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Kirby Research Group

Professor Mark Campbell's Research Group
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Student Satellite Projects

The vision of the student satellite projects is to develop and maintain a Space Systems Center that gives students of many disciplines and levels access to space. The mission of this center is to design, fabricate, test, and operate micro-and nano-satellites, i.e., satellites in the 50 to 1 kg range, using a broad base of students from MAE, ECE, CS, and other disciplines. The center supports both research and education. Three types of missions are underway and/or envisioned:

  • Simple satellites that give undergraduates and MEng students quick access to space, and a challenging space based educational environment; an example of this is the CubeSat program
  • More complex science and technology demonstrations, where engineering expertise is required to fly and test cutting edge technologies that will pay off in the future for Earth and space science; an example of this is the ION-F/Dawgstar and CUSat missions
  • Earth and space science missions, with PI leads at Cornell. This includes ionospheric science, as well as space science.

To date, our group has focused on missions in the first two classes (described below). Funding has come from a variety of sources including NASA, the Navy, Air Force, and DARPA, alumni, and industry.

Projects

ICECube
Sponsors: ONR, alumni

ICECube satellite prior to delivery

Description of GPS scintillations, which are measured in the ICECube mission.

Testing of the communications system from Ithaca College; Cornell's Bell Tower is in the background.

The Ionospheric sCintillation Experimental CubeSat (ICE CUBE) is a two satellite mission designed to explore simple GPS scintillation experiments in the mid-equitorial region. The science instrument is the Cornell Cougar GPS receiver. The space based testbed consists of two clusters of 10cm CubeSats, to be flown in 2006. The satellite bus, a 10cm aluminum cube with functional power electronics, communication capability, and a science instrument. The attitude control system is based on a gravity gradient boom and magnetic coils.

The goal of Cornell ICECube satellite project in general is two-fold: First, to qualify the concept of small satellites as useful instruments for science and engineering, to lower the cost of space utilization and exploration; Second, to educate students in all major aspects of the design, construction, and launch of space satellite systems.

The ICECube mission will launch two 10cm cube satellites designed to study the effects of scintillations in the Earth’s ionosphere on communication signals. Irregularly structured ionospheric regions can cause diffraction and scattering of trans-ionospheric radio signals. When received at an antenna, these signals present random temporal fluctuations in both amplitude and phase. Ionospheric scintillations may cause problems such as signal power fading, phase cycle slips, receiver loss of lock, etc. They are also known to degrade the quality of satellite navigation systems. This degradation lowers the signal-to-noise ratio of received GPS signals. The satellite will include an on-board GPS receiver, which will record the SNR of the received signal from the GPS satellites. This information will be stored on the satellite until it is transmitted to the ground station where it will be used to characterize the effects of the scintillations on communication signals.

To date, the ICECube project has educated over 100 students in several disciplines (ME, AE, EE, CS), in several stages of education (High School, BS, MS, MEng, PhD).

The CubeSat program was established in 1999 by Stanford University, Cal Poly Tech, and One Stop Satellite Solutions in an effort to bring satellite development, launch, and operation more closely to the students. Said another way, most satellites take years to develop, usually wait to be launched, and usually must be operated by the government or NASA. This program is designed to make is very inexpensive ($30K+ satellite costs) to launch the satellites. In addition, launches occur on a yearly basis which allows universities to design and fly a new satellite each year.

Currently, the two Cornell ICECube satellites have been delivered to Cal Poly University for integration, with launch expected in January 2006.

ION-F/Dawgstar
Sponsors: AFRL, NASA, AFOSR, Primex, WTC, alumni.

Dawgstar in the clean room.

Prototype PPT firing in the vacuum chamber.

Flight units for PPT's.

ION-F mission patch.

The Ionospheric Observation Nanosatellite Formation (ION-F) comprises three 15 kg spacecraft designed and built in cooperation by Utah State University, University of Washington (Cornell University), and Virginia Polytechnic Institute in order to develop a space based distributed control testbed. A novel feature of the mission is the planned suite of formation flying control experiments involving the three satellites.

The ION-F mission is part of the Air Force Research Laboratory/AFOSR/DARPA University Nanosatellite Program, which provides technology development and demonstrations for the TechSat21 Program. The University Nanosatellite Program involves 10 universities building nanosatellites for a 2004 launch on a space shuttle mission. The ION-F satellites are being designed and built by students at the three universities, with close coordination to insure compatibility for launch, deployment, and the formation flying mission.

The ION-F satellites will have many of the capabilities necessary to demonstrate multiple spacecraft distributed control. These include propulsion, inter-satellite communication, and GPS measurements. Most of the technology development is being developed in parallel to the program. This includes the UW pulsed plasma thrusters (UW with Primex), and the inter-satellite crosslink/GPS system (Applied Physics Lab at Johns Hopkins under NASA funding).

The Dawgstar satellite, started in 1998-99, has educated over 75 students in several disciplines (ME, AE, EE, CS), in several stages of education (High School, BS, MS, MEng, PhD). The students designed the satellite in conjunction with other universities, presented to Air Force, NASA, and Industry, and worked with the NASA safety board to gain acceptances for Shuttle. Dawgstar is unique in its ability to integrate research (formation flying) and education (space systems engineering).

The PPT thrusters were designed as a part of the DAWGSTAR program to provide formation keeping, orbit maintenance and attitude control functions for satellites in the 10-100 kg range. Thrust is created when solid Teflon propellant is ionized by a pulsed, high current electrical arc and accelerated by a combination of electromagnetic and gas dynamic forces. The system presented provides thrust levels from 60 to 275 micro-N with specific impulses up to 625 sec. A centralized power-processing unit utilizing high voltage switching enables a reduction in system mass when compared to previous designs. The total mass for the system presented is 4.20 kg which enables control of three axes of rotation and two axes of translation. Approximately 1.7 Million pulses were successfully accumulated on the flight qualification unit representing a total system impulse of approximately 1000 N•s.

