title: New results for the space radiation environment of MIR space station obtained by Liulin dosimeter-radiometer.  Comparison with LET spectrometer NAUSICAA.
abstract: Since 1988 high sensitivity semiconductor dosimeter-radiometer "Liulin" worked on board of MIR space station. Device measured the absorbed dose rate and the flux of penetrating particles. The analysis of the data shows the following new results: In October 1989 and after March 24, 1991, two additional stable maximums in flux channel were observed in the southern-eastern part of South Atlantic Anomaly (SAA). These two maximums existed at least several months and seem to be due to trapped high energy electron and proton fluxes. In April 1991 additional maximums were localized in the following geographical coordinates regions: latitude = (-35 degrees)-(-50 degrees) longitude = 332 degrees-l6 degrees and lat.(-46 degrees)-(-52 degrees) long. 360 degrees-60 degrees. Additional maximums diffusion occurs inside radiation belt. Appearance of these maximums seems to be closely connected with preceding powerful solar proton events and associated geomagnetic dynamics of new belt disturbances. Alter the series of solar proton events in June 1991 we observed significant enhancement of this new radiation belt formation. To achieve sufficient accuracy of dose rate predictions in low Earth orbits the structure and dynamics of new belt should be carefully analyzed to be included in a new environment model. From the inter comparison of the data from "Liulin" and French developed tissue equivalent LET spectrometer NAUSICAA in the time period August-November 1992 we come to the following conclusions: Mainly there is good agreement between both data sets for absorbed dose in the region of SAA; Different situation of the instruments on the station can explain the cases when differences up to 2 times are observed;  At high latitudes usually the tissue equivalent absorbed dose observations are 2 times larger than "Liulin" doses.
authors.affiliation: Solar-Terrestrial Influences Laboratory, Sofia, Bulgaria.
authors.lastname: Dachev TsP
authors.forename: J V
authors.initials: JV
authors.lastname: Semkova
authors.lastname: Matviichuk YuN
authors.forename: R T
authors.initials: RT
authors.lastname: Koleva
authors.forename: B T
authors.initials: BT
authors.lastname: Tomov
authors.forename: P T
authors.initials: PT
authors.lastname: Baynov
authors.forename: J F
authors.initials: JF
authors.lastname: Bottollier-Depois
authors.forename: V D
authors.initials: VD
authors.lastname: Nguen
authors.forename: L
authors.initials: L
authors.lastname: Lebaron-Jacobs
authors.forename: M
authors.initials: M
authors.lastname: Siegrist
authors.forename: E
authors.initials: E
authors.lastname: Duvivier
authors.forename: B
authors.initials: B
authors.lastname: Almarcha
authors.forename: V M
authors.initials: VM
authors.lastname: Petrov
authors.forename: V V
authors.initials: VV
authors.lastname: Shurshakov
mesh_terms: D001267:Atlantic Ocean; D018499:Linear Energy Transfer; D011522:Protons; D011829:Radiation Dosage; D011834:Radiation Monitoring / Q000295:instrumentation*; D019445:Solar Activity; D013020:South America; D018531:Spacecraft / Q000295:instrumentation*
chemical_list: D011522:Protons