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Brief Description of Goals

General

This experiment will test the effect of different levels and type of radioactivity in radioisotopes implemented in soil of plants on bean plant growth and development. This is significant because these radioisotopes are utilized in everyday life including the use of Am-241 in smoke detectors and medical diagnostics; Cs-137 in cancer treatment; and Sr-90 in bone cancer treatment and eye treatment.

Cosmic Ray Detector

The purpose of this detector is to establish an uncertainty of the fluctuation of cosmic radiation which contributes to the uncertainty of the overall radiation effecting the plants being tested. It also provides a method to check the dosage of the varying types of radiation from the following radioisotopes.

This website provides in-depth directions on how to construct a cosmic ray detector, and it's instructions provide us with a backbone from which we can design our own detector [1]

We have also done calculations according to the procedure laid out by this procedure:

ΔΩ=(A/4πR^2)*4π

Where ΔΩ equals the subtended solid angle (in steradians) of the cone the two detectors make, A equals the area of the paddle, and R equals the distance from the center of one paddle to a corner of the other.

flux=ΔΩ*Fv*A

Where Fv equals the published value for flux at sea level, which equals 0.66/(cm squared*min*steradians)

Using this method, we calculated the expected flux using the setup in the lab already [1.50/(cm squared*min*steradians)] and using larger sized paddles (14cmx10cmx1xcm) which gave us the expected flux of 9.19/(cm squared*min*steradians). If this process is to be trusted, making the paddles this size would result in an increase in flux of 613%, which makes the construction of new scintillators worthwhile.

Preliminary Test Results

Running the muon counter for a cycle of 24 hours (1440 minutes) a total of 1948 counts were recorded.

**Radioactive Isotopes**
Source	Initial Activity	Input Date	Current Activity	Radioactive Particle Distribution
Bi-210	12 μCi	11/3/1972	0 μCi	β- and a little alpha
Cs-137	2.3 μCi	7/1/1988	1.3 μCi	Gamma and Beta
Cs-137	17.8 μCi	10/15/1965	5.92 μCi	Gamma and Beta
Cs-137	3.86 μCi	10/15/1965	1.28 μCi	Gamma and Beta
UO₂ - Ore	(1.90 g)			Alpha
Am-241	0.1 μCi	10/1965	0.09 μCi	Primarily emits alpha, but also gamma
Co-60	unknown			Gamma and Beta
Ru-106	5.5 μCi	2/2/1977	1.05E-10 μCi	Beta
Sr-90	0.1 μCi	6/2003	0.1 μCi	Beta and infrequently gamma
Sr-90	0.1 μCi	6/2003	0.1 μCi	Beta and infrequently gamma

Experimental Setup

To begin our experiments, we will test the effect of different dosages and types of radiation (alpha, beta and gamma) on the bean plants. After completing this portion of the experiment, we will select the dose that stimulated plant growth the most, and use it to test different stages of plant life. To ensure that the plants germinate naturally, and without any radiation, we will germinate them on cotton pads. This should reduce an unexpected deaths prior to germination. The seeds that do germinate will be transferred to the soil in one of six cardboard boxes. A schematic of the desired setup will be attached shortly. Basically, there will be two levels of independent variable in each box, and eight repeated trials. For each type of radiation, there will be four levels of independent variable (total dose). To calculate the total dose, we are utilizing an online calculator to calculate the expected dose and subtracting the attenuation of the soil from that. Our dose levels will be within the tolerated level for that plant.

After this experiment has shown what dose we should use to test the effect of radiation on different stages of plant life. The following stages will be tested: germination, sapling (1 week), and nearing adult (2 weeks), and adult (3 weeks). We will expose the different plants for one week and compare them to a control with no radiation exposure.

@@ Line 12: / Line 12: @@
 == Cosmic Ray Detector ==
+The purpose of this detector is to establish an uncertainty of the fluctuation of cosmic radiation which contributes to the uncertainty of the overall radiation effecting the plants being tested. It also provides a method to check the dosage of the varying types of radiation from the following radioisotopes.
 This website provides in-depth directions on how to construct a cosmic ray detector, and it's instructions provide us with a backbone from which we can design our own detector [http://cosmic.lbl.gov/documentation/CosmicDetector2-0.pdf]
@@ Line 27: / Line 29: @@
 Using this method, we calculated the expected flux using the setup in the lab already [1.50/(cm squared*min*steradians)] and using larger sized paddles (14cmx10cmx1xcm) which gave us the expected flux of 9.19/(cm squared*min*steradians). If this process is to be trusted, making the paddles this size would result in an increase in flux of 613%, which makes the construction of new scintillators worthwhile.
-The purpose of this detector is to establish an uncertainty of the fluctuation of cosmic radiation which contributes to the uncertainty of the overall radiation effecting the plants being tested. It also provides a method to check the dosage of the varying types of radiation from the following radioisotopes.
+=== Preliminary Test Results ===
+Running the muon counter for a cycle of 24 hours (1440 minutes) a total of 1948 counts were recorded.
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