इंटरफेरोमेट्री हिंदी उपयोग और उदाहरण

वे ध्रुवीकृत चमक के लिए इंटरफेरोमेट्री के क्रमागत अनुप्रयोग, चमक के वितरण और एक हाइड्रोजन परमाणु द्वारा उत्सर्जित 21सेमी लाइन में जीमन इफेक्ट के एक प्रारंभिक अध्ययन करने वालों में भी प्रथम थे।

"" दोहरी पोलरीकरण इंटरफेरोमेट्री का प्रयोग पीएच, तापमान, आयनिक शक्ति या अन्य बंधन सहयोगियों द्वारा उत्तेजित किये जाने पर इन वस्तुओं के परिवर्तनों या स्वतःसमूहन को मापने के लिये किया जा सकता है।

इंटरफेरोमेट्री इसके अंग्रेजी अर्थ का उदाहरण

The telescope will be used in Very-long-baseline interferometry.

Equipment and methods used to examine the worn surfaces include optical microscopes, scanning electron microscopes, optical interferometry and mechanical roughness testers.

In terms of more direct evidence, physical effects of the difference between the rotation of a spin- particle by 360° as compared with 720° have been experimentally observed in classic experiments in neutron interferometry.

History of astronomical interferometry.

The interferometry-measured angular diameter of this star, after correcting for limb darkening, is , which, at its estimated distance, equates to a physical radius of about 11.

The interferometry-measured angular diameter of this star, after correcting for limb darkening, is , which, at its estimated distance, equates to a physical radius of more than 24 times the radius of the Sun.

It has been resolved using speckle interferometry at a distance of 0.

At Palomar Observatory, Antoine Labeyrie and others used speckle interferometry with the Hale Telescope to resolve the system in 1977.

The interferometry-measured angular diameter of this star is about 4.

They can be used to detect explosives and chemical warfare agents, by the means of infrared spectroscopy or to evaluate the plasma densities by the means of interferometry techniques.

" Additionally, some new estimates of the level of holographic noise in interferometry show that it must be much smaller in magnitude than was claimed by Hogan.

The interferometry-measured angular diameter of this star is , which, at its estimated distance, equates to a physical radius of about six times the radius of the Sun.

Since 1981, it has been used primarily for geodetic very long baseline interferometry (VLBI).