Spenser and the Historical Revolution: Briton Moniments and the Problem of Roman Britain

Curran argues that, since Roman Britain is a key to understanding the historiographical debates of Edmund Spenser\u27s time, the Roman Britain section of Briton Moniments in The Faerie Queene needs to be examined. It is here that Spenser acknowledged the direction historiography was taking, and saw how this new trend altered the relation between history and glory

Statistical view of legal and capital markets determinants

Thesis (S.M.)--Massachusetts Institute of Technology, Sloan School of Management, 2010.Cataloged from PDF version of thesis.Includes bibliographical references.Prior authors have concluded that case-specific determinants, such as the number of professionals involved in a given case or the lead attorney's hourly rate, are the principal determinants of variance in professional fees and expenses in US corporate restructurings. The implication has been that less proximate variables, such as the availability of credit, the cost of capital or coincident economic conditions, are not relevant to predictive models. While we do not question the relevance of case-specific factors we question the practicality of models that rely exclusively on such factors in order to predict future fees and expenses. Our hypothesis is that both case-specific and less proximate variables are relevant to the determination of professional costs in bankruptcy, since we believe that variables belonging to each of these categories can act as frictions to the refinancing process or otherwise inform the court's determination as to the efficacy of refinancing, thereby impacting the complexity and duration of the restructuring process. Our results are less than conclusive, since our data is limited. However, the data that we have gives us reason to believe that the addition of non-case predictors may improve the accuracy of case-specific models; in some instances, these non-case-specific predictors even displace case specific predictors (via a screen for statistical significance). Our analysis indicates that this improvement is more pronounced when the data is sorted for Section 364 financing. Our goal is to complement the on-going analysis of professional fees and expenses so that it might better account for the potential impact of non-case factors and thereby yield a more accurate and practical predictive model.by John P. Curran, Jr.S.M

The role of proton precipitation in Jovian aurora: Theory and observation

It was proposed that the Jovian auroral emissions observed by Voyager spacecraft could be explained by energetic protons precipitating into the upper atmosphere of Jupiter. Such precipitation of energetic protons results in Doppler-shifted Lyman alpha emission that can be quantitatively analyzed to determine the energy flux and energy distribution of the incoming particle beam. Modeling of the expected emission from a reasonably chosen Voyager energetic proton spectrum can be used in conjunction with International Ultraviolet Explorer (IUE) observations, which show a relative lack of red-shifted Lyman alpha emission, to set upper limits on the amount of proton precipitation taking place in the Jovian aurora. Such calculations indicate that less than 10 percent of the ultraviolet auroral emissions at Jupiter can be explained by proton precipitation

Comment on "low time resolution analysis of polar ice cores cannot detect impulsive nitrate events" by D.F. Smart et al.

AbstractSmart et al. (2014) suggested that the detection of nitrate spikes in polar ice cores from solar energetic particle (SEP) events could be achieved if an analytical system with sufficiently high resolution was used. Here we show that the spikes they associate with SEP events are not reliably recorded in cores from the same location, even when the resolution is clearly adequate. We explain the processes that limit the effective resolution of ice cores. Liquid conductivity data suggest that the observed spikes are associated with sodium or another nonacidic cation, making it likely that they result from deposition of sea salt or similar aerosol that has scavenged nitrate, rather than from a primary input of nitrate in the troposphere. We consider that there is no evidence at present to support the identification of any spikes in nitrate as representing SEP events. Although such events undoubtedly create nitrate in the atmosphere, we see no plausible route to using nitrate spikes to document the statistics of such events.EW is supported by a Royal Society Professorship.This is the author accepted manuscript. The final version is available from Wiley via http://dx.doi.org/10.1002/2015JA02157

Comment on "low time resolution analysis of polar ice cores cannot detect impulsive nitrate events" by D.F. Smart et al.

Smart et al. (2014) suggested that the detection of nitrate spikes in polar ice cores from solar energetic particle (SEP) events could be achieved if an analytical system with sufficiently high resolution was used. Here we show that the spikes they associate with SEP events are not reliably recorded in cores from the same location, even when the resolution is clearly adequate. We explain the processes that limit the effective resolution of ice cores. Liquid conductivity data suggests that the observed spikes are associated with sodium or another non-acidic cation, making it likely that they result from deposition of sea salt or similar aerosol that has scavenged nitrate, rather than from a primary input of nitrate in the troposphere. We consider that there is no evidence at present to support the identification of any spikes in nitrate as representing SEP events. Although such events undoubtedly create nitrate in the atmosphere, we see no plausible route to using nitrate spikes to document the statistics of such events.EW is supported by a Royal Society Professorship.This is the author accepted manuscript. The final version is available from Wiley via http://dx.doi.org/10.1002/2015JA02157

A 700 year record of Southern Hemisphere extratropical climate variability

Annually dated ice cores from West and East Antarctica provide proxies for past changes in atmospheric circulation over Antarctica and portions of the Southern Ocean, temperature in coastal West and East Antarctica, and the frequency of South Polar penetration of El Niño events. During the period AD 1700–1850, atmospheric circulation over the Antarctic and at least portions of the Southern Hemisphere underwent a mode switch departing from the out-of-phase alternation of multi-decadal long phases of EOF1 and EOF2 modes of the 850 hPa field over the Southern Hemisphere (as defined in the recent record by Thompson and Wallace, 2000; Thompson and Solomon, 2002) that characterizes the remainder of the 700 year long record. From AD 1700 to 1850, lower-tropospheric circulation was replaced by in-phase behavior of the Amundsen Sea Low component of EOF2 and the East Antarctic High component of EOF1. During the first phase of the mode switch, both West and East Antarctic temperatures declined, potentially in response to the increased extent of sea ice surrounding both regions. At the end of the mode switch, West Antarctic coastal temperatures rose and East Antarctic coastal temperatures fell, respectively, to their second highest and lowest of the record. Polar penetration of El Niño events increased during the mode switch. The onset of the AD 1700–1850 mode switch coincides with the extreme state of the Maunder Minimum in solar variability. Late 20th-century West Antarctic coastal temperatures are the highest in the record period, and East Antarctic coastal temperatures close to the lowest. Since AD 1700, extratropical regions of the Southern Hemisphere have experienced significant climate variability coincident with changes in both solar variability and greenhouse gase

Comment on "low time resolution analysis of polar ice cores cannot detect impulsive nitrate events" by D.F. Smart et al.

Smart et al. (2014) suggested that the detection of nitrate spikes in polar ice cores from solar energetic particle (SEP) events could be achieved if an analytical system with sufficiently high resolution was used. Here we show that the spikes they associate with SEP events are not reliably recorded in cores from the same location, even when the resolution is clearly adequate. We explain the processes that limit the effective resolution of ice cores. Liquid conductivity data suggests that the observed spikes are associated with sodium or another non-acidic cation, making it likely that they result from deposition of sea salt or similar aerosol that has scavenged nitrate, rather than from a primary input of nitrate in the troposphere. We consider that there is no evidence at present to support the identification of any spikes in nitrate as representing SEP events. Although such events undoubtedly create nitrate in the atmosphere, we see no plausible route to using nitrate spikes to document the statistics of such events.EW is supported by a Royal Society Professorship.This is the author accepted manuscript. The final version is available from Wiley via http://dx.doi.org/10.1002/2015JA02157