Relativistic electron precipitation bands in the outside radiation environment of the International space station
The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify t...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Dachev, Tsvetan P. [verfasserIn] |
|---|
| Format: |
E-Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2018transfer abstract |
|---|
| Schlagwörter: |
|---|
| Umfang: |
10 |
|---|
| Übergeordnetes Werk: |
Enthalten in: List of Referees - 2014, Amsterdam [u.a.] |
|---|---|
| Übergeordnetes Werk: |
volume:177 ; year:2018 ; pages:247-256 ; extent:10 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.jastp.2017.11.008 |
|---|
| Katalog-ID: |
ELV043947751 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | ELV043947751 | ||
| 003 | DE-627 | ||
| 005 | 20230626004411.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 181113s2018 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1016/j.jastp.2017.11.008 |2 doi | |
| 028 | 5 | 2 | |a /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001002.pica |
| 035 | |a (DE-627)ELV043947751 | ||
| 035 | |a (ELSEVIER)S1364-6826(17)30276-6 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 082 | 0 | 4 | |a 520 |q VZ |
| 082 | 0 | 4 | |a 620 |q VZ |
| 082 | 0 | 4 | |a 610 |a 570 |q VZ |
| 084 | |a 44.89 |2 bkl | ||
| 100 | 1 | |a Dachev, Tsvetan P. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Relativistic electron precipitation bands in the outside radiation environment of the International space station |
| 264 | 1 | |c 2018transfer abstract | |
| 300 | |a 10 | ||
| 336 | |a nicht spezifiziert |b zzz |2 rdacontent | ||
| 337 | |a nicht spezifiziert |b z |2 rdamedia | ||
| 338 | |a nicht spezifiziert |b zu |2 rdacarrier | ||
| 520 | |a The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. | ||
| 520 | |a The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. | ||
| 650 | 7 | |a Relativistic electrons |2 Elsevier | |
| 650 | 7 | |a Outer radiation belt |2 Elsevier | |
| 650 | 7 | |a ISS |2 Elsevier | |
| 650 | 7 | |a Space radiation dosimetry |2 Elsevier | |
| 773 | 0 | 8 | |i Enthalten in |n Elsevier Science |t List of Referees |d 2014 |g Amsterdam [u.a.] |w (DE-627)ELV017414210 |
| 773 | 1 | 8 | |g volume:177 |g year:2018 |g pages:247-256 |g extent:10 |
| 856 | 4 | 0 | |u https://doi.org/10.1016/j.jastp.2017.11.008 |3 Volltext |
| 912 | |a GBV_USEFLAG_U | ||
| 912 | |a GBV_ELV | ||
| 912 | |a SYSFLAG_U | ||
| 912 | |a SSG-OLC-PHA | ||
| 912 | |a GBV_ILN_63 | ||
| 912 | |a GBV_ILN_70 | ||
| 936 | b | k | |a 44.89 |j Endokrinologie |q VZ |
| 951 | |a AR | ||
| 952 | |d 177 |j 2018 |h 247-256 |g 10 | ||
| author_variant |
t p d tp tpd |
|---|---|
| matchkey_str |
dachevtsvetanp:2018----:eaiitclcrnrcpttobnsnhotieaitoevrnetfh |
| hierarchy_sort_str |
2018transfer abstract |
| bklnumber |
44.89 |
| publishDate |
2018 |
| allfields |
10.1016/j.jastp.2017.11.008 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001002.pica (DE-627)ELV043947751 (ELSEVIER)S1364-6826(17)30276-6 DE-627 ger DE-627 rakwb eng 520 VZ 620 VZ 610 570 VZ 44.89 bkl Dachev, Tsvetan P. verfasserin aut Relativistic electron precipitation bands in the outside radiation environment of the International space station 2018transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. Relativistic electrons Elsevier Outer radiation belt Elsevier ISS Elsevier Space radiation dosimetry Elsevier Enthalten in Elsevier Science List of Referees 2014 Amsterdam [u.a.] (DE-627)ELV017414210 volume:177 year:2018 pages:247-256 extent:10 https://doi.org/10.1016/j.jastp.2017.11.008 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 44.89 Endokrinologie VZ AR 177 2018 247-256 10 |
| spelling |
10.1016/j.jastp.2017.11.008 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001002.pica (DE-627)ELV043947751 (ELSEVIER)S1364-6826(17)30276-6 DE-627 ger DE-627 rakwb eng 520 VZ 620 VZ 610 570 VZ 44.89 bkl Dachev, Tsvetan P. verfasserin aut Relativistic electron precipitation bands in the outside radiation environment of the International space station 2018transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. Relativistic electrons Elsevier Outer radiation belt Elsevier ISS Elsevier Space radiation dosimetry Elsevier Enthalten in Elsevier Science List of Referees 2014 Amsterdam [u.a.] (DE-627)ELV017414210 volume:177 year:2018 pages:247-256 extent:10 https://doi.org/10.1016/j.jastp.2017.11.008 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 44.89 Endokrinologie VZ AR 177 2018 247-256 10 |
| allfields_unstemmed |
