SDO HMI 2014-04-24 22:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.83 | 56.81 | 23.28 | 55.12 | -10.38 | 187.71 | 59.51 | 260.74 | 0.8603 | 243.8 | 5.4 | |
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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 |
| 8.00 | 33.51 | 8.03 | 33.76 | -10.09 | 188.95 | 60.76 | 261.11 | 0.8715 | 554.4 | 6.3 | |
| 6.58 | -1.00 | 6.60 | -1.00 | -10.33 | 188.97 | 60.77 | 260.83 | 0.8716 | 549.3 | 999999 | |
| 2.58 | 6.93 | 2.55 | 6.87 | -9.41 | 188.56 | 60.36 | 261.89 | 0.8681 | 625.6 | 449.3 | |
| 1.87 | -3.00 | 1.85 | -3.00 | -9.60 | 188.55 | 60.36 | 261.68 | 0.8681 | 667.1 | 999999 | |
| 0.00 | 1.07 | 0.00 | 1.07 | -11.45 | 188.78 | 60.58 | 259.55 | 0.8702 | 347.0 | 324.5 | |
| 0.00 | 1.69 | 0.00 | 1.52 | -10.20 | 185.11 | 56.91 | 260.93 | 0.8372 | -544.0 | -399.1 | |
| 0.71 | 1.96 | 0.64 | 1.77 | -10.81 | 185.17 | 56.97 | 260.20 | 0.8378 | -499.6 | -424.3 | |
| 0.00 | 1.07 | 0.00 | 0.96 | -11.14 | 184.87 | 56.67 | 259.80 | 0.8351 | -225.0 | -270.4 | |
| 4.09 | 5.51 | 3.61 | 4.87 | -10.83 | 184.39 | 56.19 | 260.15 | 0.8304 | -585.5 | -415.4 | |
| 0.00 | 0.71 | 0.00 | 0.61 | -11.11 | 183.04 | 54.85 | 259.77 | 0.8175 | -442.0 | -366.6 | |
| 0.00 | 0.53 | 0.00 | 0.46 | -11.39 | 182.96 | 54.77 | 259.42 | 0.8168 | -377.0 | -304.3 | |
| 0.00 | 0.80 | 0.00 | 0.68 | -11.28 | 182.77 | 54.58 | 259.55 | 0.8148 | -526.0 | -470.0 | |
| 0.00 | 1.96 | 0.00 | 1.67 | -12.22 | 182.94 | 54.74 | 258.41 | 0.8169 | 407.0 | 447.5 | |
| 0.00 | 1.07 | 0.00 | 0.88 | -13.85 | 181.45 | 53.25 | 256.27 | 0.8030 | 513.0 | 448.1 | |
| 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. | |