Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015
Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions t...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Garrett, Henry B [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2016 |
|---|
| Rechteinformationen: |
Nutzungsrecht: Copyright © 2016 by the American Institute of Aeronautics and Astronautics, Inc. The U.S. Government has a royalty-free license to exercise all rights under the copyright claimed herein for Governmental purposes. All other rights are reserved by the copyright owner. Copies of this paper may be made for personal and internal use, on condition that the copier pay the per-copy fee to the Copyright Clearance Center (CCC). All requests for copying and permission to reprint should be submitted to CCC at ; employ the ISSN (print) or (online) to initiate your request. |
|---|
| Übergeordnetes Werk: |
Enthalten in: Journal of spacecraft and rockets - Reston, Va. [u.a.] : Inst., 1964, (2016), Seite 693-707 |
|---|---|
| Übergeordnetes Werk: |
year:2016 ; pages:693-707 |
| Links: |
|---|
| DOI / URN: |
10.2514/1.A33510 |
|---|
| Katalog-ID: |
OLC1979800677 |
|---|
| LEADER | 01000caa a2200265 4500 | ||
|---|---|---|---|
| 001 | OLC1979800677 | ||
| 003 | DE-627 | ||
| 005 | 20230714204040.0 | ||
| 007 | tu | ||
| 008 | 160816s2016 xx ||||| 00| ||eng c | ||
| 024 | 7 | |a 10.2514/1.A33510 |2 doi | |
| 028 | 5 | 2 | |a PQ20160815 |
| 035 | |a (DE-627)OLC1979800677 | ||
| 035 | |a (DE-599)GBVOLC1979800677 | ||
| 035 | |a (PRQ)a630-464df68111628d4f4d381a313217f99afa5c40ad33e9a312ec3198b3ffa663820 | ||
| 035 | |a (KEY)0013696420160000000000000693updatingthejovianplasmaandradiationenvironmentsthe | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 082 | 0 | 4 | |a 380 |a 620 |q DNB |
| 100 | 1 | |a Garrett, Henry B |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 |
| 264 | 1 | |c 2016 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
| 338 | |a Band |b nc |2 rdacarrier | ||
| 520 | |a Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept. | ||
| 540 | |a Nutzungsrecht: Copyright © 2016 by the American Institute of Aeronautics and Astronautics, Inc. The U.S. Government has a royalty-free license to exercise all rights under the copyright claimed herein for Governmental purposes. All other rights are reserved by the copyright owner. Copies of this paper may be made for personal and internal use, on condition that the copier pay the per-copy fee to the Copyright Clearance Center (CCC). All requests for copying and permission to reprint should be submitted to CCC at ; employ the ISSN (print) or (online) to initiate your request. | ||
| 700 | 1 | |a Kim, Wousik |4 oth | |
| 700 | 1 | |a Evans, Robin W |4 oth | |
| 773 | 0 | 8 | |i Enthalten in |t Journal of spacecraft and rockets |d Reston, Va. [u.a.] : Inst., 1964 |g (2016), Seite 693-707 |w (DE-627)129359114 |w (DE-600)160513-6 |w (DE-576)014731444 |x 0022-4650 |7 nnns |
| 773 | 1 | 8 | |g year:2016 |g pages:693-707 |
| 856 | 4 | 1 | |u http://dx.doi.org/10.2514/1.A33510 |3 Volltext |
| 856 | 4 | 2 | |u http://arc.aiaa.org/doi/full/10.2514/1.A33510 |
| 912 | |a GBV_USEFLAG_A | ||
| 912 | |a SYSFLAG_A | ||
| 912 | |a GBV_OLC | ||
| 912 | |a SSG-OLC-TEC | ||
| 912 | |a SSG-OPC-AST | ||
| 912 | |a GBV_ILN_22 | ||
| 912 | |a GBV_ILN_70 | ||
| 912 | |a GBV_ILN_2006 | ||
| 912 | |a GBV_ILN_4046 | ||
| 912 | |a GBV_ILN_4700 | ||
| 951 | |a AR | ||
| 952 | |j 2016 |h 693-707 | ||
| author_variant |
h b g hb hbg |
|---|---|
| matchkey_str |
article:00224650:2016----::paighjvapamadaitoevrnette |
| hierarchy_sort_str |
2016 |
| publishDate |
2016 |
| allfields |
