Results 181 to 190 of about 1,984,073 (216)

Group Formation on a Line

Symposium i Anvendt Statistik, 2010
Artiklen viser at en nummerering af indsamlede evalueringsskemaer kan afsløre gruppedannelse blandt de tilhørende studenter på et stort undervisningshold.Gruppedannelsen viser sig ved at sequenser med ens bedømmelse afviger fra en tilfældig fordeling defineret som en negativ binomialfordeling, der løber indtil to "succeer" er opnået.
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Line formation in magnetic fields

Solar Physics, 1970
Hyder (1968) has suggested that longitudinal magnetograph measurements of weak magnetic fields in prominences have underestimated field strengths as the result of zero-field levelcrossing interference (the Hanle effect). Hyder (1968) also suggested that resonance polarization effects have sometimes led to errors in measurements of the transverse ...
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Line Formation in Expanding Atmospheres

1976
The current state of understanding of line formation processes in expanding atmospheres is reviewed, and the successes and limitations of current computational techniques are summarized. Some results for differential rotation are also given, although very little work has been done in this area. Special attention is given to the severe difficulties that
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A Survey of Autonomous Underwater Vehicle Formation: Performance, Formation Control, and Communication Capability

IEEE Communications Surveys and Tutorials, 2021
Yang Xiao, Tieshan Li, Yue Yang
exaly  

Line format and program structure

1994
A CNC program is a set of instructions that is read by the machine tool computer system to control machine slide movements, tool movements and additional miscellaneous functions. There are two types of CNC programming: conversational format and word address format.
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Line Formation in Turbulent Media

1975
Since 1934, when Struve and Elvey introduced the concept of microturbulence for spectral line broadening in addition to pressure and thermal Doppler broadening, this mechanism has frequently been used in the analysis of stellar spectra. According to the discussions in standard textbooks on stellar spectra the effect of microturbulence is due to an ...
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Formation of FEII Lines in AGN

1988
Up to now photoionization models of the Broad Line Region of quasars fail to explain the strength of low ionization lines, in particular, FeII lines are too weak compared to H3. Using a code mainly designed to study low ionized and optically thick medium, I have calculated the radiation transfer in a non-photoionized homogeneous cloud in order to ...
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On the Formation of Squall Lines

Bulletin of the American Meteorological Society, 1952
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Cosmic Star-Formation History

Annual Review of Astronomy and Astrophysics, 2014
Mark Dickinson, Piero Madau
exaly  

Astrochemistry During the Formation of Stars

Annual Review of Astronomy and Astrophysics, 2020
Robin Garrod, Jes KRISTIAN Jørgensen, Arnaud Belloche   +2 more
exaly