Cloud measurements on day 245 of gate

Abstract

On day 245 of GATE (2 September 1974) two lines of convection ‐ north (N) and south (S) ‐ were studied by aircraft stacked vertically, patrolling a north‐south line at longitude 22.85° W of length about 200 km. These lines were part of a complex of convection related to an easterly wave. Photogrammetry shows that the northern line consisted at first of a dense aggregate of small clouds, of width roughly 50 m at cloud base. There were a few tall clouds. No line organization was apparent from the aircraft at 1208 GMT. Fifteen minutes later there was line organization, readily apparent from the DC‐6 aircraft. From study of Electra and DC‐6 records, it appears that a vigorous cold northeasterly surface current initiated line N, and that this was a downdraft originating at altitude about 2.5 km in a mesoscale cloud feature to the north. It appears further that penetrative convection to 14 km followed after the first rain, which moistened air near the surface, and thus lowered cloud bases from about 500 to 350 m.

In overhangs of cloud, anvils to the north of line S, active cloud towers only about 2 km wide were found. The anvils were roughly 2 km thick. Patterns of clouds corresponded to a profile of A/B‐scale divergence; active towers at low levels corresponded to convergence up to the 60 kPa level, and stratus coincided with A/B‐scale divergence aloft at about 50 and 26 kPa.

Statistical analyses from the aircraft films indicated that the area covered by clouds of dark base ‐ signifying concentrated updrafts ‐ was ～5%, much less than that covered by rain at cloud base, ～ 18%. Cloud cover at altitude 4 km was ～ 10%.     

Systematics of superoutbursts in dwarf novae

Photometric properties of known and suspected members of the SU UMa subclass of dwarf novae are tabulated and discussed. The precessing disc model of superoutbursts gives a satisfactory quantitative explanation of the periods of superhumps and their changes during superoutburst. The systems such as WZ Sge and HV Vir that have very long intervals between superoutbursts are deduced to be beyond the orbital period minimum, and have degenerate secondaries. The systems such as V1159 Ori that have extremely short recurrence times have high rates of mass transfer and are the equivalent of the Z Cam subclass that occurs at longer orbital periods.A simplified analytical approach to the theory of accretion discs is able to explain the correlations between normal and superoutburst recurrence times. It also explains the slope of the plateau region of superoutbursts, and why the slope is shallower in the very short recurrence time systems.     

Uy phoenicis: RR lyrae variable,not dwarf nova

Stellar and atomic systems obey analogous angular momentum/mass relationships and analogous angular momentum/magnetic dipole moment relationships. The dimensional constants in both pairs of angular momentum laws appear to be related by a simple set of self-similar scaling equations, suggesting that atomic and stellar systems may be self-similar.     

The component masses of the cataclysmic variable V347 Puppis

We present time-resolved spectroscopy and photometry of the double-lined eclipsing cataclysmic variable V347 Pup (=LB 1800). There is evidence of irradiation on the inner hemisphere of the secondary star, which we correct for using a model to give a secondary-star radial velocity of   K _R= 198 ± 5 km s⁻¹  . The rotational velocity of the secondary star in V347 Pup is found to be   v sin  i = 131 ± 5 km s⁻¹  and the system inclination is   i = 840 ± 23  . From these parameters we obtain masses of   M ₁= 0.63 ± 0.04 M_⊙  for the white dwarf primary and   M ₂= 0.52 ± 0.06 M_⊙  for the M0.5V secondary star, giving a mass ratio of   q = 0.83 ± 0.05  . On the basis of the component masses, and the spectral type and radius of the secondary star in V347 Pup, we find tentative evidence for an evolved companion. V347 Pup shows many of the characteristics of the SW Sex stars, exhibiting single-peaked emission lines, high-velocity S-wave components and phase-offsets in the radial velocity curve. We find spiral arms in the accretion disc of V347 Pup and measure the disc radius to be close to the maximum allowed in a pressureless disc.     

A mathematical model for predicting coupled heat and water movement in unsaturated soil

An investigation was conducted to develop a comprehensive moisture model for predicting non-isothermal moisture conditions in soils. An extensive literature review indicated that a model based on the Philip and de Vries equations for non-isothermal moisture movement and heat conduction would give the best results. By using numerical methods, the implicit finite difference approximations to the moisture movement and heat-transfer equations were programmed for computer solution of water content and temperature in the soil with time. Validation studies indicate that the moisture model can be used to predict accurately moisture conditions in the soil. The model was validated by using hydraulic data from laboratory studies conducted on soil columns compacted with AASHO A-3 and AASHO A-4 soil. The application of the moisture model to the study of non-isothermal moisture movement in the field is demonstrated. The influence of parameters such as water table depth, precipitation, and soil hydraulic properties on soil moisture content are shown by use of the moisture model. The model is shown to be applicable to a wide range of boundary conditions and that it predicts the moisture-temperature regime with time in soils utilizing climatic input data.     

The orientation of the solar rotation axis from Doppler velocity observations

Mt. Wilson observations of solar velocity fields have been examined for evidence that the rotation axis of the nonmagnetic gas at the solar surface is oriented differently than the axis found by Carrington (1863) from sunspot observations. No difference is found with an accuracy of 0°.15 in the angle of inclination of the axis to the ecliptic.     

Fabry-Perot determinations of midlatitude F-region neutral winds and temperatures from 1975 to 1979

Fabry-Perot interferometer measurements of the Doppler shifts and widths of the nightglow 630.0 nm line at Laurel Ridge Observatory, Pennsylvania are presented for the period 1975 to 1979, covering both solar minimum and solar maximum conditions. The F-region neutral wind vectors v_n and temperatures T_n deduced from these measurements show both day-to-day changes and overall seasonal patterns in the nocturnal variations during geomagnetically quiet conditions. Divergence in both the meridional and zonal horizontal flow is noted on occasion. The v_n results are compared with models including only solar EUV heating and those with EUV plus a high latitude heat source. The aggregate v_n data for solar cycle minimum conditions agree best with model predictions for winter zonal and equinoctal meridional winds and worst for winter meridional and summer zonal winds. At solar cycle maximum the predicted, rapid transition at equinox from summer to winter wind patterns and vice-versa is observed. The T_n data are in reasonable agreement with the MSIS model predictions.     

A GEOGRAPHY OF RESEARCH-GRANT GETTING IN GEOGRAPHY

Geographers have become increasingly interested in who receives grants for basic research and why. Northeastern U.S. universities, and especially private universities in the Northeast, dominated those of all other regions in the number of proposals submitted to the Geography and Regional Science Program of the National Science Foundation as well as the number of funded projects and total awarded funds during the period 1979–1981. Successful grant applicants submitted proposals that demonstrated excellent potential to make a significant contribution towards improving the theoretical and methodological foundations of geography.