An Investigation of the Induced Magnetosphere of Venus and Its Interaction with the Solar Wind

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Venus (Planet), Venus Atmosphere, Solar Wind, Sun, Solar Planetary Interactions, Planetary Magnetospheres, Planetary Magnetic Fields, Planetary Magnetotails, Interplanetary Magnetic Fields, Astrophysics, Reproduction (Copying), Students, University Program, Bow Waves, Magnetometers, Data Processing, Compressibility, Plasma Waves

Scientific paper

This brief report discusses the data processing accomplishments and the scientific results from this grant for the stated activity period. All the data received from ARC were processed up to the final orbit 5055. This processing included both the experiment data records and the supplemental experiment data records. The processed data that we have been submitting to NSSDC were also submitted up to orbit 5055. This included the 13 second UADS data for the hour around periapsis and the full resolution data for the one-hour period around periapsis. We also completed copying both the EDR and SEDR data to 6250 bpi tapes for our files and copied these two data sets to 12 inch OPTIMEM optical platters for submittal to NSSDC. We created the first CDROMS of the full processed OMAG data set. Finally we completed the microfiching of data plots to orbit 1500 and fulfilled data requests for numerous researchers. The scientific research efforts of four graduate students are highlighted in this article and a listing of the published papers, invited papers, and presentations at meetings are listed.

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