To send content items to your account,
please confirm that you agree to abide by our usage policies.
If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account.
Find out more about sending content to .
To send content items to your Kindle, first ensure firstname.lastname@example.org
is added to your Approved Personal Document E-mail List under your Personal Document Settings
on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part
of your Kindle email address below.
Find out more about sending to your Kindle.
Note you can select to send to either the @free.kindle.com or @kindle.com variations.
‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi.
‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
This book chapter compares civil litigation in the courts of first and second instances in Taiwan in 2010–2015 with that in U.S. federal courts in 2010–2013. The two judicial systems, as expected, are different in many ways. Settlement rates in Taiwan, even broadly defined, were below 25%; in U.S. federal court, they exceed 70%. In Taiwan, summary judgments were basically non-existent; in U.S. federal court, they represent nearly a third of merits judgments. Rates of appeal in Taiwan are nearly 10 times higher (27% versus 3%) than in the U.S. federal courts. And yet judges in Taiwan, at least those in the court of first instance, handled cases more quickly than their colleagues in the U.S. federal courts—indeed, twice as fast. Yet, the two judicial systems respond similarly when encountering simple debt collection cases. These cases, large in number in both systems, fail to settle as standard theories would predict. Instead, these disputes are frequently resolved through default judgments. This chapter provides cautionary lessons for future empirical comparative civil procedure studies.
The Indian Supreme Court has been called “the most powerful court in the world” for its wide jurisdiction, its expansive understanding of its own powers, and the billion plus people under its authority. Yet scholars and policy makers have a very uneven picture of the court’s functioning: deep knowledge about the more visible, “high-profile” cases but very little about more mundane, but far more numerous and potentially equally important, decisions. This chapter aims to address this imbalance with a rigorous, empirical account of the Court’s decisions from 2010 to 2015. We use the most extensive original dataset of Indian Supreme Court opinions yet created to provide a broad, quantitative overview of the social identity of the litigants that approach the court, the types of matters they bring to the court, the levels of success that different groups of litigants have before the Court, and the opinion-writing patterns of the various judges of the Supreme Court. This analysis provides foundational facts for the study of the Court and its role in progressive social change.
A simple single-crystal goniostat has been built for the Norelco X-ray diffractometer using a modified eucentric goniometer head and the basic geometry of the Norelco pole-figure device.
The goniometer head was modified to provide interchangeable mounting tn the goniostat, a two-circle optical goniometer, or the sample holder of a flat-plate camera.
With this device one can orient and mount a. crystal along any desired direction in a fraction of the time required by conventional film techniques, thus reducing the mounting of a sample for intensity measure ment s for structure determinations or for measurements of anisotropic physical properties to a routine procedure.
We review our current understanding of the interior structure and thermal evolution of Saturn, with a focus on recent results in the Cassini era. There has been important progress in understanding physical inputs, including equations of state of planetary materials and their mixtures, physical parameters like the gravity field and rotation rate, and constraints on Saturnian free oscillations. At the same time, new methods of calculation, including work on the gravity field of rotating fluid bodies, and the role of interior composition gradients, should help to better constrain the state of Saturn’s interior, now and earlier in its history. However, a better appreciation of modeling uncertainties and degeneracies, along with a greater exploration of modeling phase space, still leave great uncertainties in our understanding of Saturn’s interior. Further analysis of Cassini data sets, as well as precise gravity field measurements from the Cassini Grand Finale orbits, will further revolutionize our understanding of Saturn’s interior over the next few years.