TECHNICAL NOTE D ABLATING UNDER CONSTANT AERODYNAMIC CONDITIONS. By Robert R. Howell. Langley Research Center Langley Station, Hampton, Va.

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-. NASA TN D-1635 TECHNICAL NOTE 1 D- 1635 AN EXPERIMENTAL STUDY OF THE BEHAVIOR OF SPHERES ABLATING UNDER CONSTANT AERODYNAMIC CONDITIONS By Robert R. Howell Langley Research Center Langley Station, Hampton, Va. NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WASHINGTON April 1963

NATIONAL AERONAUTICS AND SPACE ADMINISTRATION TECHNICAL NOTE D-1635 AN EXF'ERIMNTAL STUDY OF THE BEHAVIOR OF SPHERES ABLATING UNDEB CONSTANT AERODYNAMIC CONDITIONS By Robert R. Howell SUMMARY Five spheres constructed of ablative material, with diameters of 0.6 inch to 2.0 inches, were subjected to aerodynamic heating to determine the physical behavior of such bodies as they are reduced toward zero volume by the ablation process. Three of the bodies were tested in hypersonic flow, one was tested in supersonic flow, and one was tested in subsonic flow. The stagnation-point heating rate for the tests varied between '32 and 565 Btu/(sq ft)(sec). The Reynolds number based on model diameter varied between 1.0 x lo4 and 9.6 x 10 li. For the range of.test conditions covered in the experiment, results indicate that the recession rate of the stagnation point is essentially constant over the life span of such bodies, regardless of the magnitude and character of the convective heating imposed. There was an apparent tendency for the average radius of the ablating face to increase slightly with time at supersonic and hypersonic speeds and to decrease with time at the subsonic speed. In the supersonic tests, no noticeable loss of material occurred over the downstream surface of the bodies. In the subsonic test, however, loss on the downstream surface equaled that over the forward surface. A discussion of the measured recession rate of the stagnation point is presented. INTRODUCTION The ablation process has been shown to be a most efficient means of achieving thermal protection for vehicles reentering the earth's atmosphere. Post-reentry examinations have indicated that ballistic vehicles protected in this manner generally experience only small changes in basic shape and a relatively small loss of ablation material. Meteoroids, however, which enter the earth's atmosphere at higher velocities, are often completely destroyed. Any theory of meteoroid entry (ref. 1, for example) or spacecraft entry must necessarily include certain assumptions regarding the variation of the heating load on the reentering body and the resulting shape changes. Inasmuch as the ablation process for such bodies may not proceed in the manner assumed, it was considered appropriate to make a brief experimental study of the process.

~ Tests have been conducted at the Lctngley Research Center to determine experimentally the changes in shape and mass-loss rate with time experienced by spheres ablating under constant convective heating and loading. Three facilities, a subsonic arc-heated jet, a supersonic arc-heated jet, and a hypersonic combustionheated tunnel, were used to provide a range of aerodynamic heating rates and flow conditions. The stagnation-point heating rate for the tests varied between 52 sq ft)(sec) and the Reynolds number varied between 1.0 x lo4 and 9.6 x 10. A detailed description of these tests and a discussion of the pertinent results are presented herein. SYMBOLS cp DO specific heat of ablative material (solid), Btu/( lb) (OR) initial diameter of sphere, ft % E m = cpta + HL + v(hs - Hw), Btu/lb I HL HS HW rh 9 qs latent heat of vaporization, Btu/lb stream enthalpy at body stagnation point, Btu/lb enthalpy at body surface, Btu/lb mass loss rate due to ablation, lb/(sq ft)(sec) local heating rate to body, Btu/(sq ft)(sec) stagnation-point heat-transfer rate, Btu/( sq ft) (sec) I R Ta t V VO X Xf test Reynolds number based on initial diameter of sphere temperature at which material ablates, OR time, sec volume of body, cu ft initial volume of sphere, cu ft distance along streamwise axis of body (fig. 3) streamwise body-axis station where volume integral is closed (fig. 3) I 2