10.1016/j.jastp.2017.11.008 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001002.pica (DE-627)ELV043947751 (ELSEVIER)S1364-6826(17)30276-6 DE-627 ger DE-627 rakwb eng 520 VZ 620 VZ 610 570 VZ 44.89 bkl Dachev, Tsvetan P. verfasserin aut Relativistic electron precipitation bands in the outside radiation environment of the International space station 2018transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. Relativistic electrons Elsevier Outer radiation belt Elsevier ISS Elsevier Space radiation dosimetry Elsevier Enthalten in Elsevier Science List of Referees 2014 Amsterdam [u.a.] (DE-627)ELV017414210 volume:177 year:2018 pages:247-256 extent:10 https://doi.org/10.1016/j.jastp.2017.11.008 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 44.89 Endokrinologie VZ AR 177 2018 247-256 10 |
| allfieldsGer |
10.1016/j.jastp.2017.11.008 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001002.pica (DE-627)ELV043947751 (ELSEVIER)S1364-6826(17)30276-6 DE-627 ger DE-627 rakwb eng 520 VZ 620 VZ 610 570 VZ 44.89 bkl Dachev, Tsvetan P. verfasserin aut Relativistic electron precipitation bands in the outside radiation environment of the International space station 2018transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. Relativistic electrons Elsevier Outer radiation belt Elsevier ISS Elsevier Space radiation dosimetry Elsevier Enthalten in Elsevier Science List of Referees 2014 Amsterdam [u.a.] (DE-627)ELV017414210 volume:177 year:2018 pages:247-256 extent:10 https://doi.org/10.1016/j.jastp.2017.11.008 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 44.89 Endokrinologie VZ AR 177 2018 247-256 10 |
| allfieldsSound |
10.1016/j.jastp.2017.11.008 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001002.pica (DE-627)ELV043947751 (ELSEVIER)S1364-6826(17)30276-6 DE-627 ger DE-627 rakwb eng 520 VZ 620 VZ 610 570 VZ 44.89 bkl Dachev, Tsvetan P. verfasserin aut Relativistic electron precipitation bands in the outside radiation environment of the International space station 2018transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. Relativistic electrons Elsevier Outer radiation belt Elsevier ISS Elsevier Space radiation dosimetry Elsevier Enthalten in Elsevier Science List of Referees 2014 Amsterdam [u.a.] (DE-627)ELV017414210 volume:177 year:2018 pages:247-256 extent:10 https://doi.org/10.1016/j.jastp.2017.11.008 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 44.89 Endokrinologie VZ AR 177 2018 247-256 10 |
| language |
English |
| source |
Enthalten in List of Referees Amsterdam [u.a.] volume:177 year:2018 pages:247-256 extent:10 |
| sourceStr |
Enthalten in List of Referees Amsterdam [u.a.] volume:177 year:2018 pages:247-256 extent:10 |
| format_phy_str_mv |
Article |
| bklname |
Endokrinologie |
| institution |
findex.gbv.de |
| topic_facet |
Relativistic electrons Outer radiation belt ISS Space radiation dosimetry |
| dewey-raw |
520 |
| isfreeaccess_bool |
false |
| container_title |
List of Referees |
| authorswithroles_txt_mv |
Dachev, Tsvetan P. @@aut@@ |
| publishDateDaySort_date |
2018-01-01T00:00:00Z |
| hierarchy_top_id |
ELV017414210 |
| dewey-sort |
3520 |
| id |
ELV043947751 |
| language_de |
englisch |
| fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV043947751</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230626004411.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">181113s2018 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.jastp.2017.11.008</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">/cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001002.pica</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV043947751</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S1364-6826(17)30276-6</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">610</subfield><subfield code="a">570</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">44.89</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Dachev, Tsvetan P.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Relativistic electron precipitation bands in the outside radiation environment of the International space station</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2018transfer abstract</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">10</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Relativistic electrons</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Outer radiation belt</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">ISS</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Space radiation dosimetry</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="n">Elsevier Science</subfield><subfield code="t">List of Referees</subfield><subfield code="d">2014</subfield><subfield code="g">Amsterdam [u.a.]