The Vasa's New Battle

Methods

To analyse the samples several x-ray based methods, XANES, ESCA and powder diffraction XRD, have been used. The methods differ in the effects measured.

The different methods Explenation of esca
(right) X-ray analytical methods used in these investigations are XANES, ESCA and x-ray powder diffraction XRD. (left) Scheme of electronic energy levels in an atom. The bound electron, e.g. an 1s electron in the sulfur K-shell, absorbs x-ray radiation (hν) and is ejected as a photoelectron. ESCA: the energy of the photoelectron is measured and gives the bonding energy of the electrons in the element.  XANES: The empty "hole" created in the energy level A is filled very rapidly and fluorescence x-ray radiation is emitted and detected to measure the x-ray absorption.

XANES

When the X-ray energy is varied the absorption of the X-rays can increase sharply when a core electron in the K-shell of the sulfur atom is excited to an unoccupied molecular orbital. This is called X-ray Absorption Near Edge Structure (XANES) spectroscopy, The energy of the absorption edge is sensitive to the sulfur oxidation state and shifts as much as 13 eV from sulfide, S(-II), to sulfate, S(VI). The shape, intensity and energy of the XANES features allow insight into the chemical state and bonding of the sulfur atom, and are used to characterize the sulfur compound.

XANES XANES
XANES
The principle of the dedicated sulfur XANES instrument at beamline 6-2, Stanford Synchrotron Radiation Laboratory (SSRL), which was used to identify sulfur compounds in core samples. The intense x-rays from the synchrotron pass through a monochromator that can vary the energy, before hitting the sample in 1 atm helium pressure. The Lytle detector measures the x-ray fluorescence
SSRL logga SSRL

ESCA

Electron Spectroscopy for Chemical Analysis (ESCA) was performed by exposing slices from various depths of a core sample to x-rays of known energy (Al Kα 1487 eV), and measure the kinetic energy of the ejected photoelectrons.from all elements in the sample. Since the kinetic energy directly depends on the binding energy of the electrons in different elements, the number of photoelectrons at different energies provide, with fair accuracy, concentrations of all elements (except hydrogen) in the sample. For sulfur, the 2p electrons were used, and 1s for boron. High vacuum is needed and volatile compounds, such as water, are pumped away. The vacuum pumping takes several hours and may affect the composition of the Vasa's core samples to some extent  (Sandström 2000a). ESCA is very surface-sensitive and since the samples are not very homogeneous, also with variation of the composition in cracks etc, or smearing of the PEG when cutting slices, may influence the results.

ESCA ESCA instrument
ESCA principles. X-rays from a rotating anode are focussed on the sample. Photoelectrons are emitted from all elements and their kinetic energy measured in a hemi-spherical analyser.

XRD (X-Ray Powder Diffraction)

X-ray powder diffraction is a useful method for identifying crystalline substances in a sample. In these investigations we have used a Guinier camera, which requires a small amount of sample.

Guiner camera

The diffracted x-rays in a Guinier camera produce sharp lines on an X-ray film, while the disordered (amorphous) substances of the wood, e.g. lignin, do not give sharp lines. A scanner is used to eliminate the background from the characteristic diffraction pattern (see below) that is obtained because of the constructive interference between waves from different planes through the crystal lattice. This pattern can be used as a fingerprint of the crystalline compound, and the identification is performed by comparing with such patterns of known standards in a data base to identify which substances that are present in a sample.

Reflection
If the distance between the atomic planes is d, the path difference between successive reflections is 2dsin(θ), where θ is the angle between the incident beam and the planes (see the figur above). For constructive interference the path difference must be an integral number of wavelengths. This gives Bragg's law for possible reflections:  2d sin(θ) = nλ .
Jarosite Jarosite pattern
 
The diffraction pattern above is from the yellow jarosite salt, NaFe3(SO4)2(OH)6, that did not dissolve when a deck plank of the Vasa was treated with DTPA, see below where Yvonne samples the plank.
Yvonne takes samples