10.2514/1.A33510 doi PQ20160815 (DE-627)OLC1979800677 (DE-599)GBVOLC1979800677 (PRQ)a630-464df68111628d4f4d381a313217f99afa5c40ad33e9a312ec3198b3ffa663820 (KEY)0013696420160000000000000693updatingthejovianplasmaandradiationenvironmentsthe DE-627 ger DE-627 rakwb eng 380 620 DNB Garrett, Henry B verfasserin aut Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept. Nutzungsrecht: Copyright © 2016 by the American Institute of Aeronautics and Astronautics, Inc. The U.S. Government has a royalty-free license to exercise all rights under the copyright claimed herein for Governmental purposes. All other rights are reserved by the copyright owner. Copies of this paper may be made for personal and internal use, on condition that the copier pay the per-copy fee to the Copyright Clearance Center (CCC). All requests for copying and permission to reprint should be submitted to CCC at ; employ the ISSN (print) or (online) to initiate your request. Kim, Wousik oth Evans, Robin W oth Enthalten in Journal of spacecraft and rockets Reston, Va. [u.a.] : Inst., 1964 (2016), Seite 693-707 (DE-627)129359114 (DE-600)160513-6 (DE-576)014731444 0022-4650 nnns year:2016 pages:693-707 http://dx.doi.org/10.2514/1.A33510 Volltext http://arc.aiaa.org/doi/full/10.2514/1.A33510 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OPC-AST GBV_ILN_22 GBV_ILN_70 GBV_ILN_2006 GBV_ILN_4046 GBV_ILN_4700 AR 2016 693-707 |
| spelling |
10.2514/1.A33510 doi PQ20160815 (DE-627)OLC1979800677 (DE-599)GBVOLC1979800677 (PRQ)a630-464df68111628d4f4d381a313217f99afa5c40ad33e9a312ec3198b3ffa663820 (KEY)0013696420160000000000000693updatingthejovianplasmaandradiationenvironmentsthe DE-627 ger DE-627 rakwb eng 380 620 DNB Garrett, Henry B verfasserin aut Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept. Nutzungsrecht: Copyright © 2016 by the American Institute of Aeronautics and Astronautics, Inc. The U.S. Government has a royalty-free license to exercise all rights under the copyright claimed herein for Governmental purposes. All other rights are reserved by the copyright owner. Copies of this paper may be made for personal and internal use, on condition that the copier pay the per-copy fee to the Copyright Clearance Center (CCC). All requests for copying and permission to reprint should be submitted to CCC at ; employ the ISSN (print) or (online) to initiate your request. Kim, Wousik oth Evans, Robin W oth Enthalten in Journal of spacecraft and rockets Reston, Va. [u.a.] : Inst., 1964 (2016), Seite 693-707 (DE-627)129359114 (DE-600)160513-6 (DE-576)014731444 0022-4650 nnns year:2016 pages:693-707 http://dx.doi.org/10.2514/1.A33510 Volltext http://arc.aiaa.org/doi/full/10.2514/1.A33510 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OPC-AST GBV_ILN_22 GBV_ILN_70 GBV_ILN_2006 GBV_ILN_4046 GBV_ILN_4700 AR 2016 693-707 |
| allfields_unstemmed |
10.2514/1.A33510 doi PQ20160815 (DE-627)OLC1979800677 (DE-599)GBVOLC1979800677 (PRQ)a630-464df68111628d4f4d381a313217f99afa5c40ad33e9a312ec3198b3ffa663820 (KEY)0013696420160000000000000693updatingthejovianplasmaandradiationenvironmentsthe DE-627 ger DE-627 rakwb eng 380 620 DNB Garrett, Henry B verfasserin aut Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept. Nutzungsrecht: Copyright © 2016 by the American Institute of Aeronautics and Astronautics, Inc. The U.S. Government has a royalty-free license to exercise all rights under the copyright claimed herein for Governmental purposes. All other rights are reserved by the copyright owner. Copies of this paper may be made for personal and internal use, on condition that the copier pay the per-copy fee to the Copyright Clearance Center (CCC). All requests for copying and permission to reprint should be submitted to CCC at ; employ the ISSN (print) or (online) to initiate your request. Kim, Wousik oth Evans, Robin W oth Enthalten in Journal of spacecraft and rockets Reston, Va. [u.a.] : Inst., 1964 (2016), Seite 693-707 (DE-627)129359114 (DE-600)160513-6 (DE-576)014731444 0022-4650 nnns year:2016 pages:693-707 http://dx.doi.org/10.2514/1.A33510 Volltext http://arc.aiaa.org/doi/full/10.2514/1.A33510 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OPC-AST GBV_ILN_22 GBV_ILN_70 GBV_ILN_2006 GBV_ILN_4046 GBV_ILN_4700 AR 2016 693-707 |
| allfieldsGer |
