Deglaciation history and landscape development of fjord-valley deposits in Buvika, Mid-Norway

Thick deposits of glaciomarine clay and silt overlain by Holocene marine sediments in Norwegian fjord valleys have been, and still are, subject to erosional processes such as river incision, ravine formation and slide activity. In Buvika, Mid‐Norway, these land‐forming processes have been highly influenced by the valley‐fill stratigraphy. Glaciomarine and marine clay sediments dominate this 8 km long hanging valley south of the Gaulosen fjord, with local occurrences of coarser‐grained sediments. Studies of sediments and structures in road excavations together with ¹⁴C ages indicate at least one, possibly two, minor glacier readvances in late Allerød/early Younger Dryas (YD) time. This implies a more dynamic ice sheet with more minor ice‐front oscillations than earlier documented in this region. Glacioisostatic rebound resulted in groundwater leaching of marine clay and quick‐clay formation in certain layers or zones. The relative sea‐level fall led to incision by rivers accompanied by numerous slides involving quick clay, which completely liquefies when remoulded. To the east, permeInger‐Lise Solberg (e‐mail: inger‐lise.solberg@sintef.no ), Department of Geology and Mineral Resources Engineering, Norwegian University of Science and Technology (NTNU). Present address: SINTEF Building and Infrastructure, Høgskoleringen 7a, NO‐7465 Trondheim, Norway; Kåre Rokoengen, Department of Geology and Mineral Resources Engineering, NTNU, Sem Sælands veg 1, NO‐7491 Trondheim, Norway; Louise Hansen, Lars Olsen and Harald Sveian, Geological Survey of Norway, NO‐7491 Trondheim, Norwayable layers of northwesterly dipping sand and gravel generally originate from a former ice‐marginal delta. These relatively thick and frequent layers of interbedded sand and gravel in the clay‐dominated deposits drain groundwater in the slopes, leading to the development of deeply incised ravines. To the south and north, thinner layers of coarse material in the clay lead to pore‐pressure build‐ups and quick‐clay development, resulting in numerous slide scars. Knowledge of the morphology, stratigraphy and erosion pattern of areas prone to formation of quick clay is important in order to understand the landscape development and evaluate risk areas.     

Are There Radio-quiet Solar Flares?

Some 15% of solar flares having a soft X-ray flux above GOES class C5 are reported to lack coherent radio emission in the 100 – 4000 MHz range (type I – V and decimetric emissions). A detailed study of 29 such events reveals that 22 (76%) of them occurred at a radial distance of more than 800″ from the disk center, indicating that radio waves from the limb may be completely absorbed in some flares. The remaining seven events have statistically significant trends to be weak in GOES class and to have a softer non-thermal X-ray spectrum. All of the non-limb flares that were radio-quiet above 100 MHz were accompanied by metric type III emission below 100 MHz. Out of 201 hard X-ray flares, there was no flare except near the limb (R>800″) without coherent radio emission in the entire meter and decimeter range. We suggest that flares above GOES class C5 generally emit coherent radio waves when observed radially above the source.     

Effect of organic complexation on the toxicity of Cu to the earthworm Eisenia fetida

The relationship between Cu speciation in solution and mortality and tissue Cu concentrations in Eisenia fetida was investigated. E. fetida were exposed to solutions containing 0.009, 0.049 and 0.125 mg Cu L⁻¹and 0, 0.15, 0.35 and 50 mg EDTA L⁻¹. Mortalities of 100, 60, 50 and 25% were recorded in the 0.125 mg Cu L⁻¹ solutions containing 0, 0.15, 0.35 and 50 mg EDTA L⁻¹, respectively. Similarly tissue body burden decreased with increasing EDTA concentration. Complexation capacity of the solution increased with EDTA concentration. In the 0.125 mg Cu L⁻¹ solution labile Cu concentration decreased with increasing EDTA concentration. These trends are attributed to complexation of free Cu ions with EDTA molecules, and the non-bioavailable nature of the resultant Cu–EDTA complex.     

Pulsar magnetosphere

Pulsars are presently believed to be rotating neutron stars with large frozen-in magnetic fields normally assumed to be dipole fields. It has been shown that such a star must possess a magnetosphere if it rotates sufficiently rapidly. By assuming that the magnetic field is dipolar, and unaffected by the trapped particles in the magnetosphere, and that the field dipole axis is parallel to the rotation axis, Goldreich and Julian determined many of the properties of the magnetosphere. In this paper is given a self-consistent model of the closed field lines of a pulsar magnetosphere. Using this model, it is shown that, close to the star, the above assumptions of Goldreich and Julian are justified. Their results are extended to the oblique rotator as well as to stars with magnetic multipoles of arbitrary order and arbitrary orientation.Supported in part by the U.S. Atomic Energy Commission under Grant 2171T.     

Stratospheric trace gas analysis from ions: H2O and HNO3

A new method for stratospheric trace gas analysis based upon in situ ion composition measurements is presented. The strength of the method lies in its extremely high sensitivity which at present allows for detection limits of the order of 100–1000 molecules cm^?3 corresponding to volume mixing ratios of the order of 10^?15–10^?14 around 35 km altitude. The typical uncertainty of derived trace gas abundances is plus or minus a factor of about two. A disadvantage lies in the selectivity of the method which is restricted to trace gases having either large proton affinities, dipole moments or gas phase acidities. Analyses of water vapor and nitric acid vapor in the upper stratosphere are presented.     

Ion-induced nucleation of atmospheric water vapor at the mesopause

The possibility of aerosol formation at the mesopause by ion-induced water vapor nucleation is investigated. A simple kinetic model considering new information on ion-growth and -recombination processes as well as on mesospheric water vapor and temperatures is put forward. It predicts ion-nucleation to be possible only at high latitudes during local summer in a narrow height region, extending from about 88 to 91 km. Derived nucleation rates increase steeply with decreasing temperatures and electron number densities. If for the latter typical values are considered nucleation rates may become sufficiently high to account for the observed mesospheric aerosol layer. Various observed characteristic temporal and spatial variations of the aerosol layer including its response to geomagnetic activity may be explained by the model.     

Echeloned Series Processor (ESP)

An Echeloned Series Processor (ESP) has been implemented on a computer. The processor has certain similarities with MAO (MAO is a processor for Poisson series). Echeloned Series contain divisors in literal form. List processing and dynamic storage techniques are used to handle Echeloned Series by computer.