model or whether there are other mechanisms for producing such echoes. Possible mechanisms are wind-driven atmospheric waves excited by topographic features and various types of wavelike structures in the ionosphere driven by interactions with the solar wind.Conclusion. The MARSIS ionospheric soundings have shown that the ionosphere of Mars is in good agreement with the expectations of Chapman's 1931 photoequilibrium theory for the origin of planetary ionospheres. The soundings have also revealed a number of unexpected features. These include echoes that reoccur at the electron cyclotron period, large variations in the absorption apparently caused by energetic solar events, oblique echoes caused by ionospheric structures associated with the crustal magnetic fields of Mars, diffuse echoes apparently caused by scattering from ionospheric irregularities, and ionospheric holes. Because the subsurface soundings must occur at frequencies well above the maximum electron plasma frequency in the ionosphere and under conditions of low ionospheric absorption, these measurements have already proved to be quite useful for planning subsurface sounding operations. The electron cyclotron echoes also provide a new method of measuring the local magnetic field strength, which is useful because Mars Express does not have a magnetometer.
Animal Evolution and the Molecular Signature of Radiations Compressed in TimeAntonis Rokas,* Dirk Krüger,. Sean B. Carroll-The phylogenetic relationships among most metazoan phyla remain uncertain.We obtained large numbers of gene sequences from metazoans, including key understudied taxa. Despite the amount of data and breadth of taxa analyzed, relationships among most metazoan phyla remained unresolved. In contrast, the same genes robustly resolved phylogenetic relationships within a major clade of Fungi of approximately the same age as the Metazoa. The differences in resolution within the two kingdoms suggest that the early history of metazoans was a radiation compressed in time, a finding that is in agreement with paleontological inferences. Furthermore, simulation analyses as well as studies of other radiations in deep time indicate that, given adequate sequence data, the lack of resolution in phylogenetic trees is a signature of closely spaced series of cladogenetic events.Detailed knowledge of the phylogenetic relationships among Metazoa and their eukaryotic relatives is critical for understanding the history of life and the evolution of molecules, phenotypes, and developmental mechanisms.Currently, with the exception of the well-resolved phylogenetic history of the deuterostomes (1), the relationships between and within protostome and diploblastic metazoan phyla remain unresolved (2-5). The uncertainty surrounding metazoan relationships may result from analytical and biological factors such as insufficient amounts of available sequence data, mutational saturation, the occurrence of unequal rates of evolution between lineages, or the rapidity with which metazoan phyla diversified (3-7). Recen...