.4073 | 598.0 | 420.8 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -6.42 | 148.86 | 23.42 | 270.50 | 0.3967 | 804.0 | 716.2 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -5.51 | 146.85 | 21.41 | 273.32 | 0.3655 | -699.0 | -535.2 | |
| 0.00 | 1.81 | 0.00 | 0.96 | -9.14 | 146.65 | 21.20 | 263.27 | 0.3611 | 801.0 | 669.3 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -8.39 | 146.28 | 20.83 | 265.34 | 0.3546 | 713.0 | 433.2 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -9.30 | 145.02 | 19.57 | 262.47 | 0.3349 | -706.0 | -647.2 | |
| 0.00 | 1.38 | 0.00 | 0.72 | -5.66 | 144.57 | 19.12 | 273.53 | 0.3280 | -796.0 | -710.6 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -6.08 | 144.49 | 19.04 | 272.27 | 0.3261 | -803.0 | -563.2 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -5.73 | 144.41 | 18.97 | 273.37 | 0.3254 | -1015.0 | -741.3 | |
| 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. | |