SDO HMI 2014-07-01 14:00:40 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.88 | 136.16 | 40.85 | 114.28 | 14.64 | 259.77 | -53.26 | 73.93 | 0.8088 | -338.9 | -132.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-01 14:00:40 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 | 1.00 | 0.00 | 0.73 | 11.06 | 266.23 | -46.80 | 77.58 | 0.7349 | 578.0 | 490.5 | |
| 0.00 | 1.00 | 0.00 | 0.77 | 13.13 | 263.48 | -49.55 | 75.26 | 0.7685 | -130.0 | -242.5 | |
| 0.00 | 0.36 | 0.00 | 0.29 | 17.28 | 261.98 | -51.06 | 70.27 | 0.7912 | -470.0 | -541.8 | |
| 0.00 | 0.54 | 0.00 | 0.44 | 17.15 | 261.72 | -51.32 | 70.50 | 0.7935 | -518.0 | -473.8 | |
| 18.35 | 46.05 | 14.89 | 37.37 | 16.00 | 261.48 | -51.55 | 71.97 | 0.7939 | -761.4 | -294.4 | |
| 5.81 | 14.08 | 4.70 | 11.40 | 14.96 | 261.44 | -51.60 | 73.28 | 0.7928 | -777.2 | -515.8 | |
| 2.09 | -5.00 | 1.72 | -5.00 | 16.07 | 260.89 | -52.15 | 71.99 | 0.8000 | -356.1 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.90 | 16.20 | 260.84 | -52.19 | 71.85 | 0.8007 | -155.0 | -228.2 | |
| 0.00 | 0.82 | 0.00 | 0.68 | 16.25 | 260.61 | -52.42 | 71.82 | 0.8030 | -275.0 | -180.0 | |
| 0.00 | 0.82 | 0.00 | 0.66 | 11.78 | 261.43 | -51.61 | 77.28 | 0.7888 | -395.0 | -343.4 | |
| 0.00 | 1.00 | 0.00 | 0.80 | 10.92 | 261.49 | -51.54 | 78.37 | 0.7872 | -518.0 | -469.4 | |
| 0.00 | 0.64 | 0.00 | 0.51 | 10.70 | 261.44 | -51.59 | 78.65 | 0.7875 | -519.0 | -456.0 | |
| 0.00 | 0.73 | 0.00 | 0.61 | 15.16 | 260.12 | -52.91 | 73.25 | 0.8063 | -439.0 | -396.2 | |
| 6.18 | 9.26 | 4.98 | 7.47 | 10.28 | 261.09 | -51.95 | 79.22 | 0.7909 | -512.9 | -308.9 | |
| 0.00 | 1.91 | 0.00 | 1.63 | 16.07 | 259.19 | -53.84 | 72.29 | 0.8166 | -64.0 | 9.9 | |
| 0.00 | 9.17 | 0.00 | 7.77 | 14.79 | 259.41 | -53.63 | 73.82 | 0.8128 | 462.0 | 352.4 | |
| 0.91 | 3.09 | 0.79 | 2.70 | 16.54 | 258.29 | -54.75 | 71.87 | 0.8258 | 628.4 | 529.9 | |
| 0.00 | 1.27 | 0.00 | 1.12 | 16.69 | 258.06 | -54.98 | 71.73 | 0.8282 | 455.0 | 416.1 | |
| 0.00 | 1.63 | 0.00 | 1.40 | 14.58 | 258.84 | -54.20 | 74.16 | 0.8181 | 643.0 | 562.6 | |
| 1.09 | 2.27 | 0.96 | 2.01 | 16.33 | 257.71 | -55.33 | 72.22 | 0.8310 | 599.5 | 464.2 | |
| 0.00 | 2.54 | 0.00 | 2.22 | 14.96 | 258.15 | -54.89 | 73.80 | 0.8251 | 419.0 | 421.9 | |
| 0.00 | 0.73 | 0.00 | 0.65 | 15.40 | 257.42 | -55.62 | 73.37 | 0.8325 | 534.0 | 447.9 | |
| 0.00 | 3.09 | 0.00 | 2.76 | 15.49 | 257.16 | -55.88 | 73.30 | 0.8350 | 509.0 | 403.9 | |
| 1.91 | 26.25 | 1.68 | 23.15 | 13.31 | 257.64 | -55.40 | 75.85 | 0.8282 | -870.5 | -473.9 | |
| 3.09 | 4.54 | 2.78 | 4.08 | 14.88 | 256.94 | -56.09 | 74.05 | 0.8363 | 607.3 | 434.5 | |
| 7.72 | -24.00 | 6.83 | -24.00 | 13.43 | 257.37 | -55.66 | 75.74 | 0.8308 | -482.3 | 999999 | |
| 1.73 | -24.00 | 1.52 | -24.00 | 13.09 | 257.43 | -55.60 | 76.14 | 0.8299 | -547.9 | 999999 | |
| 0.00 | 0.73 | 0.00 | 0.65 | 8.08 | 256.86 | -56.17 | 82.21 | 0.8322 | 280.0 | 201.8 | |
| 0.00 | 0.91 | 0.00 | 0.89 | 15.41 | 253.68 | -59.36 | 73.83 | 0.8656 | -527.0 | -463.7 | |
| 0.00 | 0.64 | 0.00 | 0.62 | 11.87 | 253.58 | -59.46 | 77.93 | 0.8639 | 494.0 | 471.6 | |
| 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. | |