A hypothesis on the locations of lunar gas venting
Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
|---|
| Format: |
E-Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1977 |
|---|
| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
|---|---|
| Übergeordnetes Werk: |
in: Physics of the Earth and Planetary Interiors - Amsterdam : Elsevier, 14(1977), 3, Seite 274-275 |
| Übergeordnetes Werk: |
volume:14 ; year:1977 ; number:3 ; pages:274-275 |
| Links: |
|---|
| Katalog-ID: |
NLEJ181645734 |
|---|
| LEADER | 01000caa a22002652 4500 | ||
|---|---|---|---|
| 001 | NLEJ181645734 | ||
| 003 | DE-627 | ||
| 005 | 20210706160133.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 070505s1977 xx |||||o 00| ||eng c | ||
| 035 | |a (DE-627)NLEJ181645734 | ||
| 035 | |a (DE-599)GBVNLZ181645734 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 245 | 1 | 2 | |a A hypothesis on the locations of lunar gas venting |
| 264 | 1 | |c 1977 | |
| 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 Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters. | ||
| 533 | |f Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 | ||
| 700 | 1 | |a Friesen, L.J. |4 oth | |
| 773 | 0 | 8 | |i in |t Physics of the Earth and Planetary Interiors |d Amsterdam : Elsevier |g 14(1977), 3, Seite 274-275 |w (DE-627)NLEJ180732102 |w (DE-600)1500666-9 |x 0031-9201 |7 nnns |
| 773 | 1 | 8 | |g volume:14 |g year:1977 |g number:3 |g pages:274-275 |
| 856 | 4 | 0 | |u http://dx.doi.org/10.1016/0031-9201(77)90176-5 |
| 912 | |a GBV_USEFLAG_H | ||
| 912 | |a ZDB-1-SDJ | ||
| 912 | |a GBV_NL_ARTICLE | ||
| 951 | |a AR | ||
| 952 | |d 14 |j 1977 |e 3 |h 274-275 | ||
| matchkey_str |
article:00319201:1977----::hpteioteoainoln |
|---|---|
| hierarchy_sort_str |
1977 |
| publishDate |
1977 |
| allfields |
(DE-627)NLEJ181645734 (DE-599)GBVNLZ181645734 DE-627 ger DE-627 rakwb eng A hypothesis on the locations of lunar gas venting 1977 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Friesen, L.J. oth in Physics of the Earth and Planetary Interiors Amsterdam : Elsevier 14(1977), 3, Seite 274-275 (DE-627)NLEJ180732102 (DE-600)1500666-9 0031-9201 nnns volume:14 year:1977 number:3 pages:274-275 http://dx.doi.org/10.1016/0031-9201(77)90176-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1977 3 274-275 |
| spelling |
(DE-627)NLEJ181645734 (DE-599)GBVNLZ181645734 DE-627 ger DE-627 rakwb eng A hypothesis on the locations of lunar gas venting 1977 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Friesen, L.J. oth in Physics of the Earth and Planetary Interiors Amsterdam : Elsevier 14(1977), 3, Seite 274-275 (DE-627)NLEJ180732102 (DE-600)1500666-9 0031-9201 nnns volume:14 year:1977 number:3 pages:274-275 http://dx.doi.org/10.1016/0031-9201(77)90176-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1977 3 274-275 |
| allfields_unstemmed |
(DE-627)NLEJ181645734 (DE-599)GBVNLZ181645734 DE-627 ger DE-627 rakwb eng A hypothesis on the locations of lunar gas venting 1977 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Friesen, L.J. oth in Physics of the Earth and Planetary Interiors Amsterdam : Elsevier 14(1977), 3, Seite 274-275 (DE-627)NLEJ180732102 (DE-600)1500666-9 0031-9201 nnns volume:14 year:1977 number:3 pages:274-275 http://dx.doi.org/10.1016/0031-9201(77)90176-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1977 3 274-275 |
| allfieldsGer |
(DE-627)NLEJ181645734 (DE-599)GBVNLZ181645734 DE-627 ger DE-627 rakwb eng A hypothesis on the locations of lunar gas venting 1977 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Friesen, L.J. oth in Physics of the Earth and Planetary Interiors Amsterdam : Elsevier 14(1977), 3, Seite 274-275 (DE-627)NLEJ180732102 (DE-600)1500666-9 0031-9201 nnns volume:14 year:1977 number:3 pages:274-275 http://dx.doi.org/10.1016/0031-9201(77)90176-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1977 3 274-275 |
| allfieldsSound |
(DE-627)NLEJ181645734 (DE-599)GBVNLZ181645734 DE-627 ger DE-627 rakwb eng A hypothesis on the locations of lunar gas venting 1977 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Friesen, L.J. oth in Physics of the Earth and Planetary Interiors Amsterdam : Elsevier 14(1977), 3, Seite 274-275 (DE-627)NLEJ180732102 (DE-600)1500666-9 0031-9201 nnns volume:14 year:1977 number:3 pages:274-275 http://dx.doi.org/10.1016/0031-9201(77)90176-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 14 1977 3 274-275 |
| language |
English |
| source |
in Physics of the Earth and Planetary Interiors 14(1977), 3, Seite 274-275 volume:14 year:1977 number:3 pages:274-275 |
| sourceStr |
in Physics of the Earth and Planetary Interiors 14(1977), 3, Seite 274-275 volume:14 year:1977 number:3 pages:274-275 |
| format_phy_str_mv |
Article |
| institution |
findex.gbv.de |
| isfreeaccess_bool |
false |
| container_title |
Physics of the Earth and Planetary Interiors |
| authorswithroles_txt_mv |
Friesen, L.J. @@oth@@ |
| publishDateDaySort_date |
1977-01-01T00:00:00Z |
| hierarchy_top_id |
NLEJ180732102 |
| id |
NLEJ181645734 |
| language_de |
englisch |
