. . "The Gaisser\u2013Hillas function is used in astroparticle physics. It parameterizes the longitudinal particle density in a cosmic ray air shower. The function was proposed in 1977 by and . The number of particles as a function of traversed atmospheric depth is expressed as where is maximum number of particles observed at depth , and and are primary mass and energy dependent parameters. Using substitutions , and the function can be written in an alternative one-parametric (m) form as"@en . "\u064A\u0633\u062A\u062E\u062F\u0645 \u0627\u0642\u062A\u0631\u0627\u0646 \u062C\u0627\u064A\u0633\u0631-\u0647\u064A\u0644\u0627\u0633 \u0641\u064A \u0641\u064A\u0632\u064A\u0627\u0621 \u0627\u0644\u062C\u0633\u064A\u0645\u0627\u062A \u0627\u0644\u0641\u0644\u0643\u064A\u0629 \u0644\u062A\u062D\u062F\u064A\u062F \u0627\u0644\u0643\u062B\u0627\u0641\u0629 \u0627\u0644\u0637\u0648\u0644\u064A\u0629 \u0644\u0644\u062C\u0632\u064A\u0626\u0627\u062A \u0641\u064A \u0648\u0627\u0628\u0644 \u0627\u0644\u0627\u0634\u0639\u0629 \u0627\u0644\u0643\u0648\u0646\u064A\u0629. \u062A\u0645 \u0627\u0642\u062A\u0631\u0627\u062D \u0627\u0644\u0627\u0642\u062A\u0631\u0627\u0646 \u0641\u064A \u0639\u0627\u0645 1977 \u0645\u0646 \u0642\u0628\u0644 \u062A\u0648\u0645\u0627\u0633 \u0643. \u062C\u0627\u064A\u0633\u0631 \u0648\u0623\u0646\u062A\u0648\u0646\u064A \u0645\u0627\u064A\u0643\u0644 \u0647\u064A\u0644\u0627\u0633. \u064A\u062A\u0645 \u0627\u0644\u062A\u0639\u0628\u064A\u0631 \u0639\u0646 \u0639\u062F\u062F \u0627\u0644\u062C\u0632\u064A\u0626\u0627\u062A \u0628\u062F\u0644\u0627\u0644\u0629 \u0639\u0645\u0642 \u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0627\u0644\u0630\u064A \u062A\u0645 \u0627\u062C\u062A\u064A\u0627\u0632\u0647 \u0643\u0627\u0644\u062A\u0627\u0644\u064A: \u062D\u064A\u062B \u0647\u0648 \u0627\u0644\u0639\u062F\u062F \u0627\u0644\u0623\u0642\u0635\u0649 \u0644\u0644\u062C\u0632\u064A\u0626\u0627\u062A \u0627\u0644\u0645\u0648\u062C\u0648\u062F\u0629 \u0639\u0646\u062F \u0627\u0644\u0639\u0645\u0642 \u060C \u0648 \u0648 \u0647\u0645\u0627 \u0645\u0639\u0644\u0645\u062A\u0627\u0646 \u0623\u0633\u0627\u0633\u064A\u062A\u0627\u0646 \u062A\u0639\u062A\u0645\u062F\u0627\u0646 \u0639\u0644\u0649 \u0627\u0644\u0643\u062A\u0644\u0629 \u0648\u0627\u0644\u0637\u0627\u0642\u0629. \u0628\u0627\u0633\u062A\u062E\u062F\u0627\u0645 \u0627\u0644\u062A\u0639\u0648\u064A\u0636: \u0648 \u0648 \u064A\u0645\u0643\u0646 \u0643\u062A\u0627\u0628\u0629 \u0627\u0644\u0627\u0642\u062A\u0631\u0627\u0646 \u0628\u0635\u064A\u063A\u0629 \u0628\u062F\u064A\u0644\u0629 \u0623\u062D\u0627\u062F\u064A\u0629 \u0627\u0644\u0639\u0627\u0645\u0644 \u0643\u0627\u0644\u062A\u0627\u0644\u064A: ."@ar . "Fungsi Gaisser\u2014Hillas"@in . . "Fungsi Gaisser\u2013Hillas digunakan dalam . Fungsi Gaisser-Hillas memparameterkan kepadatan partikel longitudinal dalam pancaran sinar kosmis. Fungsi ini diusulkan pada tahun 1977 oleh Thomas K. Gaisser dan Anthony M. Hillas. Jumlah partikel sebagai fungsi melintasi kedalaman atmosfer dinyatakan sebagai: dimana adalah jumlah maksimum partikel teramati pada kedalaman , dan dan adalah massa primer dan energi yang tergantung parameter. Menggunakan subtitusi, dan fungsi tersebut dapat ditulis dalam bentuk alternatif satu-parametrik (m) sebagai"@in . . . . . . . "Gaisser\u2013Hillas function"@en . . . . . "\u0627\u0642\u062A\u0631\u0627\u0646 \u062C\u0627\u064A\u0633\u0631-\u0647\u064A\u0644\u0627\u0633"@ar . . . . "1098772612"^^ . . . . "\u064A\u0633\u062A\u062E\u062F\u0645 \u0627\u0642\u062A\u0631\u0627\u0646 \u062C\u0627\u064A\u0633\u0631-\u0647\u064A\u0644\u0627\u0633 \u0641\u064A \u0641\u064A\u0632\u064A\u0627\u0621 \u0627\u0644\u062C\u0633\u064A\u0645\u0627\u062A \u0627\u0644\u0641\u0644\u0643\u064A\u0629 \u0644\u062A\u062D\u062F\u064A\u062F \u0627\u0644\u0643\u062B\u0627\u0641\u0629 \u0627\u0644\u0637\u0648\u0644\u064A\u0629 \u0644\u0644\u062C\u0632\u064A\u0626\u0627\u062A \u0641\u064A \u0648\u0627\u0628\u0644 \u0627\u0644\u0627\u0634\u0639\u0629 \u0627\u0644\u0643\u0648\u0646\u064A\u0629. \u062A\u0645 \u0627\u0642\u062A\u0631\u0627\u062D \u0627\u0644\u0627\u0642\u062A\u0631\u0627\u0646 \u0641\u064A \u0639\u0627\u0645 1977 \u0645\u0646 \u0642\u0628\u0644 \u062A\u0648\u0645\u0627\u0633 \u0643. \u062C\u0627\u064A\u0633\u0631 \u0648\u0623\u0646\u062A\u0648\u0646\u064A \u0645\u0627\u064A\u0643\u0644 \u0647\u064A\u0644\u0627\u0633. \u064A\u062A\u0645 \u0627\u0644\u062A\u0639\u0628\u064A\u0631 \u0639\u0646 \u0639\u062F\u062F \u0627\u0644\u062C\u0632\u064A\u0626\u0627\u062A \u0628\u062F\u0644\u0627\u0644\u0629 \u0639\u0645\u0642 \u0627\u0644\u063A\u0644\u0627\u0641 \u0627\u0644\u062C\u0648\u064A \u0627\u0644\u0630\u064A \u062A\u0645 \u0627\u062C\u062A\u064A\u0627\u0632\u0647 \u0643\u0627\u0644\u062A\u0627\u0644\u064A: \u062D\u064A\u062B \u0647\u0648 \u0627\u0644\u0639\u062F\u062F \u0627\u0644\u0623\u0642\u0635\u0649 \u0644\u0644\u062C\u0632\u064A\u0626\u0627\u062A \u0627\u0644\u0645\u0648\u062C\u0648\u062F\u0629 \u0639\u0646\u062F \u0627\u0644\u0639\u0645\u0642 \u060C \u0648 \u0648 \u0647\u0645\u0627 \u0645\u0639\u0644\u0645\u062A\u0627\u0646 \u0623\u0633\u0627\u0633\u064A\u062A\u0627\u0646 \u062A\u0639\u062A\u0645\u062F\u0627\u0646 \u0639\u0644\u0649 \u0627\u0644\u0643\u062A\u0644\u0629 \u0648\u0627\u0644\u0637\u0627\u0642\u0629. \u0628\u0627\u0633\u062A\u062E\u062F\u0627\u0645 \u0627\u0644\u062A\u0639\u0648\u064A\u0636: \u0648 \u0648 \u064A\u0645\u0643\u0646 \u0643\u062A\u0627\u0628\u0629 \u0627\u0644\u0627\u0642\u062A\u0631\u0627\u0646 \u0628\u0635\u064A\u063A\u0629 \u0628\u062F\u064A\u0644\u0629 \u0623\u062D\u0627\u062F\u064A\u0629 \u0627\u0644\u0639\u0627\u0645\u0644 \u0643\u0627\u0644\u062A\u0627\u0644\u064A: ."@ar . . . "2320"^^ . . . . . . . . . . "Fungsi Gaisser\u2013Hillas digunakan dalam . Fungsi Gaisser-Hillas memparameterkan kepadatan partikel longitudinal dalam pancaran sinar kosmis. Fungsi ini diusulkan pada tahun 1977 oleh Thomas K. Gaisser dan Anthony M. Hillas. Jumlah partikel sebagai fungsi melintasi kedalaman atmosfer dinyatakan sebagai: dimana adalah jumlah maksimum partikel teramati pada kedalaman , dan dan adalah massa primer dan energi yang tergantung parameter. Menggunakan subtitusi, dan fungsi tersebut dapat ditulis dalam bentuk alternatif satu-parametrik (m) sebagai"@in . . "10196392"^^ . . "The Gaisser\u2013Hillas function is used in astroparticle physics. It parameterizes the longitudinal particle density in a cosmic ray air shower. The function was proposed in 1977 by and . The number of particles as a function of traversed atmospheric depth is expressed as where is maximum number of particles observed at depth , and and are primary mass and energy dependent parameters. Using substitutions , and the function can be written in an alternative one-parametric (m) form as"@en . .