Interdisciplinary Research of Magnetic Fields and Life Sciences

2021 ◽  
2011 ◽  
Vol 30 (01) ◽  
pp. 56-60
Author(s):  
William P. Brandon

This essay explores efforts to establish interdisciplinary research associations by comparing two organizations that were founded in the early 1980s. One has focused on the field of politics and the life sciences and the other on health services research. Both are involved in securing recognition for a research area—or “field of research”—that had not previously been conceptualized as a coherent academic or professional enterprise. The motivation for this paper is my interest in politics and the life sciences (the field), the organization—the Association for Politics and the Life Sciences that was established in 1980 to foster scholarly study of the field—and its journal Politics and the Life Sciences. (For the sake of clarity I adopt the convention of signifying a field entirely in lower-case orthography, beginning an organizational name with capital letters and naming the related journals in italics.)


2011 ◽  
Vol 30 (1) ◽  
pp. 56-60 ◽  
Author(s):  
William P. Brandon

This essay explores efforts to establish interdisciplinary research associations by comparing two organizations that were founded in the early 1980s. One has focused on the field of politics and the life sciences and the other on health services research. Both are involved in securing recognition for a research area—or “field of research”—that had not previously been conceptualized as a coherent academic or professional enterprise. The motivation for this paper is my interest in politics and the life sciences (the field), the organization—the Association for Politics and the Life Sciences that was established in 1980 to foster scholarly study of the field—and its journal Politics and the Life Sciences. (For the sake of clarity I adopt the convention of signifying a field entirely in lower-case orthography, beginning an organizational name with capital letters and naming the related journals in italics.)


We will try to present critically published works on Quantum Mechanics (QM) and Psychology (perhaps more generally regarding the so called social sciences), partly by ourselves (Giacomuzzi, 2008, 2002), in an overview. It is of course impossible to give a complete summary here, but critical points should be emphasized, which perhaps leave a more differentiated view on the problems of "psychological reality". Nowadays QM is “hip” in scientific literature. But common approaches doesn`t take into consideration that physicists already 80 years ago tried to establish a connection between life sciences and physics. But do neuroscientific findings really validate essential psychological basic assumptions? Do they really open up new, interdisciplinary research perspectives? Physics itself today struggles with its theories and we`ve a big gap between on what we experience and on what we really understand. Maybe this gap of understanding our own reality is much bigger than 120 years ago when QM was born by the work of Max Planck.


2006 ◽  
Vol 3 (8) ◽  
pp. 351-365 ◽  
Author(s):  
Kieron O'Hara ◽  
Richard Morris ◽  
Nigel Shadbolt ◽  
Graham J Hitch ◽  
Wendy Hall ◽  
...  

This paper discusses scientific, social and technological aspects of memory. Recent developments in our understanding of memory processes and mechanisms, and their digital implementation, have placed the encoding, storage, management and retrieval of information at the forefront of several fields of research. At the same time, the divisions between the biological, physical and the digital worlds seem to be dissolving. Hence, opportunities for interdisciplinary research into memory are being created, between the life sciences, social sciences and physical sciences. Such research may benefit from immediate application into information management technology as a testbed. The paper describes one initiative, memories for life, as a potential common problem space for the various interested disciplines.


eLife ◽  
2021 ◽  
Vol 10 ◽  
Author(s):  
Oskar Staufer ◽  
Jacqueline A De Lora ◽  
Eleonora Bailoni ◽  
Alisina Bazrafshan ◽  
Amelie S Benk ◽  
...  

Employing concepts from physics, chemistry and bioengineering, 'learning-by-building' approaches are becoming increasingly popular in the life sciences, especially with researchers who are attempting to engineer cellular life from scratch. The SynCell2020/21 conference brought together researchers from different disciplines to highlight progress in this field, including areas where synthetic cells are having socioeconomic and technological impact. Conference participants also identified the challenges involved in designing, manipulating and creating synthetic cells with hierarchical organization and function. A key conclusion is the need to build an international and interdisciplinary research community through enhanced communication, resource-sharing, and educational initiatives.