</subfield><subfield code="w">(DE-627)ELV017414210</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:177</subfield><subfield code="g">year:2018</subfield><subfield code="g">pages:247-256</subfield><subfield code="g">extent:10</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1016/j.jastp.2017.11.008</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ELV</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHA</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_63</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="936" ind1="b" ind2="k"><subfield code="a">44.89</subfield><subfield code="j">Endokrinologie</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">177</subfield><subfield code="j">2018</subfield><subfield code="h">247-256</subfield><subfield code="g">10</subfield></datafield></record></collection>
|
| author |
Dachev, Tsvetan P. |
| spellingShingle |
Dachev, Tsvetan P. ddc 520 ddc 620 ddc 610 bkl 44.89 Elsevier Relativistic electrons Elsevier Outer radiation belt Elsevier ISS Elsevier Space radiation dosimetry Relativistic electron precipitation bands in the outside radiation environment of the International space station |
| authorStr |
Dachev, Tsvetan P. |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)ELV017414210 |
| format |
electronic Article |
| dewey-ones |
520 - Astronomy & allied sciences 620 - Engineering & allied operations 610 - Medicine & health 570 - Life sciences; biology |
| delete_txt_mv |
keep |
| author_role |
aut |
| collection |
elsevier |
| remote_str |
true |
| illustrated |
Not Illustrated |
| topic_title |
520 VZ 620 VZ 610 570 VZ 44.89 bkl Relativistic electron precipitation bands in the outside radiation environment of the International space station Relativistic electrons Elsevier Outer radiation belt Elsevier ISS Elsevier Space radiation dosimetry Elsevier |
| topic |
ddc 520 ddc 620 ddc 610 bkl 44.89 Elsevier Relativistic electrons Elsevier Outer radiation belt Elsevier ISS Elsevier Space radiation dosimetry |
| topic_unstemmed |
ddc 520 ddc 620 ddc 610 bkl 44.89 Elsevier Relativistic electrons Elsevier Outer radiation belt Elsevier ISS Elsevier Space radiation dosimetry |
| topic_browse |
ddc 520 ddc 620 ddc 610 bkl 44.89 Elsevier Relativistic electrons Elsevier Outer radiation belt Elsevier ISS Elsevier Space radiation dosimetry |
| format_facet |
Elektronische Aufsätze Aufsätze Elektronische Ressource |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
zu |
| hierarchy_parent_title |
List of Referees |
| hierarchy_parent_id |
ELV017414210 |
| dewey-tens |
520 - Astronomy 620 - Engineering 610 - Medicine & health 570 - Life sciences; biology |
| hierarchy_top_title |
List of Referees |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)ELV017414210 |
| title |
Relativistic electron precipitation bands in the outside radiation environment of the International space station |
| ctrlnum |
(DE-627)ELV043947751 (ELSEVIER)S1364-6826(17)30276-6 |
| title_full |
Relativistic electron precipitation bands in the outside radiation environment of the International space station |
| author_sort |
Dachev, Tsvetan P. |
| journal |
List of Referees |
| journalStr |
List of Referees |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
500 - Science 600 - Technology |
| recordtype |
marc |
| publishDateSort |
2018 |
| contenttype_str_mv |
zzz |
| container_start_page |
247 |
| author_browse |
Dachev, Tsvetan P. |
| container_volume |
177 |
| physical |
10 |
| class |
520 VZ 620 VZ 610 570 VZ 44.89 bkl |
| format_se |
Elektronische Aufsätze |
| author-letter |
Dachev, Tsvetan P. |
| doi_str_mv |
10.1016/j.jastp.2017.11.008 |
| dewey-full |
520 620 610 570 |
| title_sort |
relativistic electron precipitation bands in the outside radiation environment of the international space station |
| title_auth |
Relativistic electron precipitation bands in the outside radiation environment of the International space station |
| abstract |
The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. |
| abstractGer |
The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. |
| abstract_unstemmed |
The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations. |
| collection_details |
GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_63 GBV_ILN_70 |
| title_short |
Relativistic electron precipitation bands in the outside radiation environment of the International space station |
| url |
https://doi.org/10.1016/j.jastp.2017.11.008 |
| remote_bool |
true |
| ppnlink |
ELV017414210 |
