NASA Technical Reports Server (NTRS) 19990027824: Martian Meteorology: Determination Of Large Scale Weather Patterns From Surface Measurements - Info and Reading Options

The Internet Archive:

We employed numerical modelling of the martian atmosphere, and our expertise in understanding martian atmospheric processes, to better understand the coupling between lower and upper atmosphere processes. One practical application of this work has been our involvement with the ongoing atmospheric aerobraking which the Mars Global Surveyor (MGS) spacecraft is currently undergoing at Mars. Dr. Murphy is currently a member of the Mars Global Surveyor (MGS) Aerobraking Atmospheric Advisory Group (AAG). He was asked to participate in this activity based upon his knowledge of martian atmospheric dynamical processes. Aerobraking is a process whereby a spacecraft, in an elliptical orbit, passes through the upper layers of the atmosphere (in this instance Mars). This passage through the atmosphere 'drags'upon the spacecraft, gradually reducing its orbital velocity. This has the effect, over time, of converting the elliptical orbit to a circular orbit, which is the desired mapping orbit for MGS. Carrying out aerobraking eliminates the need for carrying large amounts of fuel on the spacecraft to execute an engine burn to achieve the desired orbit. Eliminating the mass of the fuel reduces the cost of launch. Damage to one of MGS's solar panels shortly after launch has resulted in a less aggressive extended in time aerobraking phase which will not end until March, 1999. Phase I extended from Sept. 1997 through March 1998. During this time period, Dr. Murphy participated almost daily in the AAG meetings, and beginning in December 1997 lead the meeting several times per week. The leader of each of the daily AAG meetings took the results of that meeting (current state of the atmosphere, identification of any time trends or spatial patterns in upper atmosphere densities, etc.) forward to the Aerobraking Planning Group (APG) meeting, at which time the decision was made to not change MGS orbit, to lower the orbit to reach higher densities (greater 'drag'), or raise the orbit to avoid experiencing excessive, possibly damaging densities.

Search for “NASA Technical Reports Server (NTRS) 19990027824: Martian Meteorology: Determination Of Large Scale Weather Patterns From Surface Measurements” downloads:

Visit our Downloads Search page to see if downloads are available.

Find “NASA Technical Reports Server (NTRS) 19990027824: Martian Meteorology: Determination Of Large Scale Weather Patterns From Surface Measurements” in Libraries Near You:

Read or borrow “NASA Technical Reports Server (NTRS) 19990027824: Martian Meteorology: Determination Of Large Scale Weather Patterns From Surface Measurements” from your local library.

• The WorldCat Libraries Catalog: Find a copy of “NASA Technical Reports Server (NTRS) 19990027824: Martian Meteorology: Determination Of Large Scale Weather Patterns From Surface Measurements” at a library near you.