A Canvas for Establishing Global Software Development Collaborations

Jufo-id:80620There is an increasing need and interest for organizations to collaborate with internal and external partners on a global scale for creating software-based products and services. Potential risks and different strategies need to be addressed when setting up such collaborations. Aspects such as cultural and social features, coordination, infrastructure, organizational change processes, or communication issues need to be con- sidered. Although there are already experiences available with respect to setting up global collaborations, they mainly focus on specific areas. It is dicult for companies to quickly assess if they have considered all rele- vant aspects. An overall aid that guides companies in systematically setting up global collaborations is widely missing. In this paper we present a study based on the snowballing method as a systematic approach to literature review. Based on this literature review and inputs from indus- try we investigated what aspects and practices need to be considered when establishing global software development collaborations and how to prioritize them. Based on that we created activity roadmaps that aggregate existing experiences. Reported experiences were structured into nine main aspects each containing extracted successful practices for set- ting up global software development collaborations. As a result we came up with an initial version of a canvas that is proposed as guidance for companies for setting up global collaborations in the software development domain.Peer reviewe

Eclipses observed by LYRA - a sensitive tool to test the models for the solar irradiance

We analyze the light curves of the recent solar eclipses measured by the Herzberg channel (200-220 nm) of the Large Yield RAdiometer (LYRA) onboard PROBA-2. The measurements allow us to accurately retrieve the center- to-limb variations (CLV) of the solar brightness. The formation height of the radiation depends on the observing angle so the examination of the CLV provide information about a broad range of heights in the solar atmosphere. We employ the 1D NLTE radiative transfer COde for Solar Irradiance (COSI) to model the measured light curves and corresponding CLV dependencies. The modeling is used to test and constrain the existing 1D models of the solar atmosphere, e.g. the temperature structure of the photosphere and the treatment of the pseudo- continuum opacities in the Herzberg continuum range. We show that COSI can accurately reproduce not only the irradiance from the entire solar disk, but also the measured CLV. It hence can be used as a reliable tool for modeling the variability of the spectral solar irradiance.Comment: 19 pages, 9 figures, Solar Physic

The Role of Background Cloud Microphysics in the Radiative Formation of Ship Tracks

The authors investigate the extent to which the contrast brightness of ship tracks, that is, the relative change in observed solar reflectance, in visible and near-infrared imagery can be explained by the microphysics of the background cloud in which they form. The sensitivity of visible and near-infrared wavelengths for detecting reflectance changes in ship tracks is discussed, including the use of a modified cloud susceptibility parameter, termed the ‘‘contrast susceptibility,’’ for assessing the sensitivity of background cloud microphysics on potential track development. It is shown that the relative change in cloud reflectance for ship tracks is expected to be larger in the near-infrared than in the visible and that 3.7-mm channels, widely known to be useful for detecting tracks, have the greatest sensitivity. The usefulness of contrast susceptibility as a predictor of ship track contrast is tested with airborne and satellite remote sensing retrievals of background cloud parameters and track contrast. Retrievals are made with the high spatial resolution Moderate Resolution Imaging Spectroradiometer Airborne Simulator flown on the National Aeronautics and Space Administration’s high-altitude ER-2 aircraft, and with the larger-scale perspective of the advanced very high resolution radiometer. Observed modifications in cloud droplet effective radius, optical thickness, liquid water path, contrast susceptibility, and reflectance contrast are presented for several ship tracks formed in background clouds with both small and large droplet sizes. The remote sensing results are augmented with in situ measurements of cloud microphysics that provide data at the smaller spatial scales