Y radius of body normal to streaxwise axis (fig. 3) 6 recession of stagnation point due to ablation of body, ft 7 shielding coefficient P density, lb/cu ft Sub scripts : calc exp calculated experimental MODELS All the bodies tested were initially spherical and were sized in accordance with the heating rate, running time, or test-section size of the facility to be used for testing. Table I presents the pertinent information for each sphere and TABLE I. - DESCRIPmON OF SPEIERES AND T- PROPERTIES OF TBE WLWKULS Model Sphere Do, in. Density (solid), p, lb/cu ft Shielding coeff., q heat J cpi Btu/( lb) (OF) Effective heat of ablation,* chloride Teflon 88 137 137 137 137 1,420 1,550 0.5.4.4.4.4 0.38.30-30 * 30-30 1,890 1,332 1,907 1,783 "Computed on basis of test conditions in table 11. indicates the model designations. Sketches of the models and their supports are presented in figure 1 and photographs of models A, D, and E are presented in figure 2. (Models A, B, and C differ only in material and sphere diameter.) It should be noted that the sphere support stings for the arc-heated (higher energy level) facilities were constructed of a phenolic-impregnated cloth. Experience has indicated that the high heating rate would cause failure of less bulky metal support stings in a time interval less than that needed to ablate the sphere to zero volume. FACILITIES Tests were conducted in three different facilities. Models A, B, and C were tested in the '7-inch Mach 7 pilot tunnel, which is a hypersonic blowdown tunnel that uses as its test medium the combustion products resulting from burning a 3

_- MODEL A MODEL B MODEL C MODEL D \ MODEL E Figure 1.- Support arrangement and pertinent dimensions for the various spheres tested. All dimensions are in inches. 4

Figure 2.- Photographs of spheres p r i o r t o t e s t i n g. L-63-23 5

mixture of ethylene (C2H4) and air under pressure. The flow developed by this facility simulates flight at a Mach number of 7.0 in that the gas Ls expanded to a static temperature near Oo F and correct velocity is simulated. The usable test core in this facility is approximately 3 inches in diameter. Model D was tested in a subsonic arc-heated air jet. The flow developed by this facility is a 4-inch-diameter jet of underexpanded high-temperature air discharging to the atmosphere at a velocity of approximately 900 ft/sec. The static temperature of the jet is about 6,800~ R. Model E was tested in a supersonic arc-heated air jet. The flow developed by this facility is an underexpanded free jet which discharges to a reduced pressure at a Mach number of 2.6. and the velocity about 7,300 ft/sec. The jet diameter is 2 inches at the nozzle exit. The static temperature of the jet is about 3,700 R TESTS Table I1 presents the pertinent test conditions to which each model was subjected. In each case the model was held out of the test region until the test conditions were established. The model was then inserted into the test region TABLE 11.- TEST CONDITIONS Stagnation- Stagnationpoint press., atm Stagnation-point heating rate, 's, Btu/(sq ft)(sec) Test Reynolds number, R A B C D E 3,100 3,100 3,200 6,840 5,850 0.64.64-69 1.13.95 930 9 30 1,080 2,500 2, loo 52.4 7.0 350 65.6 7.0 35 0 88.9 7.0 360 180.0.24 6,804 565.0 2.6 3,715 9.6 x I& 1.4 1.1 for the duration of the test and retracted prior to tunnel shutdown. Cn the case of models A, B, C, and E, reference measurements for the determination of stagnation pressure and temperature were recorded continuously during the test interval. These measurements were generally in the form of output from thermocouples and pressure transducers and were recorded on oscillographs. For the test of model D, a calibrated calorimeter was inserted into the jet just prior to insertion of the model. The output from this calorimeter was calibrated in terms of stagnationpoint heating rate. With this rate and the known pressure in the arc chamber, the stagnation conditions on the model were computed. The degree of uncertainty of the body stagnation-point conditions quoted in table I1 varies for the different test facilities used. For example, for models A, B, and C the stagnation-point heating rate is believed to be quite 6

