MIRA has a long and established history of vehicle test and development, especially within the fields of vehicle ride, handling, NVH and durability. With the move towards zero prototype engineering, fewer vehicles are available for development and greater emphasis is placed on conducting more accurate analysis upfront at the concept and design stages. MIRA has embraced this shift, by integratin...

Mira is an iPad app for mirroring Max patchers in real time with minimal configuration. The Mira iPad app discovers open Max patchers automatically using the Bonjour protocol, connects to them over WiFi and negotiates a description of the Max patcher. As objects change position and appearance, Mira makes sure that the interface on the iPad stays up to date. Mira eliminates the need for an expli...

2 Bart Krekelberg and Richard J.A. van Wezel 3 4 Center for Molecular and Behavioral Neuroscience, Rutgers University, Newark, New Jersey 5 Biomedical Signals and Systems, MIRA, Twente University, 6 Enschede, The Netherlands 7 Department of Biophysics, Donders Institute for Brain, Cognition and Behaviour, 8 Radboud University, Nijmegen, The Netherlands 9 10 11 Figures: 8 12 Pages: 40 13 Running...

In this review we rst describe basic information for carbon stars starting with the most recent spectral classi cation system of P.C. Keenan and luminosities derived from data in the Hipparcos Catalogue. For the SRb and Lb variables MK = 6:8 1:2 (21 stars). Only two R stars (non-variables) have measured K magnitudes and showMK = 5:2. The four N stars show MV = +0:76 1:06. Using the Magellanic C...

Summary DNA methylation contains information about the regulatory state of the cell. MIRA aggregates genome-scale DNA methylation data into a DNA methylation profile for independent region sets with shared biological annotation. Using this profile, MIRA infers and scores the collective regulatory activity for each region set. MIRA facilitates regulatory analysis in situations where classical re...

RENATO COLUCCI, JORGE MIRA, JUAN J. NIETO, AND M. VICTORIA OTERO-ESPINAR Department of Mathematical Sciences, Xi’an Jiatong-Liverpool University, Suzhou, China; Departamento de F ısica Aplicada, Universidade de Santiago de Compostela, 15782 Santiago de Compostela, Spain; Departamento de An alise Matem atica, Instituto de Matem aticas, Universidade de Santiago de Compostela, 15782, Santiago de C...

Through polarization observations, circumstellar masers are excellent probes of the magnetic field in the envelopes of late-type stars. Whereas observations of the polarization of the SiO masers close to the star and on the OH masers much further out were fairly commonplace, observations of the magnetic field strength in the intermediate density and temperature region where the 22 GHz H 2 O mas...

We present an analysis of AAVSO visual observations of the Mira variable R Cen from 1918 to 2000. The period of the dominant mode has been steadily decreasing from 550 days at JD 2,434,000 (1951) to its present value of 505–510 days. In the same interval, the pulsational amplitude has decreased by 3 mag, from 5.5–11.8 V to 6.3–9.1 V. We suggest that both are caused by a He-shell flash, as the p...