Accounts of the English Crown with Italian merchant societies, 1272-1345

The credit arrangements between the three Edwards and Italian merchants were crucial for financing England’s ambitious foreign policies and ensuring the smooth running of governmental administration. The functioning of this credit system can be followed in detail through the well-kept but mostly unpublished records of the English Exchequer. This volume combines a transcription of the most important surviving accounts between the merchants and the Crown, with a parallel abstract presenting the core data in a double-entry format as credits to or debits from the king's account. This dual format was chosen to facilitate the interpretation of the source while still retaining the language and, as far as possible, the structure of the original documents. The wealth of evidence presented here has much value to add to our understanding of the financing of medieval government and the early development of banking services provided by Italian merchant societies. In particular, although the relationship between king and banker was, for the most part, mutually profitable, the English kings also acquired a reputation for defaulting on their debts and thus 'breaking' a succession of merchant societies. These documents provide an essential basis for a re-examination of the 'credit rating' of the medieval English Crown.

A potential lag between the open solar magnetic source flux and solar EUV and X-ray emissions as measured by the Earth's ionosphere during total solar eclipses

Measurements of the ionospheric E-region during total solar eclipses have been used to provide information about the evolution of the solar magnetic field and EUV and X-ray emissions from the solar corona and chromosphere. By measuring levels of ionisation during an eclipse and comparing these measurements with an estimate of the unperturbed ionisation levels (such as those made during a control day, where available) it is possible to estimate the percentage of ionising radiation being emitted by the solar corona and chromosphere. Previously unpublished data from the two eclipses presented here are particularly valuable as they provide information that supplements the data published to date. The eclipse of 23 October 1976 over Australia provides information in a data gap that would otherwise have spanned the years 1966 to 1991. The eclipse of 4 December 2002 over Southern Africa is important as it extends the published sequence of measurements. Comparing measurements from eclipses between 1932 and 2002 with the solar magnetic source flux reveals that changes in the solar EUV and X-ray flux lag the open source flux measurements by approximately 1.5 years. We suggest that this unexpected result comes about from changes to the relative size of the limb corona between eclipses, with the lag representing the time taken to populate the coronal field with plasma hot enough to emit the EUV and X-rays ionising our atmosphere.