Zobrazeno 1 - 10
of 390
pro vyhledávání: '"R. H. Miller"'
Autor:
D. R. Serwanski, Richard Milner, Craig S. Moore, R. H. Miller, Stephen J. Crocker, Akiko Nishiyama, J. L. Whitton, R. R. Pagarigan, Ricardo F. Frausto
Publikováno v:
The Journal of Neuroscience. 31:6247-6254
Tissue inhibitor of metalloproteinase-1 (TIMP-1) is an extracellular protein and endogenous regulator of matrix metalloproteinases (MMPs) secreted by astrocytes in response to CNS myelin injury. We have previously reported that adult TIMP-1 knock-out
Publikováno v:
Zeitschrift für Tierzüchtung und Züchtungsbiologie. 98:108-124
Autor:
R. H. Miller
Publikováno v:
Sign Language Studies. 7:225-232
Out of this silence yet I picked a welcome, And in the modesty of fearful duty I read as much as from the rattling tongue Of saucy and audacious eloquence. A Midsummer Night's Dream, 5.1.100-103 IN THIS FAMOUS PASSAGE Theseus, the king of Athens, tel
Publikováno v:
Organic Farming
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::aaef913864de446a709b5ce12b387e8d
https://doi.org/10.2134/asaspecpub46.c7
https://doi.org/10.2134/asaspecpub46.c7
Publikováno v:
Sulfur in Agriculture
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a66ccfacd2beca570af6b3603a3df731
https://doi.org/10.2134/agronmonogr27.c2
https://doi.org/10.2134/agronmonogr27.c2
Autor:
R. H. Miller
Publikováno v:
Space Science Reviews. 102:115-120
We inquire whether some important features might be lost in studying the gravitational n-body problem because chaos makes it impossible to follow exact phase trajectories. We test this by comparing deliberately crude ‘integrations’ with published
Autor:
R. H. Miller
Publikováno v:
High Gradient Accelerating Structure.
Autor:
R. H. Miller
Publikováno v:
Renascence. 51:133-143
Autor:
R. H. Miller
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 73:139-147
The gravitational n—body problem is chaotic. Phase trajectories that start very near each other separate rapidly. The rate looks exponential over long times. At any instant, trajectories separated in certain directions move apart rapidly (unstable