1994 ◽  
Vol 144 ◽  
pp. 559-564
Author(s):  
P. Ambrož ◽  
J. Sýkora

AbstractWe were successful in observing the solar corona during five solar eclipses (1973-1991). For the eclipse days the coronal magnetic field was calculated by extrapolation from the photosphere. Comparison of the observed and calculated coronal structures is carried out and some peculiarities of this comparison, related to the different phases of the solar cycle, are presented.


1994 ◽  
Vol 144 ◽  
pp. 21-28 ◽  
Author(s):  
G. B. Gelfreikh

AbstractA review of methods of measuring magnetic fields in the solar corona using spectral-polarization observations at microwaves with high spatial resolution is presented. The methods are based on the theory of thermal bremsstrahlung, thermal cyclotron emission, propagation of radio waves in quasi-transverse magnetic field and Faraday rotation of the plane of polarization. The most explicit program of measurements of magnetic fields in the atmosphere of solar active regions has been carried out using radio observations performed on the large reflector radio telescope of the Russian Academy of Sciences — RATAN-600. This proved possible due to good wavelength coverage, multichannel spectrographs observations and high sensitivity to polarization of the instrument. Besides direct measurements of the strength of the magnetic fields in some cases the peculiar parameters of radio sources, such as very steep spectra and high brightness temperatures provide some information on a very complicated local structure of the coronal magnetic field. Of special interest are the results found from combined RATAN-600 and large antennas of aperture synthesis (VLA and WSRT), the latter giving more detailed information on twodimensional structure of radio sources. The bulk of the data obtained allows us to investigate themagnetospheresof the solar active regions as the space in the solar corona where the structures and physical processes are controlled both by the photospheric/underphotospheric currents and surrounding “quiet” corona.


2000 ◽  
Vol 179 ◽  
pp. 263-264
Author(s):  
K. Sundara Raman ◽  
K. B. Ramesh ◽  
R. Selvendran ◽  
P. S. M. Aleem ◽  
K. M. Hiremath

Extended AbstractWe have examined the morphological properties of a sigmoid associated with an SXR (soft X-ray) flare. The sigmoid is cospatial with the EUV (extreme ultra violet) images and in the optical part lies along an S-shaped Hαfilament. The photoheliogram shows flux emergence within an existingδtype sunspot which has caused the rotation of the umbrae giving rise to the sigmoidal brightening.It is now widely accepted that flares derive their energy from the magnetic fields of the active regions and coronal levels are considered to be the flare sites. But still a satisfactory understanding of the flare processes has not been achieved because of the difficulties encountered to predict and estimate the probability of flare eruptions. The convection flows and vortices below the photosphere transport and concentrate magnetic field, which subsequently appear as active regions in the photosphere (Rust & Kumar 1994 and the references therein). Successive emergence of magnetic flux, twist the field, creating flare productive magnetic shear and has been studied by many authors (Sundara Ramanet al.1998 and the references therein). Hence, it is considered that the flare is powered by the energy stored in the twisted magnetic flux tubes (Kurokawa 1996 and the references therein). Rust & Kumar (1996) named the S-shaped bright coronal loops that appear in soft X-rays as ‘Sigmoids’ and concluded that this S-shaped distortion is due to the twist developed in the magnetic field lines. These transient sigmoidal features tell a great deal about unstable coronal magnetic fields, as these regions are more likely to be eruptive (Canfieldet al.1999). As the magnetic fields of the active regions are deep rooted in the Sun, the twist developed in the subphotospheric flux tube penetrates the photosphere and extends in to the corona. Thus, it is essentially favourable for the subphotospheric twist to unwind the twist and transmit it through the photosphere to the corona. Therefore, it becomes essential to make complete observational descriptions of a flare from the magnetic field changes that are taking place in different atmospheric levels of the Sun, to pin down the energy storage and conversion process that trigger the flare phenomena.


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