16 September 2010 Payload Proposal Page 1 Colorado Space Grant Consortium GATEWAY TO SPACE FALL 2010 BALLOON PAYLOAD PROPOSAL Team Khufu Members: Henry Shennan, Chelsea Donaldson, Graham Risch, Jennifer Nill, and Jonathan Lupkin 16 September 2010 Revision 0 16 September 2010 Payload Proposal Page 2 1: Mission Overview This satellite will be equipped with a magnetometer, as well as thin solar films attached to a data collector. The purpose of the magnetometer is to measure how magnetic fields change as elevation increases. We expect to find a change in magnetism as the balloonSat rises through the atmosphere. Just as the different levels of the atmosphere affect temperature, we are going to measure the effects of the levels of the troposphere on the magnetic field around the satellite. If we consider the earth as a point charge, and the satellite as another, then the data we can expect to collect will follow Coulomb’s law, which states that the electromagnetic force will decrease in an inverse square relationship as elevation increases. The solar panels placed outside of the satellite will convert solar energy to electrical energy, which will then be measured in watts. We can use this data to analyze how solar energy varies in each layer of the atmosphere. Because of money and technological restraints, we will utilize photovoltaic solar cells, which use a silicon phosphorous material in which easily moveable electrons create an electric current when struck by photons from the sun. The atmosphere is known to refract light, which can affect the energy output of a solar cell. Measuring the solar intensity throughout the atmosphere will allow us to locate the optimum altitude for solar energy collection. In conjunction with the solar panels, we will also measure UV radiation through the use of photodiodes. The photodiodes will measure UV radiation in the form of watts as well. The ozone has been proven to block some UV rays, and by comparing where the UV radiation is strongest with the electrical output of the solar cells, we can determine the role ultraviolet light has in solar energy collection. It stands to reason that the more photons there are, the more energy is radiated by the sun. We aim to prove the correlation, if there is any, between atmospheric conditions and different forms of electromagnetic waves. By conducting these experiments simultaneously, we will be able to isolate which variable is affecting our data, since there are many factors-- such as temperature and weather-- that can alter the mission’s results. This mission will allow us to perform a comparative analysis of electromagnetics in the atmosphere. In addition, we will use a HOBO data collector to measure temperature inside and outside the satellite and relative humidity. This will allow us to record how climate changes throughout the atmosphere. A camera will also be mounted on the satellite to track our flight path visually. One adjustment that will need to be accounted for is the effect of extreme temperature on the solar panel and UV photodiode. Temperature affects the resistance of materials, and therefore modifications must be made to ensure the accuracy of the data collected. We can monitor just how much the temperature is affecting our results by plotting how the temperature changes throughout the flight. Using all of the data collected, we can form a correlation between temperature, altitude and atmospheric conditions and UV, magnetic and solar strength. 16 September 2010 Payload Proposal Page 3 2: Design and Technical Overview 2.0: Design Description The structure of will consist of a triangular box constructed from 0.125” foam board, reinforced along the exterior edges with Aluminium tape, and insulated with 0.25” foam insulation. Structural joints will be made by bonding the foam board with hot melt adhesive. The balloon tether line will be run through a PVC tube along the center of gravity of the craft and will be fixed in place through the use of knots at either end of the tube and protected using rubber bushings. Data collection will be carried out by three separate subsystems: the HOBO unit, which will record internal and external temperature and internal humidity; the digital camera, which will record images of the ascent, descent, and of Earth’s curvature at predefined intervals for the duration of the mission; and by the Arduino microcontroller, which will record data from the onboard sensors to flash memory. The intervals at which the camera takes photographs will be controlled by a cracked version of the camera firmware. The primary mission payload will consist of two UV photodiodes, operational over the 20-350nm wavelength range, four photovoltaic cells, and a magnetometer. The secondary mission payload will consist of the camera and the temperature and pressure sensors onboard the HOBO. The photodiodes will be used to collect data on the intensity of incident ultraviolet radiation at various altitudes, and will be compared to data collected from the photovoltaic cells. The efficiency of the encapsulated photovoltaic cells will be tested under the varying atmospheric conditions as the balloon-sat rises through the atmosphere by measuring the power they collect. The magnetometer will be used to characterize Earth’s magnetic field and to look for minute changes in the magnetic field as a function of altitude. 2.1.1: Testing The first round of testing will consist of tests on all of the individual components to ensure that they function properly. Components will be tested according to their manufacturer’s instructions, and will be tested in conditions consistent with what they will experience during the mission. The second round of testing will be conducted on the subsystems. The magnetometer will be tested while in its final configuration and the results will be compared to the earlier tests in which the instrument was isolated in order to determine if onboard electronics will cause unacceptable levels of interference (above) within the instrument. The external structure of the craft will be tested for integrity by first conducting drop tests from a height of 20m, and then by being spun on a 1m cord at a minimum of 50rpm. Those tests will only consist of the structure with representative weights replacing onboard instruments. If any single component or subsystem fails a test, it will not be integrated into the larger subsystem (or craft as a whole). The final round of testing will be tests on the entire craft complete with electronics. These tests will include, at minimum, a vibration test to simulate atmospheric buffeting, a temperature test to simulate 16 September 2010 Payload Proposal Page 4 temperatures down to 253K, and a full mission simulation. The temperature test will be achieved by packing the craft into an insulated container with 100-300g of dry ice while the electronic systems are running. Temperatures will be monitored from outside the external container using either a digital thermometer or an additional HOBO device. 