| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.10 | 186.11 | 41.72 | 129.26 | -10.68 | 295.89 | 44.90 | 261.90 | 0.7023 | -73.3 | -51.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-19 08:00:30 UT
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 | 1.05 | 0.00 | 0.90 | -10.64 | 306.30 | 55.32 | 261.94 | 0.8184 | 353.0 | 372.2 | |
| 0.00 | 0.87 | 0.00 | 0.74 | -10.42 | 306.03 | 55.04 | 262.22 | 0.8158 | 468.0 | 413.6 | |
| 0.00 | 0.70 | 0.00 | 0.59 | -11.08 | 306.10 | 55.12 | 261.40 | 0.8164 | 553.0 | 422.8 | |
| 0.00 | 1.22 | 0.00 | 0.97 | -14.56 | 303.12 | 52.14 | 257.00 | 0.7865 | 566.0 | 470.6 | |
| 0.00 | 1.13 | 0.00 | 0.86 | -5.25 | 300.69 | 49.70 | 269.13 | 0.7619 | 382.0 | 401.0 | |
| 0.00 | 0.78 | 0.00 | 0.57 | -8.05 | 298.63 | 47.65 | 265.56 | 0.7362 | -609.0 | -533.6 | |
| 0.00 | 0.87 | 0.00 | 0.64 | -8.26 | 298.66 | 47.68 | 265.27 | 0.7365 | -579.0 | -486.9 | |
| 0.00 | 1.05 | 0.00 | 0.76 | -10.01 | 298.57 | 47.58 | 262.88 | 0.7349 | 209.0 | 154.6 | |
| 0.00 | 1.83 | 0.00 | 1.33 | -10.31 | 298.58 | 47.59 | 262.47 | 0.7351 | 228.0 | 188.2 | |
| 8.10 | 11.50 | 5.88 | 8.35 | -10.66 | 298.42 | 47.44 | 262.00 | 0.7333 | 694.1 | 495.3 | |
| 5.75 | 34.50 | 4.16 | 24.87 | -10.19 | 298.20 | 47.21 | 262.63 | 0.7306 | 705.0 | 653.1 | |
| 9.15 | -11.00 | 6.60 | -11.00 | -9.81 | 298.08 | 47.09 | 263.16 | 0.7292 | 909.1 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.68 | -10.04 | 297.54 | 46.56 | 262.85 | 0.7229 | 787.0 | 592.1 | |
| 0.00 | 6.27 | 0.00 | 4.45 | -10.53 | 297.06 | 46.08 | 262.16 | 0.7171 | 641.0 | 532.2 | |
| 1.66 | 6.80 | 1.17 | 4.80 | -9.83 | 296.85 | 45.86 | 263.15 | 0.7145 | 859.3 | 648.6 | |
| 0.00 | 1.22 | 0.00 | 0.86 | -10.85 | 296.86 | 45.87 | 261.71 | 0.7148 | 722.0 | 616.2 | |
| 0.00 | 2.35 | 0.00 | 1.66 | -11.05 | 296.68 | 45.69 | 261.43 | 0.7126 | 893.0 | 734.9 | |
| 0.00 | 1.57 | 0.00 | 1.09 | -10.43 | 296.13 | 45.14 | 262.29 | 0.7058 | 208.0 | 168.8 | |
| 3.05 | 7.06 | 2.10 | 4.87 | -11.09 | 295.52 | 44.53 | 261.34 | 0.6985 | -493.1 | -334.3 | |
| 0.00 | 1.05 | 0.00 | 0.73 | -12.60 | 295.79 | 44.80 | 259.19 | 0.7025 | -199.0 | -228.5 | |
| 1.39 | 2.96 | 0.96 | 2.04 | -10.35 | 295.30 | 44.31 | 262.40 | 0.6956 | -535.1 | -358.9 | |
| 0.78 | 2.35 | 0.54 | 1.61 | -10.80 | 294.96 | 43.97 | 261.74 | 0.6915 | -589.4 | -290.8 | |
| 0.35 | 1.83 | 0.24 | 1.25 | -11.37 | 295.02 | 44.03 | 260.92 | 0.6924 | -569.0 | -451.8 | |
| 0.00 | 6.19 | 0.00 | 4.22 | -10.42 | 294.85 | 43.86 | 262.29 | 0.6900 | -322.0 | -185.0 | |
| 0.00 | 1.22 | 0.00 | 0.83 | -11.74 | 294.58 | 43.60 | 260.36 | 0.6872 | -335.0 | -299.5 | |
| 5.92 | 86.78 | 4.00 | 58.26 | -10.78 | 294.15 | 43.17 | 261.75 | 0.6814 | -715.9 | -511.3 | |
| 1.74 | -26.00 | 1.18 | -26.00 | -11.61 | 294.31 | 43.32 | 260.53 | 0.6836 | -660.0 | 999999 | |
| 3.57 | -26.00 | 2.41 | -26.00 | -11.48 | 294.07 | 43.08 | 260.72 | 0.6806 | -842.4 | 999999 | |
| 1.13 | -26.00 | 0.76 | -26.00 | -10.96 | 293.77 | 42.78 | 261.47 | 0.6766 | -894.7 | 999999 | |
| 7.14 | -26.00 | 4.79 | -26.00 | -11.29 | 293.79 | 42.80 | 260.98 | 0.6769 | -978.2 | 999999 | |
| 9.50 | -26.00 | 6.35 | -26.00 | -10.83 | 293.58 | 42.59 | 261.66 | 0.6741 | -1051.9 | 999999 | |
| 0.87 | -26.00 | 0.58 | -26.00 | -10.60 | 293.37 | 42.39 | 261.99 | 0.6715 | -924.9 | 999999 | |
| 0.00 | 0.78 | 0.00 | 0.52 | -11.85 | 293.56 | 42.57 | 260.13 | 0.6744 | -639.0 | -489.7 | |
| 0.00 | 0.87 | 0.00 | 0.58 | -12.05 | 293.31 | 42.32 | 259.82 | 0.6713 | -628.0 | -531.4 | |
| 0.00 | 0.35 | 0.00 | 0.23 | -16.16 | 292.44 | 41.46 | 253.56 | 0.6653 | -488.0 | -491.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |