「Speckle」の共起表現一覧(1語右で並び替え)
該当件数 : 36件
The | speckle can also represent some useful information, p |
Roland | Speckle helped with production of the album. |
Diffraction-limited | speckle images of it in visible and near infrared lig |
For the bispectral analysis | speckle imaging method, see speckle masking. |
The use of | speckle imaging using adaptive optics at the WIYN Obs |
s been estimated through very high-resolution | speckle imaging, the results of which suggest that LB |
A search with a near-infrared | speckle interferometer failed to detect a companion o |
t the companion has not been resolved through | speckle interferometery. |
This star was observed to be double in | speckle interferometric observations in 1988, but thi |
orbiting one of the ε2 pair, was detected by | speckle interferometry in 1985 and confirmed in two s |
Radar and | speckle interferometry observations show that the sha |
Although it was observed to be binary by | speckle interferometry in 1985, subsequent observatio |
er of measurements, from Hipparcos and Tycho, | speckle interferometry, and other sources. |
Binary star nature discovered by | speckle interferometry. |
troscopic binary, it has now been resolved by | speckle interferometry. |
nothing, nor did a search with near infrared | speckle interferometry. |
ional influence of another body) and infrared | speckle interferometry. |
Speckle noise in SAR is generally more serious, causi | |
disadvantage of CSLDV is the additional laser | speckle noise that occurs if the laser spot scans the |
thereby reducing the problem of dealing with | speckle noise to a known tractable case. |
Speckle noise in conventional radar results from rand | |
Speckle noise is difficult to predict, depending on t | |
Speckle noise is caused by micro-scale irregularities | |
In SAR oceanography, for example, | speckle noise is caused by signals from elementary sc |
Recent | speckle observations (Weigelt et al. 1998 A&A,333,51, |
Daniel Specklin (or | Speckle or Speckel) (1536 - 18 October 1589) was an A |
The Canadian | Speckle Park is a breed of cattle native to the Canad |
n was formed in 1985, and exports of Canadian | Speckle Park to the U.S. and Australia have occurred. |
Work on breeding the Canadian | Speckle Park began in the 1950s with the crossing of |
The Canadian | Speckle Park is one of the newest cattle breeds, havi |
A | Speckle Park, Stampede Park, Calgary, Alberta |
Electronic | Speckle Pattern Interferometry, also known as TV holo |
new observing instruments, including an early | speckle spectrograph for obtaining spatially resolved |
Speckle structure can be subdued at the expense of re | |
The scale of that random | speckle structure is governed by the size of the synt |
dar cross-section, and the other representing | speckle that is a characteristic of coherent imaging. |
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