| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 111.91 | 572.39 | 138.25 | 713.67 | 15.18 | 260.88 | 67.34 | 283.69 | 0.9171 | -60.1 | -97.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-30 08:00:33 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 | 2.73 | 0.00 | 4.48 | 12.55 | 267.00 | 73.46 | 281.07 | 0.9548 | 333.0 | 300.9 | |
| 0.00 | 1.50 | 0.00 | 2.42 | 13.20 | 266.73 | 73.20 | 281.74 | 0.9533 | 302.0 | 284.8 | |
| 0.00 | 2.29 | 0.00 | 3.69 | 12.97 | 266.56 | 73.02 | 281.49 | 0.9524 | 38.0 | 142.4 | |
| 4.94 | 101.94 | 7.69 | 153.69 | 13.16 | 265.96 | 72.43 | 281.66 | 0.9492 | -371.1 | -165.4 | |
| 1.50 | -4.00 | 2.26 | -4.00 | 13.60 | 265.37 | 71.84 | 282.09 | 0.9459 | -218.8 | 999999 | |
| 0.79 | -4.00 | 1.19 | -4.00 | 13.87 | 265.17 | 71.64 | 282.37 | 0.9448 | 101.1 | 999999 | |
| 5.47 | -4.00 | 8.04 | -4.00 | 13.84 | 264.85 | 71.32 | 282.32 | 0.9430 | -513.2 | 999999 | |
| 4.59 | -4.00 | 6.61 | -4.00 | 14.01 | 264.40 | 70.87 | 282.49 | 0.9404 | -662.1 | 999999 | |
| 1.41 | 2.82 | 1.93 | 3.85 | 13.98 | 263.26 | 69.73 | 282.42 | 0.9336 | -436.4 | -427.4 | |
| 0.00 | 0.97 | 0.00 | 1.30 | 13.66 | 262.86 | 69.33 | 282.05 | 0.9313 | -598.0 | -577.8 | |
| 0.00 | 0.79 | 0.00 | 0.99 | 13.33 | 261.04 | 67.51 | 281.64 | 0.9196 | 263.0 | 233.0 | |
| 30.60 | 199.12 | 39.52 | 254.87 | 15.15 | 261.95 | 68.42 | 283.64 | 0.9253 | -706.4 | -329.9 | |
| 6.70 | -12.00 | 8.57 | -12.00 | 15.79 | 261.73 | 68.19 | 284.33 | 0.9237 | -617.6 | 999999 | |
| 7.50 | -12.00 | 9.22 | -12.00 | 14.98 | 260.67 | 67.14 | 283.43 | 0.9169 | 0.0 | 999999 | |
| 0.00 | 1.32 | 0.00 | 1.58 | 13.83 | 259.82 | 66.28 | 282.15 | 0.9111 | 154.0 | 83.6 | |
| 0.00 | 1.15 | 0.00 | 1.44 | 16.97 | 261.24 | 67.71 | 285.61 | 0.9205 | -541.0 | -461.1 | |
| 0.35 | 2.12 | 0.41 | 2.46 | 13.70 | 259.05 | 65.52 | 281.99 | 0.9057 | 438.8 | 397.3 | |
| 0.00 | 5.11 | 0.00 | 5.93 | 14.22 | 259.04 | 65.51 | 282.57 | 0.9056 | 544.0 | 384.6 | |
| 0.00 | 1.23 | 0.00 | 1.41 | 14.57 | 258.71 | 65.18 | 282.95 | 0.9032 | 504.0 | 428.6 | |
| 0.79 | 7.58 | 0.91 | 8.68 | 14.78 | 258.69 | 65.15 | 283.19 | 0.9030 | 475.2 | 295.1 | |
| 1.50 | -20.00 | 1.71 | -20.00 | 15.07 | 258.63 | 65.10 | 283.51 | 0.9025 | 413.1 | 999999 | |
| 2.73 | 15.70 | 3.04 | 17.41 | 14.65 | 257.88 | 64.34 | 283.04 | 0.8970 | 760.7 | 405.0 | |
| 0.26 | 222.93 | 0.30 | 246.15 | 15.57 | 258.33 | 64.80 | 284.06 | 0.9004 | 216.7 | 85.8 | |
| 0.00 | 1.06 | 0.00 | 1.17 | 15.06 | 257.82 | 64.28 | 283.50 | 0.8965 | 571.0 | 508.5 | |
| 4.85 | -23.00 | 5.40 | -23.00 | 15.45 | 257.97 | 64.43 | 283.93 | 0.8977 | 679.0 | 999999 | |
| 6.00 | -23.00 | 6.66 | -23.00 | 15.83 | 257.90 | 64.37 | 284.35 | 0.8972 | 501.9 | 999999 | |
| 26.90 | -23.00 | 29.37 | -23.00 | 16.38 | 257.37 | 63.83 | 284.98 | 0.8932 | 678.4 | 999999 | |
| 0.00 | 0.97 | 0.00 | 1.04 | 15.80 | 256.67 | 63.14 | 284.33 | 0.8879 | 459.0 | 448.0 | |
| 1.59 | -23.00 | 1.74 | -23.00 | 17.47 | 257.40 | 63.87 | 286.20 | 0.8936 | 299.4 | 999999 | |
| 1.15 | -23.00 | 1.24 | -23.00 | 17.42 | 257.01 | 63.47 | 286.15 | 0.8907 | 626.2 | 999999 | |
| 2.29 | -23.00 | 2.44 | -23.00 | 17.09 | 256.52 | 62.99 | 285.79 | 0.8869 | 693.5 | 999999 | |
| 0.00 | 1.06 | 0.00 | 1.11 | 16.96 | 255.96 | 62.43 | 285.66 | 0.8825 | 327.0 | 235.6 | |
| 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. | |