Z-selective olefin metathesis using chelating ruthenium alkylidene catalysts

Publications about olefin metathesis will generally discuss how the discovery and development of well-defined catalysts to carry out this unique transformation have revolutionized many fields, from natural product and materials chemistry, to green chemistry and biology. However, until recently, an entire manifestation of this methodology had been inaccessible. Except for a few select examples, metathesis catalysts favor the thermodynamic trans- or E-olefin products in cross metathesis (CM), macrocyclic ring closing metathesis (mRCM), ring opening metathesis polymerization (ROMP), and many other types of reactions. Judicious choice of substrates had allowed for the direct synthesis of cis- or Z-olefins or species that could be converted upon further reaction, however the catalyst controlled synthesis of Z-olefins was not possible until very recently.

Research into the structure and stability of metallacyclobutane intermediates has led to the proposal of models to impart Z-selectivity in metathesis reactions. Having the ability to influence the orientation of metallacyclobutane substituents to cause productive formation of Z- double bonds using steric and electronic effects was highly desired. The first successful realization of this concept was by Schrock and Hoveyda et al. who synthesized monoaryloxide pyrolidine (MAP) complexes of tungsten and molybdenum that promoted Z-selective CM. The Z-selectivity of these catalysts was attributed to the difference in the size of the two axial ligands. This size difference influences the orientation of the substituents on the forming/incipient metallacyclobutane intermediate to a cis-geometry and leads to productive formation of Z-olefins. These catalysts have shown great utility in the synthesis of complicated natural product precursors and stereoregular polymers. More recently, ruthenium catalysts capable of promoting Z-selective metathesis have been reported by our group and others. This thesis will discuss the development of ruthenium-based NHC chelated Z-selective catalysts, studies probing their unique metathesis mechanism, and synthetic applications that have been investigated thus far.

Chapter 1 will focus on studies into the stability of NHC chelated complexes and the synthesis of new and improved stable chelating architectures. Chapter 2 will discuss applications of the highly active and Z-selective developed in Chapter 1, including the formation of lepidopteran female sex pheromones using olefin cross metathesis and highly Z- and highly E-macrocycles using macrocyclic ring closing metathesis and Z-selective ethenolysis. Chapter 3 will explore studies into the unique mechanism of olefin metathesis reactions catalyzed by these NHC chelated, highly Z-selective catalysts, explaining observed trends by investigating the stability of relevant, substituted metallacyclobutane intermediates.

Solar photospheric and coronal abundances from solar energetic particle measurements

Observations of solar energetic particles (SEPs) from 22 solar flares in the 1977-1982 time period are reported. The observations were made by the Cosmic Ray Subsystem on board the Voyager 1 and 2 spacecraft. SEP abundances have been obtained for all elements with 3 ≤ Z ≤ 30 except Li, Be, B. F, Sc, V, Co and Cu. for which upper limits have been obtained. Statistically meaningful abundances of several rare elements (e.g., P, Cl, K, Ti, Mn) have been determined for the first time, and the average abundances of the more abundant elements have been determined with improved precision, typically a factor of three better than the best previous determinations.

Previously reported results concerning the dependence of the fractionation of SEPs relative to photosphere on first ionization potential (FIP) have been confirmed and amplified upon with the new data. The monotonic Z-dependence of the variation between flares noted by earlier studies was found to be interpretable as a fractionation, produced by acceleration of the particles from the corona and their propagation through interplanetary space, which is ordered by the ionic charge-to-mass ratio Q/ M of the species making up the SEPs. It was found that Q/M is the primary organizing parameter of acceleration and propagation effects in SEPs, as evidenced by the dependence on Q/M of time, spatial and energy dependence within flares and of the abundance variability from flare to flare.

An unfractionated coronal composition was derived by applying a simple Q/M fractionation correction to the observed average SEP composition, to simultaneously correct for all Q/M-correlated acceleration/propagation fractionation of SEPs. The resulting coronal composition agrees well with current XUV/X-ray spectroscopic measurements of coronal composition but is of much higher precision and is available for a much larger set of elements. Compared to spectroscopic photospheric abundances, the SEP-derived corona appears depleted in C and somewhat enriched in Cr (and possibly Ca and Ti).

An unfractionated photospheric composition was derived by applying a simple FIP fractionation correction to the derived coronal composition, to correct for the FIP-associated fractionation of the corona during its formation from photospheric material. The resulting composition agrees well with the photospheric abundance tabulation of Grevesse (1984) except for an at least 50% lower abundance of C and a significantly greater abundance of Cr and possibly Ti. The results support the Grevesse photospheric Fe abundance, about 50% higher than meteoritic and earlier solar values. The SEP-derived photospheric composition is not generally of higher precision than the available spectroscopic data, but it relies on fewer physical parameters and is available for some elements (C, N, Ne, Ar) which cannot be measured spectroscopically in the photosphere.

The conjugate representation of signal envelope

The problem of the representation of signal envelope is treated, motivated by the classical Hilbert representation in which the envelope is represented in terms of the received signal and its Hilbert transform. It is shown that the Hilbert representation is the proper one if the received signal is strictly bandlimited but that some other filter is more appropriate in the bandunlimited case. A specific alternative filter, the conjugate filter, is proposed and the overall envelope estimation error is evaluated to show that for a specific received signal power spectral density the proposed filter yields a lower envelope error than the Hilbert filter.