2.1.2: Data Analysis After recovery of the satellite, data recorded in the flash ROM of the Arduino microcontroller will be downloaded from that device using a USB cable to a laptop computer running the LabVIEW instrumentation suite produced by National Instruments. Data will be exported from LabVIEW to Microsoft Excel and analyzed along with data collected from the HOBO using Onset’s HOBOware software. 2.2: Requirements Met The total mass of the craft with payload is projected to be 750g (with a mass allowance of 100g. For details, please see section 2.4), within the 850g limit set by the requirements in the RFP. Our design includes the HOBO, Canon camera, internal heater, and temperature sensors mandated by the requirements, and satisfies the requirement that the craft be constructed of foam-core board. Our budget does include a $50 lump sum for spare parts and damaged part replacement, and still meets the requirement that the total budget be under $300. The craft is designed to be reusable, and will include identification and an American flag on an exterior surface. Finally, onboard heaters will ensure that the internal temperature of the craft remains above 263K and a central PVC tube with rubber bushings will ensure that the tether is not damaged during the mission. 2.3: Safety Observations While constructing and testing this satellite we will observe proper safety precautions as outlined by Professor Koehler and as described on the ITLL safety sheet. Work with soldering irons will take place in a well-ventilated area and diligence will be exercised to prevent burns and solder overflow and sputtering. During construction of the electronic subsystems ESD precautions will be observed; all members working on the microcontroller, sensors, and magnetometer will be required to wear antistatic bracelets properly connected to a common ground. In addition, wiring of key electronic components will be checked at least twice prior to the application of current in order to both safeguard the electronics and prevent accidents due to component malfunction and/or failure. Finally, both the drop and whip tests will be conducted in broad daylight under favorable weather conditions, and by at least two people: one to conduct the test, and the second to spot him or her. Both team members will be required to wear helmets for the duration of the tests. Finally, any tests involving dry ice will be conducted with the use of gloves and safety glasses to prevent contact burns and injuries due to fragmentation of the dry ice. 2.4: Necessary Components Part Dimensions Supplier Cost 16 September 2010 Arduino Nano HOBO H08-004-02 Canon A570IS digital camera Heating circuit 9V Batteries and 5V regulator Foam Board and Foam insulation Camera Timing Circuit External switches (x3) PVC pipe with rubber bushings Low Cost–High Output Encapsulated Solar Cells (x4) UV Photodiodes 20-350nm (x4) MicroMag 3-Axis Magnetometer Payload Proposal Page 5 10x18x45mm, 10g SparkFun Electronics 68x48x19mm, 30g GTS 45x75x90mm, 220g GTS 10x50x50mm, 100g GTS <35g GTS See section 3.5, 150g GTS Replaced by camera firmware, N/A 5x5x20mm, 15g total GTS 10x350mm, 15g McGuckin’s Hardware 26x45x7mm, 80g total Edmund Scientifics $18.95 - 5x5x5mm, 20g total 25x25x19mm, 10g $80.00 $59.95 2.5: Craft Design Figure 1: Satellite, exploded view Figure 2: Satellite, flight configuration Boston Electronics SparkFun Electronics $3.55 $15.80 16 September 2010 Payload Proposal Page 6 2.6: Functional Block diagrams Batteries: (9V with 5V regulator) switch Microcontroller: Arduino Pro Mini 328- 5V/16MHz Magnetometer Camera: Includes power source (AA batteries) and data storage (flash memory) Flash ROM switch Photovoltaic Cells switch IR Photodiodes Heater Timing Circuit Humidity HOBO External Temperature Internal Temperature 16 September 2010 Payload Proposal 3.0: Proposed Project Schedule design complete 9/16/2010 acquire all hardware Magnetometer sensor test prototyping design complete 9/28/2010 9/30/2010 10/4/2010 DD Rev A/B and CDR presentation 10/5/2010 cold test complete Drop test Whip test 10/12/2010 10/12/2010 10/12/2010 testing final design complete mission simulation 10/26/2010 10/28/2010 LLR presentation and DD Rev C Weigh In final presentations due design document Rev D due design Expo Hardware Turn in 11/2/2010 11/5/2010 11/30/2010 12/4/2010 12/4/2010 12/7/2010 Page 7 16 September 2010 Payload Proposal Page 8 3.1: Team Organizational Chart Chelsea Team Leader Jonathan Structral Design Henry Graham Jen IT/Programming Manager, Systems Integration Solar Panel Experiment Design UV Probe Experiment Design Budget Manager 3.2: Team Member Descriptions Name Chelsea Donaldson Jennifer Nill Jonathan Lumpkin Henry Shennan Duty Structural Design, Payload Assembly Systems Integration and Programming Woodshop Skills good listener and innovative ideas Technical and computer skills Graham Risch Structural design, Budgetary Management Organization and building skills Team Leader Skills Leadership and good imagination Phone number 970-331-6409 303-241-7143 Testing and Design Troubleshooting 970-669-8776 303-564-7575 678-463-1374 3.3: Budget Graham will be in charge of ordering components and ensuring that the project remains within the stated maximum budget of $300. Component Expenses Part Arduino Nano Supplier SparkFun Electronics Cost $18.95 16 September 2010 Payload Proposal Page 9 PVC pipe with rubber bushings McGuckin’s Hardware $3.55 Low Cost–High Output Encapsulated Solar Cells (x4) UV Photodiodes (x4) MicroMag 3-Axis Magnetometer Testing Expenses Dry Ice Batteries: 9V Edmund Scientifics Boston Electronics SparkFun Electronics $15.80 $80.00 $59.95 Safeway Grocery McGuckin’s Hardware $10.00 $20.00 Allowance for spare parts and damaged part replacement - $50.00 Total Expenses $258.25