Probabilistic dynamics of a global horizontal sounding system
Probability method for position and motion of large numbers of constant-level balloons - atmospheric circulation
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Probability method for position and motion of large numbers of constant-level balloons - atmospheric circulation
NASA space science and applications program - satellite and space probe flights, sounding rocket, balloon borne, and aircraft experiments, and associated research
A method of combining the information from the infrared interferometer spectrometer (IRIS) and the backscatter ultraviolet spectrometer (BUV) on board the Nimbus-4 satellite to derive the ozone profile from 10 mb to surface is described. The radiance in the IRIS 9-micron band can be related to the ozone profile by the radiative transfer equation. The IR intensity due to ozone is dependent on the pressure broadening of spectral lines, and an estimate of a weighted mean pressure of the ozone layer can be obtained from total ozone supplied by BUV long wave intensity measurements. With the aid of the Chapman function, a model of the ozone concentration profile described by three parameters is obtained. Given the ozone concentration at 10 mb one calculates several possible combinations of the three parameters that can produce the required total ozone, and the final choice of parameter is determined from IR measurements. An ozone profile calculated in this way reproduces well the gross features of balloon ozone sounding results. Meridional cross sections of ozone concentration have also been derived which are in reasonably good agreement with balloon-derived cross-section for the northern latitudes and tropics.
Personnel from the Goddard Space Flight Center Wallops Flight Facility (GSFC/WFF in Virginia have successfully tested commercial LEO communications satellites for sounding rocket, balloon and aircraft flight TT&C. The Flight Modern became a GSFC/WFF Advanced Range Technology Initiative (ARTI) in an effort to streamline TT&C capability to the user community at low cost. Ground tests of the Flight Modem verified duplex communications quality of service and measured transmission latencies. These tests were completed last year and results reported in the John Hopkins University (JHU) Applied Physics Laboratory (APL) 4th International Symposium on Reducing Spacecraft Costs for Ground Systems and Operations. The second phase of the Flight Modem baseline test program was a demonstration of the ruggedized version of the WFF Flight Modem flown on a sounding rocket launched it the Swedish rocket range (Esrangc) near Kiruna, Sweden, with results contained in this paper. Aircraft flight tests have been and continue to be conducted. Flights of opportunity are being actively pursued with other centers, ranges and users at universities. The WFF Flight Modem contains a CPS receiver to provide vehicle position for tracking and vehicle recovery. The system architecture, which integrates antennas, CPS receiver, commercial satellite packet data modem and a single board computer with custom software, is described. Small satellite use of the WFF Flight Modem is also being investigated, The Flight Modem provides an independent vehicle position source for Range Safety applications. The LEO communication system contains a coarse position location system, which is compared to GPS ace acy. This comparison allows users, to determine the need for a CPS receiver in addition to the satellite packet data modem for their application.
Analog-to-digital converter-pulse height analyzer for data reduction from balloon measurements
Balloon-borne spark chamber and magnet system for identifying and measuring momentum of cosmic radiation particles
IR spectroscopic observations with balloon-borne telescope, Stratoscope II
Balloon measurement of charge ratio of primary cosmic ray electrons in energy level from 100 mev to 3 bev in 1964
Wind sensor capabilities of several types of balloon, noting expandable neoprene
Ballistic factors, balloon measured wind data, and impact predictions for Aerobee rocket launch
Flux and energy spectrum of primary electron component measured by balloon at period near solar activity minimum
Balloon-borne scintillation counters combined with Cerenkov counter for measuring primary cosmic ray charge and energy spectra during 1963
Spectral variation of low energy galactic cosmic ray protons and helium nuclei measured by balloon flights
Localization and motion of energetic electron precipitation regions during negative magnetic bays, noting similarity of motion to that of auroral electrojets
Mesoscale perturbations in vertical wind velocity profiles obtained from superpressure balloons tracked by FPS-16 radars
Camera tubes for recording Stratoscope II TELESCOPE, noting photometric fidelity
Crab Nebula X-ray spectrum from 16-120 kev by balloon
Flux and energy spectrum of primary electron component measured by balloon at period near solar activity minimum