| mediatype_str_mv |
z |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| doi_str |
10.1016/j.jastp.2017.11.008 |
| up_date |
2024-07-06T20:10:56.010Z |
| _version_ |
1803861786372341760 |
| fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV043947751</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230626004411.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">181113s2018 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.jastp.2017.11.008</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">/cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001002.pica</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV043947751</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S1364-6826(17)30276-6</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">620</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">610</subfield><subfield code="a">570</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">44.89</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Dachev, Tsvetan P.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Relativistic electron precipitation bands in the outside radiation environment of the International space station</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2018transfer abstract</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">10</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The Radiation risk radiometer-dosimeter (R3DR2) performed active dosimetry measurements outside the International space station (ISS) during the ESA EXPOSE-R2 missions from October 24, 2014 until January 11, 2016. The 10 s resolution flux and dose rate data were used to find, identify and classify the relativistic electron precipitation bands (PB) (Blake et al., 1996) in the outside radiation environment of the ISS. The PB were identified as rapid (10–40-s) dose rate enhancement from the normal (20–200 μGy h−1) outer radiation belt (ORB) level and similar fast return to the same low level. Only PB that have in the time profile dose rates larger than 10,000 μGy h−1, identical to flux larger than 4000 cm−2 s−1, for 10 or more seconds were selected. Sixteen PB were studied. The largest selected PB, delivered in the R3DR2 detector, which was behind 0.3 g cm−2 shielding, a dose of 464 μGy for 70 s. The later was larger than the ORB daily average dose rates for 366 days out of 442 days measurements during the analyzed period. The daily average doses inside of the ISS were measured, using the DOSTEL instrument, at an average level of 194 μGy d−1 (Reitz et al., 2005). This indicates that only for 70 s, the cosmonaut/astronaut, being on extra vehicular activity (EVA), where they are shielded only by their space suits, will accumulate the equivalent of about 2.5-days dose inside of the ISS. Only 1 PB was identified during the ESA EXPOSE-E mission on ISS in the period February 17, 2008–September 3, 2009, while in the more active geo-magnetically EXPOSE-R mission in 2010, 6 PB were registered. Although the obtained PB doses do not pose extreme risks for cosmonauts/astronauts health, being on EVA, they have to be considered as a possible extremely high dose rate source, which requires additional comprehensive investigations.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Relativistic electrons</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Outer radiation belt</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">ISS</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Space radiation dosimetry</subfield><subfield code="2">Elsevier</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="n">Elsevier Science</subfield><subfield code="t">List of Referees</subfield><subfield code="d">2014</subfield><subfield code="g">Amsterdam [u.a.]</subfield><subfield code="w">(DE-627)ELV017414210</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:177</subfield><subfield code="g">year:2018</subfield><subfield code="g">pages:247-256</subfield><subfield code="g">extent:10</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1016/j.jastp.2017.11.008</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ELV</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHA</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_63</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="936" ind1="b" ind2="k"><subfield code="a">44.89</subfield><subfield code="j">Endokrinologie</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">177</subfield><subfield code="j">2018</subfield><subfield code="h">247-256</subfield><subfield code="g">10</subfield></datafield></record></collection>
|
| score |
7.4015865 |