Magnetic Resonance Microscopy. Группа авторов

Magnetic Resonance Microscopy - Группа авторов


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(MRM) has focused on magnetic resonance imaging (MRI) applied to objects of smaller scale and higher spatial resolution for more than three decades. After the pioneering work by Eccles, Callaghan, Aguayo, Blackband, Johnson et al. in 1986, MRM quickly spread to, among other fields, chemistry, histology, and materials research. Since 1992, the edited book series Magnetic Resonance Microscopy has provided an important voice describing the latest developments in spatially resolved magnetic resonance methods and their applications far beyond the scope of medical diagnostics. An excellent introduction to MRM, focusing on the practical aspects of high magnetic fields and on the study of biological systems, was authored in 2017 by Luisa Ciobanu: Microscopic Magnetic Resonance Imaging: A Practical Perspective (Pan Stanford, Singapore, 2017). Our book complements this monograph by showing the use of MRM and related techniques in a much broader area and on a wider scale, which extends from chemical engineering to plant research and battery applications, highlighting the interdisciplinary nature of MRM.

      The book opens with a section on hardware and methodology, covering aspects of micro-engineering, magnet technology, coil performance, and hyperpolarization to improve signal-to-noise ratio, a major bottleneck of MRM. Specific pulse sequences and developments in the field of mobile nuclear magnetic resonance are further topics of this first chapter. The following parts, 2 and 3, review essential processes such as filtration, multi-phase flows and transport, and a wide range of systems from biomarkers via single cells to plants and biofilms. Part 4 focuses on energy research, which is becoming increasingly important due to the globally growing environmental problems. It reports on battery types and their developments and how battery states can be recorded and characterized with MRM. However, we would like to point out to the reader that only a small sample of applications could be addressed in Chapters 1 to 4. Finally, the last chapter advocates that theory and applications should not be treated separately, because much can be gained from their complementarity.

      The editors thank all the authors for contributing their invaluable knowledge to this book during a time challenged by COVID-19. Our thanks also go to the kind staff of the Wiley books department, who helped us with advice and support throughout the whole editing process.

      Sabina Haber-Pohlmeier

      Luisa Ciobanu

      Bernhard Blümich

      Summer 2021

Part I Developments in Hardware and Methods

       Neil MacKinnon, Jan G. Korvink, and Mazin Jouda

       Institute of Microstructure Technology, Karlsruhe Institute of Technology, Eggenstein-Leopoldshafen, Germany

      1.1 Introduction

      1.1.1 Comparative Electromagnetic Radiation Imaging

      Paul Callaghan’s book [1] is perhaps the first publication to consider magnetic resonance imaging (MRI) in the same light as optical microscopy. This will also be our starting point.

      Until the advent of super-resolution microscopy, refractive optical microscopy was essentially a radiation scattering method, in which a beam of photons from an independent light source was sent on its way to scatter off objects, followed by traversal of the beam through a focusing objective on its way back to a detector, to thereby reveal the structure and composition of the scattering object. The limitations of this approach, in terms of resolution, is known as the Abbe limit δ = λ/(2 n sin θ), where n is the refractive index, θ the half-angle of the spot subtended by the lens, and λ the radiation wavelength.

      Interestingly, deep space astronomy always worked this way around by observing photon emitters, so that astronomers only consider objects that were once themselves sources of radiation, such as stars and their predecessors and descendants. In astronomy, the limit of resolution is therefore not dominated by the wavelength of the radiation, which can be very small when compared to the size and distance of the astronomical objects, but rather by the measuring instrument’s principle of operation, its detection sensitivity, and in particular, its effective aperture.

      When imaging radiation sources, such as single photon emitters in molecules, we now know that we can greatly improve on the Abbe limit, by about a factor of 10, especially when combined with techniques of stimulated emission and depletion, and one of the numerous variations based on fluorophore emission dynamics. These techniques, which have revolutionized cellular biology and won its inventor Stefan Hell the Nobel Prize in 2014, are of course not accessible to astronomers, who would have to wait too long for excitation signals to pass from observer to object and back again. But for cell biology this is not problematic. Although at currently ~30 nm, the resolution is still far from the desired 1 nm limit, advances in image processing present a feasible route to achieve further improvements. But the technique also raises some questions. Sample preparation is very difficult, and imaging is indirect as fluorophores have to be invasively attached to interesting molecules, almost certainly modifying their behavior.


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