A new class of trapped light filaments
New class light filament identified in Raman radiation of intense ruby laser beam
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New class light filament identified in Raman radiation of intense ruby laser beam
Use of filament wound toroids as pneumatic shock absorbers
Filament overwrapped metallic cylindrical pressure vessels show greater efficiency ratio and buckling strength
Methods to improve heat transfer efficiency between filament and cathode electron tubes
Smooth-bonded metal liners for glass fiber filament-wound pressure vessels
Liquid filament breakdown into drops by acoustic vibration
Tensile and interlaminar shear strengths of glass, boron, and graphite filament wound resin composites and liners for cryogenic pressure vessels
Boron filaments for possible use as reinforcing phase in composite materials for aerospace structures
Mechanical properties of continuous filament- graphite matrix composite in 0.50 inch diameter rod form, discussing limitation of binder phase and interface
Filament overwrapped metallic cylindrical pressure vessels show greater efficiency ratio and buckling strength
Metal lined glass filament-wound pressure vessel performance at cryogenic temperatures, discussing fibers, resins and liners
Adhesives to bond metal linings to filament- wound cryogenic pressure vessels evaluated by test series simulating fabrication and service conditions
Boron and graphite filament-resin composites tensile and interlaminar shear strengths and Al foil liner cyclic life in cryogenic pressure vessel tests
We will present observational evidence that the eruption of filaments and coronal mass ejections (CMEs) occur as a consequence of the destabilization of large scale coronal arcades due to newly emerging magnetic flux reconnecting with the preexisting arcades.
We report on four large filament eruptions (FEs) from solar cycles 23 and 24 that were associated with large solar energetic particle (SEP) events and interplanetary type II radio bursts. The post-eruption arcades corresponded mostly to C-class soft X-ray enhancements, but an M1.0 flare was associated with one event. However, the associated coronal mass ejections (CMEs) were fast (speeds approx. 1000 km/s) and appeared as halo CMEs in the coronagraph field of view. The interplanetary type II radio bursts occurred over a wide wavelength range, indicating the existence of strong shocks throughout the inner heliosphere. No metric type II bursts were present in three events, indicating that the shocks formed beyond 2-3 Rs. In one case, there was a metric type II burst with low starting frequency, indicating a shock formation height of approx.2 Rs. The FE-associated SEP events did have softer spectra (spectral index >4) in the 10-100 MeV range, but there were other low-intensity SEP events with spectral indices ⩾4. Some of these events are likely FE-SEP events, but were not classified as such in the literature because they occurred close to active regions. Some were definitely associated with large active region flares, but the shock formation height was large. We definitely find a diminished role for flares and complex type III burst durations in these large SEP events. Fast CMEs and shock formation at larger distances from the Sun seem to be the primary characteristics of the FE-associated SEP events.
Fiber reinforced composite materials, owing to their tailorable thermomechanical and functional properties, allow one to produce a structure that is stronger, stiffer, and lighter than its metal counterpart while performing the same function, yielding a more efficient structure. This not only allows for the improvement of current technologies like aircraft structures, but also enables new technologies like gaseous hydrogen storage for mobility applications, which are otherwise impractical when manufactured using traditional metals due to weight and space restrictions or material embrittlement. However, the use of composites imposes greater design and manufacturing challenges on an engineer, since they are heterogenous, having a distinct structure across multiple length scale, behave generally anisotropically at the structural level and require complex manufacturing and processing methods. Capturing this complex behavior requires detailed numerical simulations, including the modeling of microstructural features like undulations, voids, and fiber alignment. In this paper, multiple repeating unit cells (RUCs), representing filament wound composites, are developed (via a script provided in the Appendix) and analyzed. The refinement of these RUCs is varied, and the analyses are performed using both the Abaqus finite element software and the NASA Multiscale Analysis Tool (NASMAT). A study is undertaken to compare the predicted effective elastic properties of the wound RUC to a laminate representation of the wound RUC, which neglects the undulations. Additionally, two different sets of periodic boundary conditions (PBCs) have been examined. One approximates the real boundary conditions using a standard approach and the other represents the PBCs exactly through the use of an offset. Lastly, a comparison of the local elastic stress fields is made among the models and approaches. Since wound structures are often approximated as laminated structures, it is important to understand the degree to which this assumption is valid, namely by first comparing the elastic constants and local elastic fields. This will provide, on the one hand, information concerning the bulk mechanical behavior and, on the other hand, insights concerning local load distributions and likely damage initiation sites.
Radiofrequency radiation and particle acceleration from solar flare filaments due to rotational collective motion of electrons or ions
Resistance wire layer is introduced during winding of the fiber glass filaments with simultaneous heating. Emission of heat from the wire layer cures second fiber glass layer.