Adjective:

আলোকমিতি-সংক্রান্ত,

photometric শব্দের বাংলা অর্থ এর উদাহরণ:

এই উপগ্রহগুলির কক্ষপথ ও আলোকমিতি-সংক্রান্ত বৈশিষ্ট্যগুলি একই ধরনের ।

photometric's Usage Examples:

photometry is conducted by gathering light and passing it through specialized photometric optical bandpass filters, and then capturing and recording the light.

The set of passbands or filters is called a photometric system.

In astronomy, a photometric system is a set of well-defined passbands (or optical filters), with a known sensitivity to incident radiation.

Luminance is a photometric measure of the luminous intensity per unit area of light travelling in a given direction.

Photometric-standard stars are a series of stars that have had their light output in various passbands of photometric system measured very carefully.

The accumulated photometric exposure (Hv) is the same so long as the total exposure time is the same.

involved, brightness transfer function (BTF); it may also be called photometric camera calibration or radiometric camera calibration.

Photometry is typically based on the eye's photopic response, and so photometric measurements may not accurately indicate the perceived brightness of.

bands (J, H, and K) near 2 micrometres (or microns), from which the photometric survey with its HgCdTe detectors derives its name.

The photometric system called UBV (from Ultraviolet, Blue, Visual), also called the Johnson system (or Johnson-Morgan system), is a wide central band.

Flame photometric detector (FPD) uses a photomultiplier tube to detect spectral lines of.

together with other binaries that change brightness as they orbit, photometric binaries.

Standards organizations recommend that photometric quantities be denoted with a subscript "v" (for "visual") to avoid confusion.

Photometric measurements are made in the ultraviolet, visible, or infrared wavelength bands using standard passband filters belonging to photometric systems.

26th General Conference on Weights and Measures (CGPM) redefined the photometric units in 2018.

cluster has been estimated to be from as low as 51 myr (by the first photometric study of the cluster, in 1968, by Lindoff) to as high as 195 myr (by.

the final imaging data release (DR9) covers over 35% of the sky, with photometric observations of around nearly 1 billion objects, while the survey continues.

metallicities through measured and calibrated systems that correlate photometric measurements and spectroscopic measurements (see also Spectrophotometry).

Synonyms:

photometrical;