10.2514/1.A33510 doi PQ20160815 (DE-627)OLC1979800677 (DE-599)GBVOLC1979800677 (PRQ)a630-464df68111628d4f4d381a313217f99afa5c40ad33e9a312ec3198b3ffa663820 (KEY)0013696420160000000000000693updatingthejovianplasmaandradiationenvironmentsthe DE-627 ger DE-627 rakwb eng 380 620 DNB Garrett, Henry B verfasserin aut Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept. Nutzungsrecht: Copyright © 2016 by the American Institute of Aeronautics and Astronautics, Inc. The U.S. Government has a royalty-free license to exercise all rights under the copyright claimed herein for Governmental purposes. All other rights are reserved by the copyright owner. Copies of this paper may be made for personal and internal use, on condition that the copier pay the per-copy fee to the Copyright Clearance Center (CCC). All requests for copying and permission to reprint should be submitted to CCC at ; employ the ISSN (print) or (online) to initiate your request. Kim, Wousik oth Evans, Robin W oth Enthalten in Journal of spacecraft and rockets Reston, Va. [u.a.] : Inst., 1964 (2016), Seite 693-707 (DE-627)129359114 (DE-600)160513-6 (DE-576)014731444 0022-4650 nnns year:2016 pages:693-707 http://dx.doi.org/10.2514/1.A33510 Volltext http://arc.aiaa.org/doi/full/10.2514/1.A33510 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OPC-AST GBV_ILN_22 GBV_ILN_70 GBV_ILN_2006 GBV_ILN_4046 GBV_ILN_4700 AR 2016 693-707 |
| allfieldsSound |
10.2514/1.A33510 doi PQ20160815 (DE-627)OLC1979800677 (DE-599)GBVOLC1979800677 (PRQ)a630-464df68111628d4f4d381a313217f99afa5c40ad33e9a312ec3198b3ffa663820 (KEY)0013696420160000000000000693updatingthejovianplasmaandradiationenvironmentsthe DE-627 ger DE-627 rakwb eng 380 620 DNB Garrett, Henry B verfasserin aut Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept. Nutzungsrecht: Copyright © 2016 by the American Institute of Aeronautics and Astronautics, Inc. The U.S. Government has a royalty-free license to exercise all rights under the copyright claimed herein for Governmental purposes. All other rights are reserved by the copyright owner. Copies of this paper may be made for personal and internal use, on condition that the copier pay the per-copy fee to the Copyright Clearance Center (CCC). All requests for copying and permission to reprint should be submitted to CCC at ; employ the ISSN (print) or (online) to initiate your request. Kim, Wousik oth Evans, Robin W oth Enthalten in Journal of spacecraft and rockets Reston, Va. [u.a.] : Inst., 1964 (2016), Seite 693-707 (DE-627)129359114 (DE-600)160513-6 (DE-576)014731444 0022-4650 nnns year:2016 pages:693-707 http://dx.doi.org/10.2514/1.A33510 Volltext http://arc.aiaa.org/doi/full/10.2514/1.A33510 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OPC-AST GBV_ILN_22 GBV_ILN_70 GBV_ILN_2006 GBV_ILN_4046 GBV_ILN_4700 AR 2016 693-707 |
| language |
English |
| source |
Enthalten in Journal of spacecraft and rockets (2016), Seite 693-707 year:2016 pages:693-707 |
| sourceStr |
Enthalten in Journal of spacecraft and rockets (2016), Seite 693-707 year:2016 pages:693-707 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| dewey-raw |
380 |
| isfreeaccess_bool |
false |
| container_title |
Journal of spacecraft and rockets |
| authorswithroles_txt_mv |
Garrett, Henry B @@aut@@ Kim, Wousik @@oth@@ Evans, Robin W @@oth@@ |
| publishDateDaySort_date |
2016-01-01T00:00:00Z |
| hierarchy_top_id |
129359114 |
| dewey-sort |
3380 |
| id |
OLC1979800677 |
| language_de |
englisch |
| fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">OLC1979800677</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230714204040.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">160816s2016 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.2514/1.A33510</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">PQ20160815</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC1979800677</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVOLC1979800677</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(PRQ)a630-464df68111628d4f4d381a313217f99afa5c40ad33e9a312ec3198b3ffa663820</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(KEY)0013696420160000000000000693updatingthejovianplasmaandradiationenvironmentsthe</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">380</subfield><subfield code="a">620</subfield><subfield code="q">DNB</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Garrett, Henry B</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2016</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept.