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MEL

The Microgravity Emissions Laboratory (MEL) was developed for the support, simulation and verification of the International Space Station (ISS) microgravity environment. The MEL utilizes an inertial measurement system using acceleration emissions generated by various operating components of ISS. These emissions, if too large, could hinder the science performed on ISS, by disturbing the microgravity environment.

Typical test components are disk drives, pumps, motors, solenoids, fans, cameras, etc. These components will produce inertial forces, which disturb the microgravity on-orbit station environment. These components, usually housed within a station rack, must meet acceleration limits imposed at the rack interface for minimizing the on-board station-operating environment. NASA GRC has developed this one of a kind laboratory for testing components and eventually rack level configurations. The MEL approach is to measure the component's generated inertial forces. This force is a product of the full diagonal mass matrix including the test setup (the center of gravity, mass moment of inertia, and weight) and the resolved diagonal rigid body acceleration made up using the 10 apparatus accelerometers. The mass matrix can be test derived. The moment of inertia for the test component is measured using the bifilar torsional pendulum method.

The MEL is a low frequency (0.15-0.4 Hz) isolator. The lateral frequencies are established with the pendulum and the vertical mode is lowered with a zero rate spring mechanism (ZSRM). The ZSRM reduces the system's vertical frequencies to approximately 0.3 Hz. The ZSRM suspends the measurement apparatus with the attached test unit by a long cable. The system allows the test article to float freely similar to a zero-g condition above 1 Hz. The measured motion of the rigid body is characterized through the MEL test and post processing of the accelerometer data is done to calculate the rigid body component forces and moments at the center of gravity/interface of the test unit.

MEL was developed for the Fluid Combustion Facility through the Microgravity Sciences Division (MSD). The laboratory is located in the Structural Dynamics Laboratory (SDL). Engineering models of the FCF Optics Bench and Air Thermal Control Unit have been tested in FY 01.

These test are done on operating equipment; therefore pre-test planning is a must. All umbilicals, services such as water, power etc. are provided by the customer unless alternate arrangements are made. Due to the isolation required, umbilicals and support service lines need to be long (5-10 meters). The operations matrix is also provided by the customer. Any non-standard fixturing issues will need to be resolved as test planning begins. Any help needed in formulating these needs can be rapidly responded to by filling out our on-line form.

Award Winning Microgravity Emissions Laboratory
Tom Goodnight accepted the Silver Snoopy Award
from Astronaut Lee Morin on November 1, 2000
for successfully creating the Microgravity Emissions
Testing Laboratory at NASA Glenn Research Center.


 

Click here for PCS test report.

 

Click here for FCF Optics Bench Test Data (7216KB)



Laboratory Schedule: (last update 011/14/01)

September 2001

October 2001

November 2001 December 2001
 
 
 



Laboratory Information:

Click here for MEL Schematic Drawing

How to request and schedule your test

Click here for Microgravity Emissions Laboratory Overview Presentation

Lab capabilities

Lab personnel



MEL Manager:

Anne M. McNelis,(216)433-8880
Anne.M.McNelis@grc.nasa.gov


Location:

Structural Dynamics Laboratory
NASA Glenn Research Center
21000 Brookpark Rd.
Cleveland, Ohio 44135
(216)433-6263


SDL Lab Manager:

Gail P. Perusek, (216)433-8729
Gail.P.Perusek@grc.nasa.gov


 Responsible NASA person: Kevin McPherson pims@grc.nasa.gov

This page maintained by:
Tim Reckart,Zin Technologies, Inc.tim.reckart@grc.nasa.gov

This page was last updated on April 21, 2005

 
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