FEB 14 "94

FROM KAMAN SCIENCES CORP

14:14

TO 1722952154

COGE . 202/226

which are the residue of bamb elements and surface materials,
soil and water, made radioactive by accompanying radiation
fields. Debris is sucked high into the atmosphere by artter
winds of the explosion. ‘here this radioactive debris will

fall is a major pre-shot consideration and primarily influences

the decision to detonate a nuclear explosion at a certain time.

The area over which radioactive debris is spreac anc the
intensity of fall-out on the ground are determined by the yield
of the explosion as well as by wind pattern since the larger
the yield, the more surface materials are sucked up into the
¢loud and the more fission fragments are available. The rela-

tionship between yield and fall-out is known only qualitatively.

4.

PRE-SHOT INFORMATION:

The operational aspects of the

BRAVO experience were planned and canceived in the liaht of

experience gained from previos operations.
considered:

a.

These factors were

The basis for forecasting where fallout will go

ig exDerience gained from overseas test operations CROSSROADS,

SANDSTONE, GREENHOUSE and IVY and to a certain extent from tests

at the Nevade Froving Ground.

Prier to the firing of BRAVO,

only one megaton yield device (IVY-MIKE) had been detam ted.
Although conscientious efforts were made to document the fall-

out from MIKE, only about 5% of the total debris could ever de

accounted for.

The technique used for forecasting fallout pat-

terns is to consider the cloud as a small area source (about a
15 mile radius); then add vectorially forecast winds from the
surface to approximately 100,000 feet.
The next step is to
outline an area on the ground where faliout is expected.
This

area is computed by taking into consideration particle aize,
diffusion into the atmosphere, wind pattern, yield and source

radius.
Such patterns have seen largely confirmed by experience in Nevada as well es by the meager data available hare.

b.

The most probable value of the yield from QD

was predicted to be three to five mogatons or one half tas

value of the IVY-LIKE yield.

The upper limit of qQyyig@fyiela

was considered to be of the order of aight megatons.
co.

Tha surface radex was plotted, with an insurance

factor added, i.a.,

smaller particles than previous experience

indicated necessary were considered.
This doubled distances
from ground zero where fallout was predicted to occur.
ad.

The upwind intensity of radiation levels et vari-

ous distances was considered to be of the same order of magritude as for IVY-MTKE.
Radiation versus distance lines were
transposed to Sikini Atoll.

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