accurately known (to within +3 percent) as a result of accurate measurements of the tunnel stagnation temperature and pressure. For model D the stagnation-point heating rate indicated by the calorimeter is believed to be accurate to within about k10 percent. For model E the stagnation heating rate was deduced from a knowledge of the flow rate of air through the tunnel, the tunnel stagnation pressure, and the power input to the arc. The resulting heating rate quoted for model E is believed to be accurate to within f10 percent. The basic data obtained from the tests were shadowgraph pictures taken every 3 seconds during the test interval for models A, B, C, and D. For mdel E the pictures were taken every 1.5 seconds. In addition to these shadowgraph pictures, black and white or colored motion pictures were taken to provide pictorial data for each test. RFSULTS AND DISCUSSION The shadowgraph pictures taken at discrete time intervals during the tests were enlarged and traced for each of the models. A composite drawing of these tracings for four of the models is presented in figure 3. (For ease in making comparisons between models, the scale of the spheres has been adjusted in figure 3 so that all models appear the same size.) Models B and E were ablated to zero volume. In order to accomplish this result for model B, two runs were required. Although transient conditions were encountered at the beginning of each test run, they did not seriously alter the progression of the ablation, as will be shown later in the discussion. Model E was reduced to zero volume during one test rm. The bodies tested in hypersonic and supersonic flows experienced similar variations in forward-surface profile. In general there was a tendency for the radius of the forward surface to increase slightly with time. It should be noted here that the shape changes experienced by the bodies in these tests are due entirely to convective heating. If radiative heating were large, as it would be for hyperbolic reentry into the earth's atmosphere, further increases in forwardsurface radius could probably be expected. No significant loss of material occurred on the downstream surface of the bodies tested in supersonic flows. The irregularity of the contours of model E (fig. 3) at 11.1 and 14.1 seconds was indicated by motion pictures to be due to the interference with the body by the compression wave originating at the jet exit. The model moved off the jet center line as the test progressed because of unsymmetrical heating of the metal support, and thus encountered the effects of the compression wave during the final half of the tests. The stagnation point shifted on the body as a result of the angle of attack and caused a rounding of the shoulder opposite the one affected by the shock wave. Models A, C, and D were not ablated to zero volume. Two runs were made of model A without completing its ablation. A photograph of the remaining portion of the body is presented as figure 4. The appearance of the body in this photograph is typical of the bodies in their final stages of existence in supersonic flow.

t=o MODEL A L Flow MODEL B MODEL D MODEL E Figure 3.- Composite drawings showing the profiles of the bodies at specific times durbg the ablation process. Model D, which was tested in subsonic flow, experienced mass loss over the downstream surface of the body in an amount about equal to that over the forward face (fig. 3). After 82 seconds the ablation on the rear portion of the body caused the body to part from the sting. A photograph of the remains is presented as figure 5. The downstream ablation experienced by the body in the subsonic jet is believed to be due to the relatively high static pressure and temperature of the jet and the turbulent action of the wake downstream of the point of separation on the body. It should be noted that the forward half of this model maintained more of a spherical shape than the models in the supersonic and hypersonic tests. (Compare models A, B, and E with D in fig. 3.) 8

Figure 4.- Remaining portion of model A a f t e r t e s t s. Figure L-62-2464 5.- Remaining portions of model D and support after t e s t s. L-62-1356 9

The volume of the body corresponding to any shadowgraph picture was computed by mechanical integration of the equation JO where values of y and x were obtained from measurements made on the tracing of the enlarged shadowgraph. The enlargement for all bodies was sufficient to make small inaccuracies of measurement result in insignificant changes of computed volume. The ratios of the computed volume V to the initial volume Vo for each model are presented as a function of time in figure 6. The density of the materials from which the models were constructed was found to vary somewhat during the test run. Thermal expansion of Teflon was very noticeable during the long runs at low heating rates (see fig. 3, model B). Also, for both the ammonium chloride body (model A) and the Teflon body (model B) there was a discontinuity of volume between the test runs (see figs. 6(a) and 6(b)) that indicated thermal expansion. The apparent density changes of the ammonium chloride were less than those exhibited by the Teflon. During the initial 10 seconds of the tests that were made at low heating rates (models B and C) the expansion of the Teflon offset the volume lost due to ablation (see figs. 6(b) and 6(c)). In the tests at high'heating rates (models D and E) the expansion was not noticed. In all cases, as the body temperature approached equilibrium the apparent rate of volume loss became reasonably regular over the length of the test run. The measured recession of the stagnation point due to ablation, as obtained from measurements of shadowgraph pictures, is expressed as 1 - - and presented in figure 7 as a function of time. All the bodies experienced a nearly linear recession of the stagnation point with time. It should be noted here, also, that the recession of the stagnation point for models A and B was not significantly altered by the fact that the ablation took place during two separate test runs. DO I The effective heat of ablation for the different bodies has been determined by use of the equation where the values of stagnation-point heating rate and material density are those presented in tables I and I1 and the recession rate db/dt was determined from figure 7. These experimentally determined effective heats of ablation are compared with the values computed according to the equation 10

