LEADER 02406oam 2200661 450 001 9910711986503321 005 20190226164756.0 035 $a(CKB)5470000002488223 035 $a(OCoLC)784841184$z(OCoLC)760156134$z(OCoLC)786276700$z(OCoLC)988786543$z(OCoLC)1029949827$z(OCoLC)1035318008 035 $a(EXLCZ)995470000002488223 100 $a20120408d1929 ua 0 101 0 $aeng 135 $aurbn||||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aCauses of absence for men and for women in four cotton mills 210 1$a[Washington, D.C.] :$cUnited States Department of Labor, Women's Bureau. 210 2$aWashington :$cUnited States Government Printing Office,$d1929. 215 $a1 online resource (v, 24 pages) 225 1 $aBulletin of the Women's Bureau ;$vno. 69 300 $a"The investigation was made and the report written by Ethel L. Best, industrial supervisor of the Women's Bureau."--Letter of transmittal. 300 $a"Supplementary to a more extensive study previously published that showed the absence and turnover of men and women in 18 cotton mills." (Bulletin of the Women's Bureau, no. 52, 1926. Lost time and labor turnover in cotton mills). 320 $aIncludes bibliographical references. 606 $aAbsenteeism (Labor) 606 $aTextile workers$zUnited States 606 $aWomen$xEmployment$zUnited States 606 $aTextile industry$zUnited States 606 $aAbsenteeism (Labor)$2fast 606 $aTextile workers$2fast 606 $aWomen$xEmployment$2fast 607 $aUnited States$2fast 615 0$aAbsenteeism (Labor) 615 0$aTextile workers 615 0$aWomen$xEmployment 615 0$aTextile industry 615 7$aAbsenteeism (Labor) 615 7$aTextile workers. 615 7$aWomen$xEmployment. 700 $aBest$b Ethel L$g(Ethel Lombard),$01389982 712 02$aUnited States.$bWomen's Bureau, 801 0$bOCLCE 801 1$bOCLCE 801 2$bOCLCQ 801 2$bHMM 801 2$bOCLCQ 801 2$bOCLCF 801 2$bOCLCO 801 2$bOCLCQ 801 2$bOCL 801 2$bZ5A 801 2$bOCLCA 801 2$bOCL 801 2$bGPO 906 $aBOOK 912 $a9910711986503321 996 $aCauses of absence for men and for women in four cotton mills$93473368 997 $aUNINA LEADER 04220nam 22005775 450 001 9910254598003321 005 20200701082055.0 010 $a3-319-63411-9 024 7 $a10.1007/978-3-319-63411-1 035 $a(CKB)3710000001631582 035 $a(MiAaPQ)EBC4941322 035 $a(DE-He213)978-3-319-63411-1 035 $a(PPN)203851439 035 $a(EXLCZ)993710000001631582 100 $a20170808d2017 u| 0 101 0 $aeng 135 $aurcnu|||||||| 181 $2rdacontent 182 $2rdamedia 183 $2rdacarrier 200 10$aEmission of Radio Waves in Particle Showers $eValidation of Microscopic Simulations with the SLAC T-510 Experiment and their Potential in the Future Square Kilometre Array /$fby Anne Zilles 205 $a1st ed. 2017. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2017. 215 $a1 online resource (142 pages) $cillustrations 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 300 $a"Doctoral Thesis accepted by the Karlsruher Institute of Technology, Karlsruhe, Germany." 311 $a3-319-63410-0 320 $aIncludes bibliographical references at the end of each chapters and index. 327 $aIntroduction -- Cosmic Rays -- Modeling of Radio Emission from Particle\Air Showers -- Testing Predictions for Radio Emission from Particle Showers -- Modeling the Radio Emission from a Particle Shower -- Comparison of Microscopic Simulations to Data of the T-510 Experiment -- Detecting Cosmic Rays with SKA1-low -- Conclusions. 330 $aThis thesis offers the first laboratory validation of microscopic simulations of radio emission from particle showers, including a detailed description of the simulation study. It presents a potential future avenue for resolving the mass composition of cosmic rays via radio detection of air showers.  Particle showers are created from cascading interactions when high-energy particles collide with matter, e.g. with air in the case of cosmic radiation, or with a particle detector in the case of experiments at CERN. These showers can consist of billions of particles, mostly electrons, positrons and photons. They emit radio waves when the absorbing medium is in a magnetic field, and this radio emission can be used as a novel means of detecting and drawing inferences on the shower and the primary particle. The new method is currently being established in cosmic ray research, where large antenna arrays may soon replace or complement traditional particle detectors.  In thi s study, a complete microscopic simulation of a radio-emission experiment conducted at Stanford Linear Accelerator Center (SLAC), Stanford/USA, is performed, and the underlying physical models are validated. The model is subsequently applied to the Square Kilometre Array (SKA) project, which is a large interferometer for radio astronomy. It is demonstrated that the SKA, with some modifications, might also be used for cosmic ray research based on radio detection of high-energy particles from the cosmos. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aAstrophysics 606 $aPhysics 606 $aPhysical measurements 606 $aMeasurement 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aNumerical and Computational Physics, Simulation$3https://scigraph.springernature.com/ontologies/product-market-codes/P19021 606 $aMeasurement Science and Instrumentation$3https://scigraph.springernature.com/ontologies/product-market-codes/P31040 615 0$aAstrophysics. 615 0$aPhysics. 615 0$aPhysical measurements. 615 0$aMeasurement. 615 14$aAstrophysics and Astroparticles. 615 24$aNumerical and Computational Physics, Simulation. 615 24$aMeasurement Science and Instrumentation. 676 $a522.682 700 $aZilles$b Anne$4aut$4http://id.loc.gov/vocabulary/relators/aut$0819591 906 $aBOOK 912 $a9910254598003321 996 $aEmission of Radio Waves in Particle Showers$92047121 997 $aUNINA