</subfield></datafield><datafield tag="540" ind1=" " ind2=" "><subfield code="a">Nutzungsrecht: Copyright © 2016 by the American Institute of Aeronautics and Astronautics, Inc. The U.S. Government has a royalty-free license to exercise all rights under the copyright claimed herein for Governmental purposes. All other rights are reserved by the copyright owner. Copies of this paper may be made for personal and internal use, on condition that the copier pay the per-copy fee to the Copyright Clearance Center (CCC). All requests for copying and permission to reprint should be submitted to CCC at ; employ the ISSN (print) or (online) to initiate your request.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, Wousik</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Evans, Robin W</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Journal of spacecraft and rockets</subfield><subfield code="d">Reston, Va. [u.a.] : Inst., 1964</subfield><subfield code="g">(2016), Seite 693-707</subfield><subfield code="w">(DE-627)129359114</subfield><subfield code="w">(DE-600)160513-6</subfield><subfield code="w">(DE-576)014731444</subfield><subfield code="x">0022-4650</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">year:2016</subfield><subfield code="g">pages:693-707</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">http://dx.doi.org/10.2514/1.A33510</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">http://arc.aiaa.org/doi/full/10.2514/1.A33510</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2006</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="j">2016</subfield><subfield code="h">693-707</subfield></datafield></record></collection>
|
| author |
Garrett, Henry B |
| spellingShingle |
Garrett, Henry B ddc 380 Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 |
| authorStr |
Garrett, Henry B |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)129359114 |
| format |
Article |
| dewey-ones |
380 - Commerce, communications & transportation 620 - Engineering & allied operations |
| delete_txt_mv |
keep |
| author_role |
aut |
| collection |
OLC |
| remote_str |
false |
| illustrated |
Not Illustrated |
| issn |
0022-4650 |
| topic_title |
380 620 DNB Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 |
| topic |
ddc 380 |
| topic_unstemmed |
ddc 380 |
| topic_browse |
ddc 380 |
| format_facet |
Aufsätze Gedruckte Aufsätze |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
nc |
| author2_variant |
w k wk r w e rw rwe |
| hierarchy_parent_title |
Journal of spacecraft and rockets |
| hierarchy_parent_id |
129359114 |
| dewey-tens |
380 - Commerce, communications & transportation 620 - Engineering |
| hierarchy_top_title |
Journal of spacecraft and rockets |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)129359114 (DE-600)160513-6 (DE-576)014731444 |
| title |
Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 |
| ctrlnum |
(DE-627)OLC1979800677 (DE-599)GBVOLC1979800677 (PRQ)a630-464df68111628d4f4d381a313217f99afa5c40ad33e9a312ec3198b3ffa663820 (KEY)0013696420160000000000000693updatingthejovianplasmaandradiationenvironmentsthe |
| title_full |
Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 |
| author_sort |
Garrett, Henry B |
| journal |
Journal of spacecraft and rockets |
| journalStr |
Journal of spacecraft and rockets |
| lang_code |
eng |
| isOA_bool |
false |
| dewey-hundreds |
300 - Social sciences 600 - Technology |
| recordtype |
marc |
| publishDateSort |
2016 |
| contenttype_str_mv |
txt |
| container_start_page |
693 |
| author_browse |
Garrett, Henry B |
| class |
380 620 DNB |
| format_se |
Aufsätze |
| author-letter |
Garrett, Henry B |
| doi_str_mv |
10.2514/1.A33510 |
| dewey-full |
380 620 |
| title_sort |
updating the jovian plasma and radiation environments: the latest results for 2015 |
| title_auth |
Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 |
| abstract |
Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept. |
| abstractGer |
Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept. |
| abstract_unstemmed |
Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept. |
| collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OPC-AST GBV_ILN_22 GBV_ILN_70 GBV_ILN_2006 GBV_ILN_4046 GBV_ILN_4700 |
| title_short |
Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015 |
| url |
http://dx.doi.org/10.2514/1.A33510 http://arc.aiaa.org/doi/full/10.2514/1.A33510 |
| remote_bool |
false |
| author2 |
Kim, Wousik Evans, Robin W |
| author2Str |
Kim, Wousik Evans, Robin W |
