1. (100%) Microprobe Analysis - Andersen, C.A.
(571 p.) - 03-mar-2009

2. (100%) Qualification test report for telemetry radio frequency multiplexer, Douglas specification control number 1A69212-/GTP line item no. W19/ - Andersen, A. C.
- 05-jun-2009

3. (80%) Measurement of radium concentration in water with Mn-coated beads at the Sudbury Neutrino Observatory - Andersen, T. C.
We describe a method to measure the concentration of 224Ra and 226Ra in the heavy water target used ...
- 15-mar-2007

4. (80%) Molecular dynamics studies of heterogeneous dynamics and dynamic crossover in supercooled atomic liquids - Andersen, Hans C.
Supercooled liquids near the glass transition exhibit the phenomenon of heterogeneous relaxation; at ...
- 24-nov-2006

5. (80%) Stretching Before and After Exercise: Effect on Muscle Soreness and Injury Risk - Andersen, J. C
Reference: Herbert RD, Gabriel M. Effects of stretching before and after exercise on muscle soreness ...
- 27-nov-2006

6. (80%) Inclusion-induced bilayer deformations: effects of monolayer equilibrium curvature. - Nielsen, C; Andersen, O S
equilibrium curvature, c(0), that is different from zero. For any choice of bilayer material .... When c(0) = 0, delta G(def) can be approximated as a biquadratic function of s and the monolayer
- 29-nov-2006

7. (80%) Hemostasis and Thrombosis—Basic Principles and Clinical Practice - Andersen, Judith C.
- 30-nov-2006

8. (80%) Development and validation of a Radiance model for a translucent panel - Andersen, M.; Reinhart, C.
Abstract This study describes the development and validation of a Radiance model for a translucent p ...
- 08-jun-2007

9. (80%) Winds of M- and S-type AGB stars: an unorthodox suggestion for the driving mechanism - Hoefner, S.; Andersen, A. C.
understanding mass loss from C-rich AGB stars. For M-type objects, however, recent detailed models ... explanation for the observed similarities in wind properties of M-type and C-type AGB stars and implies
- 27-jun-2007

10. (80%) Dust from AGB stars - Andersen, Anja C.
Dust is formed in the expanding atmosphere during late stages of stellar evolution. Dust influences ...
- 27-jun-2007

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