| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.44 | 116.02 | 43.43 | 104.17 | 14.36 | 259.14 | -56.10 | 74.65 | 0.8353 | -325.7 | -93.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-01 10:00:40 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 | 1.36 | 0.00 | 1.07 | 12.82 | 264.68 | -50.56 | 75.82 | 0.7789 | -445.0 | -453.5 | |
| 0.00 | 1.09 | 0.00 | 0.93 | 17.20 | 261.84 | -53.40 | 70.84 | 0.8141 | -573.0 | -509.8 | |
| 12.17 | 23.89 | 10.40 | 20.42 | 16.17 | 261.39 | -53.85 | 72.17 | 0.8168 | -701.2 | -366.5 | |
| 5.09 | -3.00 | 4.35 | -3.00 | 15.85 | 261.30 | -53.94 | 72.57 | 0.8172 | -749.1 | 999999 | |
| 11.18 | 15.99 | 9.51 | 13.60 | 15.03 | 261.39 | -53.84 | 73.55 | 0.8152 | -683.7 | -374.5 | |
| 0.64 | -3.00 | 0.55 | -3.00 | 15.99 | 260.97 | -54.27 | 72.45 | 0.8206 | -163.0 | 999999 | |
| 0.00 | 2.18 | 0.00 | 1.90 | 16.23 | 260.49 | -54.75 | 72.24 | 0.8254 | -271.0 | -142.9 | |
| 0.00 | 1.09 | 0.00 | 0.96 | 16.09 | 260.11 | -55.13 | 72.48 | 0.8289 | -246.0 | -160.7 | |
| 0.00 | 0.91 | 0.00 | 0.81 | 15.87 | 259.41 | -55.83 | 72.84 | 0.8350 | 335.0 | 339.6 | |
| 0.00 | 2.45 | 0.00 | 2.10 | 11.46 | 260.84 | -54.40 | 77.99 | 0.8169 | -390.0 | -296.6 | |
| 3.36 | 10.08 | 2.85 | 8.58 | 10.38 | 261.02 | -54.22 | 79.29 | 0.8143 | -629.9 | -337.0 | |
| 0.00 | 2.36 | 0.00 | 2.10 | 14.90 | 259.57 | -55.67 | 73.97 | 0.8324 | -295.0 | -127.3 | |
| 2.45 | -11.00 | 2.09 | -11.00 | 10.40 | 260.80 | -54.44 | 79.28 | 0.8165 | -468.4 | 999999 | |
| 0.00 | 3.36 | 0.00 | 3.01 | 14.67 | 259.32 | -55.91 | 74.28 | 0.8344 | 390.0 | 388.5 | |
| 0.00 | 1.36 | 0.00 | 1.17 | 10.15 | 260.59 | -54.64 | 79.61 | 0.8183 | -286.0 | -162.9 | |
| 0.00 | 0.55 | 0.00 | 0.51 | 16.64 | 258.14 | -57.10 | 72.11 | 0.8474 | 577.0 | 593.5 | |
| 0.00 | 1.27 | 0.00 | 1.15 | 14.87 | 258.79 | -56.45 | 74.11 | 0.8396 | 639.0 | 523.2 | |
| 0.00 | 0.64 | 0.00 | 0.58 | 14.67 | 258.64 | -56.60 | 74.36 | 0.8408 | 450.0 | 448.9 | |
| 0.00 | 2.18 | 0.00 | 2.00 | 15.10 | 258.40 | -56.83 | 73.88 | 0.8433 | 516.0 | 364.4 | |
| 0.00 | 0.73 | 0.00 | 0.67 | 14.82 | 258.40 | -56.83 | 74.22 | 0.8430 | 567.0 | 505.2 | |
| 0.55 | 2.27 | 0.51 | 2.13 | 16.33 | 257.63 | -57.61 | 72.54 | 0.8515 | 446.5 | 378.1 | |
| 0.00 | 0.64 | 0.00 | 0.59 | 15.43 | 257.86 | -57.38 | 73.57 | 0.8485 | 529.0 | 421.3 | |
| 0.55 | 3.54 | 0.51 | 3.35 | 15.41 | 257.33 | -57.91 | 73.66 | 0.8532 | 467.5 | 322.3 | |
| 0.00 | 1.36 | 0.00 | 1.28 | 14.91 | 257.43 | -57.81 | 74.23 | 0.8518 | 586.0 | 453.1 | |
| 3.91 | 6.00 | 3.72 | 5.70 | 14.89 | 256.95 | -58.28 | 74.31 | 0.8560 | 588.4 | 407.6 | |
| 9.54 | 20.81 | 8.94 | 19.44 | 13.40 | 257.38 | -57.86 | 76.00 | 0.8510 | -636.0 | -415.5 | |
| 0.00 | 1.91 | 0.00 | 1.79 | 12.96 | 257.36 | -57.88 | 76.52 | 0.8508 | -446.0 | -392.8 | |
| 0.00 | 0.55 | 0.00 | 0.51 | 12.55 | 257.04 | -58.20 | 77.04 | 0.8533 | -267.0 | -232.5 | |
| 0.00 | 3.73 | 0.00 | 3.73 | 13.65 | 255.07 | -60.17 | 75.93 | 0.8710 | -121.0 | -191.3 | |
| 0.00 | 1.36 | 0.00 | 1.38 | 12.67 | 254.71 | -60.53 | 77.09 | 0.8734 | -395.0 | -319.6 | |
| 0.00 | 1.09 | 0.00 | 1.14 | 11.87 | 253.52 | -61.72 | 78.08 | 0.8827 | 340.0 | 373.6 | |
| 0.00 | 1.27 | 0.00 | 1.57 | 17.72 | 249.12 | -66.12 | 71.92 | 0.9180 | 444.0 | 325.1 | |
| 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. | |