| ppnlink |
129359114 |
| mediatype_str_mv |
n |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| author2_role |
oth oth |
| doi_str |
10.2514/1.A33510 |
| up_date |
2024-07-04T01:42:46.455Z |
| _version_ |
1803610873088966656 |
| fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">OLC1979800677</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230714204040.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">160816s2016 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.2514/1.A33510</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">PQ20160815</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC1979800677</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVOLC1979800677</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(PRQ)a630-464df68111628d4f4d381a313217f99afa5c40ad33e9a312ec3198b3ffa663820</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(KEY)0013696420160000000000000693updatingthejovianplasmaandradiationenvironmentsthe</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">380</subfield><subfield code="a">620</subfield><subfield code="q">DNB</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Garrett, Henry B</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Updating the Jovian Plasma and Radiation Environments: The Latest Results for 2015</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2016</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Since publication in 1983 by Divine and Garrett (“Charged Particle Distributions in Jupiter’s Magnetosphere,” Journal of Geophysical Research, Vol. null, No. , Sept. 1983, pp. 6889–6903.), the Jet Propulsion Laboratory’s plasma and radiation models have been the design standard for NASA’s missions to Jupiter. These models consist of representations of the cold plasma and electrons, the warm and auroral electrons and protons, and the radiation environment (high-energy electrons, protons, and heavy ions). The current status of these models, which have been undergoing extensive revision, is reviewed, and examples of their uses in modeling the effects of the environment on Jovian missions are provided. Of particular importance are recent changes in the plasma-environment models for modeling the charging effects on the proposed Europa mission, and the extension of the high-energy proton model from ∼12 to ∼50 RJ to study the radiation effects on the solar arrays for that mission concept.</subfield></datafield><datafield tag="540" ind1=" " ind2=" "><subfield code="a">Nutzungsrecht: Copyright © 2016 by the American Institute of Aeronautics and Astronautics, Inc. The U.S. Government has a royalty-free license to exercise all rights under the copyright claimed herein for Governmental purposes. All other rights are reserved by the copyright owner. Copies of this paper may be made for personal and internal use, on condition that the copier pay the per-copy fee to the Copyright Clearance Center (CCC). All requests for copying and permission to reprint should be submitted to CCC at ; employ the ISSN (print) or (online) to initiate your request.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kim, Wousik</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Evans, Robin W</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Journal of spacecraft and rockets</subfield><subfield code="d">Reston, Va. [u.a.] : Inst., 1964</subfield><subfield code="g">(2016), Seite 693-707</subfield><subfield code="w">(DE-627)129359114</subfield><subfield code="w">(DE-600)160513-6</subfield><subfield code="w">(DE-576)014731444</subfield><subfield code="x">0022-4650</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">year:2016</subfield><subfield code="g">pages:693-707</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">http://dx.doi.org/10.2514/1.A33510</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">http://arc.aiaa.org/doi/full/10.2514/1.A33510</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-TEC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2006</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4700</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="j">2016</subfield><subfield code="h">693-707</subfield></datafield></record></collection>
|
| score |
7.400529 |