| LDR | 02808cam a2200505Ii 4500 | ||
| 001 | 102326064 | ||
| 003 | MiAaHDL | ||
| 005 | 20220618000000.0 | ||
| 006 | m d | ||
| 007 | cr bn ---auaua | ||
| 008 | 090528e198601 maua bt f000 0 eng d | ||
| 035 | ⊔ | ⊔ | ‡a(MiU)990161180450106381 |
| 035 | ⊔ | ⊔ | ‡asdr-miu.990161180450106381 |
| 035 | ⊔ | ⊔ | ‡z(MiU)MIU01000000000000016118045-goog |
| 035 | ⊔ | ⊔ | ‡a(OCoLC)356064320 |
| 035 | ⊔ | ⊔ | ‡z(MiU)Aleph016118045 |
| 040 | ⊔ | ⊔ | ‡aLHL ‡beng ‡cLHL ‡dOCLCF ‡dOCLCO ‡dOCLCQ ‡dTRAAL |
| 049 | ⊔ | ⊔ | ‡aMAIN |
| 086 | 0 | ⊔ | ‡aD 301.45/39:945 |
| 088 | ⊔ | ⊔ | ‡aADA 172276 |
| 088 | ⊔ | ⊔ | ‡aAFGL TR 86-23 |
| 100 | 1 | ⊔ | ‡aHeinemann, Michael. |
| 245 | 1 | 0 | ‡aShuttle contamination modeling : ‡bEvolution of ionized shuttle exhaust / ‡cMichael Heinemann. |
| 264 | ⊔ | 1 | ‡aHanscom AFB, Massachusetts : ‡bAir Force Geophysics Laboratory, Air Force Systems Command, United States Air Force, ‡c1986. |
| 300 | ⊔ | ⊔ | ‡aiii, 27 pages : ‡billustrations ; ‡c28 cm. |
| 336 | ⊔ | ⊔ | ‡atext ‡btxt ‡2rdacontent |
| 337 | ⊔ | ⊔ | ‡aunmediated ‡bn ‡2rdamedia |
| 338 | ⊔ | ⊔ | ‡avolume ‡bnc ‡2rdacarrier |
| 490 | 0 | ⊔ | ‡aEnvironmental Research Papers ; ‡vNo. 945 |
| 490 | 0 | ⊔ | ‡aAFGL TR ; ‡v86-23 |
| 500 | ⊔ | ⊔ | ‡aResearch supported by the Air Force Geophysics Laboratory, United States Air Force, Hanscom AFB, Massachusetts. |
| 500 | ⊔ | ⊔ | ‡aSpace Physics Division Project 7661. |
| 500 | ⊔ | ⊔ | ‡aADA172276 (from http://www.dtic.mi). |
| 500 | ⊔ | ⊔ | ‡a"22 January 1986." |
| 504 | ⊔ | ⊔ | ‡aIncludes bibliographical references (page 27). |
| 520 | ⊔ | ⊔ | ‡aWe consider the evolution of ionized Shuttle exhaust. While the source of ionization is not treated, the subsequent evolution can be understood in a certain amount of detail. The fundamental conclusion are that: (1) Low-density ions expand with neutral exhaust for about 100 m where they go through a rapid transition to collisionless behavior and then are swept away (in the Shuttle frame of reference) by the magnetic field, and radially away from the Shuttle: neither the ambient ionosphere nor the geomagnetic field can significantly change this behavior. The details of the evolution can be affected by low-level (approx. 0.1 mV/m) parallel electric fields. The mirror force associated with the geomagnetic field is to weak to have any effect. |
| 538 | ⊔ | ⊔ | ‡aMode of access: Internet. |
| 650 | ⊔ | 7 | ‡aSpace vehicles ‡xContamination ‡xMathematical models. ‡2fast ‡0(OCoLC)fst01127978 |
| 650 | ⊔ | 7 | ‡aSpace plasmas. ‡2fast ‡0(OCoLC)fst01127789 |
| 650 | ⊔ | 7 | ‡aSpace environment. ‡2fast ‡0(OCoLC)fst01127673 |
| 650 | ⊔ | 7 | ‡aMagnetic fields. ‡2fast ‡0(OCoLC)fst01005694 |
| 650 | ⊔ | 7 | ‡aGeomagnetism. ‡2fast ‡0(OCoLC)fst00940796 |
| 650 | ⊔ | 0 | ‡aMagnetic fields. |
| 650 | ⊔ | 0 | ‡aGeomagnetism. |
| 650 | ⊔ | 0 | ‡aSpace vehicles ‡xContamination ‡xMathematical models. |
| 650 | ⊔ | 0 | ‡aSpace environment. |
| 650 | ⊔ | 0 | ‡aSpace plasmas. |
| 710 | 2 | ⊔ | ‡aU.S. Air Force Geophysics Laboratory. |
| 730 | 0 | ⊔ | ‡aTechnical Report Archive & Image Library (TRAIL) |
| 899 | ⊔ | ⊔ | ‡a39015095141159 |
| CID | ⊔ | ⊔ | ‡a102326064 |
| DAT | 0 | ⊔ | ‡b20220618000000.0 |
| DAT | 1 | ⊔ | ‡a20220619060753.0 ‡b2024-04-27T17:32:23Z |
| DAT | 2 | ⊔ | ‡a2024-04-27T17:30:02Z |
| CAT | ⊔ | ⊔ | ‡aSDR-MIU ‡dALMA ‡lprepare.pl-004-008 |
| FMT | ⊔ | ⊔ | ‡aBK |
| HOL | ⊔ | ⊔ | ‡0sdr-miu.990161180450106381 ‡aMiU ‡bSDR ‡cGWLA ‡pmdp.39015095141159 ‡sMIU ‡1990161180450106381 |
| 974 | ⊔ | ⊔ | ‡bMIU ‡cGWLA ‡d20240427 ‡sgoogle ‡umdp.39015095141159 ‡y1986 ‡rpd ‡qbib ‡tUS fed doc |