The Dawgstar satellite was completed through hardware development and testing. But, due to the Columbia shuttle accident and programmatic issues with the organization of the first nanosat program, the Dawgstar/ION-F mission currently does not have a flight scheduled. Many of the attributes have been re-incarnated into the CUSat mission (see below).

CUSat
Sponsors: AFRL, NASA, alumni

CUSat patch.

The CUSat will demonstrate how one spacecraft can diagnose the health and configuration of another, a capability that will help enable commercial, government, and manned space missions envisioned for the coming decades. The satellites will be designed, built, and operated primarily by Cornell students. One of the two spacecraft will capture three-dimensional imagery of the other with the help of carrier-phase differential GPS algorithms.

Cornell University Space Systems Labs is participating in the University Nanosatellite-4 program. This program is a joint venture between the Space Vehicles Directorate of the Air Force Research Laboratory, the Air Force Office of Scientific Research and the American Institute of Aeronautics and Astronautics. As participants, twelve universities design and fabricate proto-flight nanosatellites, each with a unique mission. The universities will participate in a June 2007 flight competition with the winner receiving accelerated flight upgrades and a fully sponsored launch.

Facilities

Over the past eight years, our facilities have grown to include a class 1000 clean room, high performance computers (CAD, development), GPS simulator, sun simulator with a Xeon lamp, thermal vacuum system, a ground constrol station atop Barton Hall on the Ithaca campus, and vibration facilities at a local company.

Thermal vacuum testing.

Sun simulator testing.

 

Vibration testing.

Publications

  • C. D. Rayburn, M. E. Campbell A. T. Mattick, “Pulsed Plasma Thruster for Microsatellites,” AIAA Journal of Spacecraft and Rockets, Vol. 42, No. 1, Jan-Feb 2005.
  • S. Mohan, M. Campbell, et al, “The ICE CUBE Project”, Space 2003, Sept 2003.
  • Hoskins, A., Sarmiento, C., Rayburn, C., and Campbell, M., “The Electromagnetic Compatibility of Pulsed Plasma Thrusters with Spacecraft Systems,” 51st Joint Army-Navy-NASA-Air Force (JANNAF) Propulsion Meeting, November 2002.
  • Waydo, S., Henry, D., Campbell, M., “CubeSat Design for LEO-Based Earth Science Missions,” IEEE Aerospace Conference, Big Sky MT, March 2002.
  • Meller, D. M., Reiter, J., Terry, M., Böhringer, K. F., Campbell, M. “A Docking System for MicroSatellites based on MEMS Actuator Arrays,” AIAA Structures, Structural Dynamics and Materials Conference, April 2001.
  • Meller, D., Sripruetkiat, P., Makovec, K., Campbell, M., Fullmer, R., Hall, C., “Digital CMOS Cameras for Attitude Determination,” 2000 AIAA/USU Small Satellite Conference, August, 2000.
  • Rayburn, C., Campbell, M., Hoskins, A., Cassady, J., “Development of a micro-PPT for the Dawgstar Nanosatellite,” AIAA Joint Propulsion Conference, July 2000.
  • Campbell, M., Swenson, C., Fullmer, R., Hall, C., “The Ionospheric Observation Nanosatellite Formation – ION-F,” Small Satellite Systems and Service Conference, La Baule, France, June 2000.
  • Campbell, M. Schetter, T., “Formation Flying Mission for the UW Dawgstar Nanosatellite,” IEEE Aerospace Conference, March 2000.
  • Cassady R. J., Hoskins, W. A., Campbell M., and Rayburn, C., “A Micro-Pulsed Plasma Thruster for the Dawgstar Spacecraft” IEEE Aerospace Conference, March 2000.
  • Campbell, M., Fullmer, R., Hall, C., “The ION-F Formation Flying Experiments,” AIAA Space Flight Mechanics Meeting, January 2000.
  • Campbell, M., et al “The ION-F Mission and Dawgstar Satellite,” 1999 AIAA Space Technology Conference, September 1999.
  • Campbell, M., et al “The UW Dawgstar Nanosatellite,” AIAA/USU Small Satellite Conference, August 1999.
  • Reiter, J., Böhringer, K., Campbell, M., “MEMS Control Moment Gyroscope Design and Wafer-Based Spacecraft Chassis Study”, SPIE Symposium on Micromachining and Microfabrication, Santa Clara, CA, September 1999.
  • Hoskins, W. A., Wilson, M. J., Willey, M. J., Meckel, M. J., Campbell, M., Chung, S., “PPT Development Efforts at Primex Aerospace Company,” Joint Propulsion Conference, July 1999.
  • Martin, M., Cobb, R., Schlossberg, H., Mitola, J., Weidow, D., Peffer, A., Blomquist, R., Campbell, M., Hall, C., Hansen, E., Horan, S., Kitts, C., Redd, F., Reed, H., Spence, H., Twiggs, B., “University Nanosatellite Program,” IAF Symposium, Redondo Beach, April 1999.
  • Martin, M., Cobb, R., Schlossberg, H., Mitola, J., Weidow, D., Peffer, A., Blomquist, R., Campbell, M., Hall, C., Hansen, E., Horan, S., Kitts, C., Redd, F., Reed, H., Spence, H., Twiggs, B., “University Nanosatellite Program,” 2nd international Conference on Integrated Micro-nanotechnology for Space Applications, April 1999.
  • Campbell, M., “Oh Now I get It!,” Journal of Engineering Education, Vol 88, No. 4, Oct 1999.
  • Campbell, M., “Oh, now I get it!” Frontiers in Education Conference, Tempe AZ, November 1998.