Перевод и анализ слов искусственным интеллектом ChatGPT
На этой странице Вы можете получить подробный анализ слова или словосочетания, произведенный с помощью лучшей на сегодняшний день технологии искусственного интеллекта:
- как употребляется слово
- частота употребления
- используется оно чаще в устной или письменной речи
- варианты перевода слова
- примеры употребления (несколько фраз с переводом)
- этимология
data element - перевод на русский
общая лексика
элемент данных
одиночное данное
синоним
общая лексика
DD
словарь данных
список всех файлов, полей и переменных, используемых в конкретной СУБД. Позволяет разработчику (в некоторых СУБД и пользователю) определить, как были заданы те или иные элементы
набор описаний данных, который может использоваться несколькими приложениями
Смотрите также
математика
принадлежность множеству
![[[Dmitri Mendeleev]]](https://commons.wikimedia.org/wiki/Special:FilePath/DIMendeleevCab.jpg?width=200 "[[Dmitri Mendeleev]]")
![[[Henry Moseley]]](https://commons.wikimedia.org/wiki/Special:FilePath/Henry Moseley.jpg?width=200 "[[Henry Moseley]]")
![[[Mendeleev]]'s 1869 [[periodic table]]: ''An experiment on a system of elements. Based on their atomic weights and chemical similarities.''](https://commons.wikimedia.org/wiki/Special:FilePath/Mendeleev's 1869 periodic table.svg?width=200 "[[Mendeleev]]'s 1869 [[periodic table]]: ''An experiment on a system of elements. Based on their atomic weights and chemical similarities.''")
![Periodic table showing the cosmogenic origin of each element in the Big Bang, or in large or small stars. Small stars can produce certain elements up to sulfur, by the [[alpha process]]. Supernovae are needed to produce "heavy" elements (those beyond iron and nickel) rapidly by neutron buildup, in the [[r-process]]. Certain large stars slowly produce other elements heavier than iron, in the [[s-process]]; these may then be blown into space in the off-gassing of [[planetary nebulae]]](https://commons.wikimedia.org/wiki/Special:FilePath/Nucleosynthesis periodic table.svg?width=200 "Periodic table showing the cosmogenic origin of each element in the Big Bang, or in large or small stars. Small stars can produce certain elements up to sulfur, by the [[alpha process]]. Supernovae are needed to produce \"heavy\" elements (those beyond iron and nickel) rapidly by neutron buildup, in the [[r-process]]. Certain large stars slowly produce other elements heavier than iron, in the [[s-process]]; these may then be blown into space in the off-gassing of [[planetary nebulae]]")
, black and white.png?width=200 "link=Periodic table")
![Abundances of the chemical elements in the Solar System. Hydrogen and helium are most common, from the Big Bang. The next three elements (Li, Be, B) are rare because they are poorly synthesized in the Big Bang and also in stars. The two general trends in the remaining stellar-produced elements are: (1) an alternation of abundance in elements as they have even or odd atomic numbers (the [[Oddo-Harkins rule]]), and (2) a general decrease in abundance as elements become heavier. Iron is especially common because it represents the minimum energy nuclide that can be made by fusion of helium in supernovae.](https://commons.wikimedia.org/wiki/Special:FilePath/SolarSystemAbundances.png?width=200 "Abundances of the chemical elements in the Solar System. Hydrogen and helium are most common, from the Big Bang. The next three elements (Li, Be, B) are rare because they are poorly synthesized in the Big Bang and also in stars. The two general trends in the remaining stellar-produced elements are: (1) an alternation of abundance in elements as they have even or odd atomic numbers (the [[Oddo-Harkins rule]]), and (2) a general decrease in abundance as elements become heavier. Iron is especially common because it represents the minimum energy nuclide that can be made by fusion of helium in supernovae.")
общая лексика
очистка данных
процедура обработки данных с целью повышения их качества
Смотрите также
химия
простое вещество
![''Iris'' flower data set]] introduced by [[Ronald Fisher]] (1936).<ref name="fisher36"/>](https://commons.wikimedia.org/wiki/Special:FilePath/Iris dataset scatterplot.svg?width=200 "''Iris'' flower data set]] introduced by [[Ronald Fisher]] (1936).<ref name=\"fisher36\"/>")
математика
набор данных
Определение
Википедия
In metadata, the term data element is an atomic unit of data that has precise meaning or precise semantics. A data element has:
- An identification such as a data element name
- A clear data element definition
- One or more representation terms
- Optional enumerated values Code (metadata)
- A list of synonyms to data elements in other metadata registries Synonym ring
Data elements usage can be discovered by inspection of software applications or application data files through a process of manual or automated Application Discovery and Understanding. Once data elements are discovered they can be registered in a metadata registry.
In telecommunication, the term data element has the following components:
- A named unit of data that, in some contexts, is considered indivisible and in other contexts may consist of data items.
- A named identifier of each of the entities and their attributes that are represented in a database.
- A basic unit of information built on standard structures having a unique meaning and distinct units or values.
- In electronic record-keeping, a combination of characters or bytes referring to one separate item of information, such as name, address, or age.
In the areas of databases and data systems more generally a data element is a concept forming part of a data model. As an element of data representation, a collection of data elements forms a data structure.
