NASA NTRS ยท 19720019351
Spherical balloon response to three-dimensional time-dependent flows
Abstract
The concept of the Lagrangian displacement of a balloon is introduced. It is shown that the general balloon response problem is extremely complicated because the wind-forcing functions in the balloon equations of motion are functions of the wind velocity vector and its Eulerian first derivatives evaluated at the location of the balloon. The linear perturbation equations for a spherical balloon are derived by perturbing the components of velocity of the balloon about a terminal velocity state which is in equilibrium with a space-time invariant mean horizontal flow. The atmospheric flow is also perturbed such that the resulting equations can be used to analyze the responses of spherical balloons to three-dimensional time-dependent flows. The wind field is represented in terms of a four-fold Fourier integral that involves three orthogonal wave numbers and a frequency, while the balloon components of velocity are represented as Fourier integrals involving a frequency which, in turn, is a function of the wind field wave numbers and frequency and the unperturbed flow components of velocity.
Keep this discovery
Explore connections, maps & timelines
Fichtl, G. H.. 1972-07-01. Spherical balloon response to three-dimensional time-dependent flows. https://ntrs.nasa.gov/citations/19720019351
Cite the original work for its findings. Save a collection to share your selection of sources.