Time, t, sec (a) Model A (ammonium chloride) 1 4-0 Q 0 Time, t, sec (b) Model B (Teflon). Figure 6.- Variation of body volume Kith time for each of the spheres tested. 11

1.0.a.6.4.2 0 0 4 0 12 16 20 24 20 36 Time, t, sec (c) Model C (Teflon). 1.0.0.6.4.2 0 (a) Model D (Teflon). Figure 6.- Continued. 12

(e) Model E (Teflon). Fiaure 6.- Concluded. results are presented in the following table: The variation of the experimental value of He from the calculated is less than k10 percent for the Teflon bodies (models B, C, D, and E), indicating that the certainty of the test conditions and the knowledge of the ablating characteristics of this material (Teflon) are very good. The prediction of the stagnationpoint recession rate based on the calculated value of R, would also have been within k10 percent if it were assumed that the bodies had a constant stagnationpoint heating rate.

1.0.8.6 6 1-- Do.4-2 0 20 40 60 80 100 120 140 160 Time, t, sec, Figure 7.- Variation of stagnation-point location with time for the various spheres tested. I 1 For model A (the ammonium chloride body) the agreement between experimental and calculated values of He was poor. This discrepancy is believed to result from a lack of knowledge of the ablation characteristics of the material. The heat of vaporization used to compute H, for the ammonium chloride model was 1,340 Btu/lb (taken from ref. 2). Handbooks give the heat of vaporization as 142 Btu/lb (see, for example, ref. 3). The heat actually absorbed in the ablation of the material is dependent upon the extent to which the sublimated material is dissociated and, hence, is a function of the stream stagnation temperature and the heating conditions. Agreement between theory and experiment could have been achieved for the ammonium chloride body if a heat of vaporization of approximately 700 Btu/lb had been used. This value is between the two values quoted from the literature and indicates that for the present results there is either a partial dissociation, a loss of material due to processes other than ablation, or a chemical process occurring in the combustion-products test medium of this particular facility that reduces the effective heat of ablation of ammonium chloride from what it would be in air under similar conditions.

CONCLUDING REMARKS Five spheres constructed of ablative material, with diameters of 0.6 inch to 2.0 inches, have been subjected to aerodynamic heating to determine the physical behavior of such bodies as they are reduced toward zero volume by the ablation process. Three of the bodies were tested in hypersonic flow, one was tested in supersonic flow, and one was tested in subsonic flow. The results indicate that the recession rate of the stagnation point is essentially constant over the life span of such bodies. There was an apparent tendency for the average radius of the ablating face to increase slightly with time at supersonic and hypersonic speeds and to decrease with time at subsonic speeds. In the supersonic tests, no noticeable loss of material occurred over the downstream surface of the bodies, whereas in the subsonic test the loss over the downstream surface equaled that over the forward surface, apparently because of turbulent wake action at the high static temperature. The effective heats of ablation computed by using the experimental stagnation-point recession rate, material density, and body stagnation-point heating rate were in good agreement with the calculated values for the Teflon bodies. The inability to achieve similar agreement for the ammonium chloride body is believed to be due primarily to lack of knowledge of the ablation characteristic of this material. Langley Research Center, National Aeronautics and Space Administration, Langley Station, Hampton, Va., January 21, 1963. 1. Hansen, C. Frederick: The Erosion of Meteors and High-speed Vehicles in the Upper Atmosphere. NACA TN 3962, 1957. 2. Welker, Jean E.: Comparison of Theoretical and Experimental Values for the Effective Heat of Ablation of Ammonium Chloride. NASA TN D-533, 1960. 3. Hodgman, Charles D., Weast, Robert C., and Selby, Samuel M., eds.: Handbook of Chemistry and Physics. Forty-first ed., Chemical Rubber Pub. Co., 1959-1960. 4. Steg, Leo: Materials for Re-Entry Heat Protection of Satellites. ARS Jour., vol. 30, no. 9, Sept. 1960, pp. 815-822.