A linear magnetic field scan driver

Reconstruction of Solar Coronal Linear Force-Free Magnetic Field

Results of the Ulysses Fast Latitude Scan: Magnetic Field Observations

The rapid crossing of the solar equatorial region by Ulysses as it returned from the south pole resulted in 7 crossings of the heliospheric current sheet between 10“S and 20”N and 10 distinct solar wind interaction regions between 18“S and 22”N. Both the extent of the current sheet and the latitude interval containing the interaction regions are a f~ctor of= 2 less than were observed by Ulysses...

reconstruction of solar coronal linear force-free magnetic field

Simple limits on achieving a quasi-linear magnetic compression for an FEL driver

Free electron lasers (FEL) need a very bright electron beam in three dimensions and a high peak charge density. In order to compress an initially longer electron bunch generated from the photoinjector, magnetic bunch compression systems are widely employed. In this paper, first harmonic RF linearization and its associated requirements are reviewed. Meanwhile it is also briefly discussed what is...

Scan Light Field Rendering

In this paper we present a new variant of the light field representation that supports improved image reconstruction by accommodating sparse correspondence information. This places our representation somewhere between a pure, two-plane parameterized, light field and a lumigraph representation, with its continuous geometric proxy. Our approach factors the rays of a light field into one of two se...