| 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">NLEJ181645734</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20210706160133.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">070505s1977 xx |||||o 00| ||eng c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ181645734</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVNLZ181645734</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="245" ind1="1" ind2="2"><subfield code="a">A hypothesis on the locations of lunar gas venting</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1977</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">Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters.</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">Elsevier Journal Backfiles on ScienceDirect 1907 - 2002</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Friesen, L.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">in</subfield><subfield code="t">Physics of the Earth and Planetary Interiors</subfield><subfield code="d">Amsterdam : Elsevier</subfield><subfield code="g">14(1977), 3, Seite 274-275</subfield><subfield code="w">(DE-627)NLEJ180732102</subfield><subfield code="w">(DE-600)1500666-9</subfield><subfield code="x">0031-9201</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:14</subfield><subfield code="g">year:1977</subfield><subfield code="g">number:3</subfield><subfield code="g">pages:274-275</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://dx.doi.org/10.1016/0031-9201(77)90176-5</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_H</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-SDJ</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_NL_ARTICLE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">14</subfield><subfield code="j">1977</subfield><subfield code="e">3</subfield><subfield code="h">274-275</subfield></datafield></record></collection>
|
| 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">NLEJ181645734</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20210706160133.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">070505s1977 xx |||||o 00| ||eng c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ181645734</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVNLZ181645734</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="245" ind1="1" ind2="2"><subfield code="a">A hypothesis on the locations of lunar gas venting</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1977</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">Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters.</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">Elsevier Journal Backfiles on ScienceDirect 1907 - 2002</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Friesen, L.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">in</subfield><subfield code="t">Physics of the Earth and Planetary Interiors</subfield><subfield code="d">Amsterdam : Elsevier</subfield><subfield code="g">14(1977), 3, Seite 274-275</subfield><subfield code="w">(DE-627)NLEJ180732102</subfield><subfield code="w">(DE-600)1500666-9</subfield><subfield code="x">0031-9201</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:14</subfield><subfield code="g">year:1977</subfield><subfield code="g">number:3</subfield><subfield code="g">pages:274-275</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://dx.doi.org/10.1016/0031-9201(77)90176-5</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_H</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-SDJ</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_NL_ARTICLE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">14</subfield><subfield code="j">1977</subfield><subfield code="e">3</subfield><subfield code="h">274-275</subfield></datafield></record></collection>
|
| series2 |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
| ppnlink_with_tag_str_mv |
@@773@@(DE-627)NLEJ180732102 |
| format |
electronic Article |
| delete_txt_mv |
keep |
| collection |
NL |
| remote_str |
true |
| illustrated |
Not Illustrated |
| issn |
0031-9201 |
| topic_title |
A hypothesis on the locations of lunar gas venting |
| format_facet |
Elektronische Aufsätze Aufsätze Elektronische Ressource |
| format_main_str_mv |
Text Zeitschrift/Artikel |
| carriertype_str_mv |
zu |
| author2_variant |
l f lf |
| hierarchy_parent_title |
Physics of the Earth and Planetary Interiors |
| hierarchy_parent_id |
NLEJ180732102 |
| hierarchy_top_title |
Physics of the Earth and Planetary Interiors |
| isfreeaccess_txt |
false |
| familylinks_str_mv |
(DE-627)NLEJ180732102 (DE-600)1500666-9 |
| title |
A hypothesis on the locations of lunar gas venting |
| spellingShingle |
A hypothesis on the locations of lunar gas venting |
| ctrlnum |
(DE-627)NLEJ181645734 (DE-599)GBVNLZ181645734 |
| title_full |
A hypothesis on the locations of lunar gas venting |
| journal |
Physics of the Earth and Planetary Interiors |
| journalStr |
Physics of the Earth and Planetary Interiors |
| lang_code |
eng |
| isOA_bool |
false |
| recordtype |
marc |
| publishDateSort |
1977 |
| contenttype_str_mv |
zzz |
| container_start_page |
274 |
| container_volume |
14 |
| format_se |
Elektronische Aufsätze |
| title_sort |
hypothesis on the locations of lunar gas venting |
| title_auth |
A hypothesis on the locations of lunar gas venting |
| abstract |
Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters. |
| abstractGer |
Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters. |
| abstract_unstemmed |
Both lunar transient phenomena and ^2^2^2Rn/^2^1^0Po anomalies observed by Apollo-15 and -16 orbital alpha spectrometers display preferences for certain kinds of locations: rims of circular maria and craters with central peaks and/or dark floors. If these classes of observations are due to lunar gas venting, why are these types of locations preferred? The hypothesis offered is that these are locations at which cracks or channels exist extending deep enough into the moon to tap lunar volatile reservoirs. Possible channels include circumferential cracks around circular maria, old lava tubes for dark-floor and volcanic central peak craters, and shattered subsurface rock structure for impact central peak craters. |
| collection_details |
GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE |
| container_issue |
3 |
| title_short |
A hypothesis on the locations of lunar gas venting |
| url |
http://dx.doi.org/10.1016/0031-9201(77)90176-5 |
| remote_bool |
true |
| author2 |
Friesen, L.J. |
| author2Str |
Friesen, L.J. |
| ppnlink |
NLEJ180732102 |
| mediatype_str_mv |
z |
| isOA_txt |
false |
| hochschulschrift_bool |
false |
| author2_role |
oth |
| up_date |
2024-07-06T07:11:50.257Z |
| _version_ |
1803812769898692608 |
| score |
7.401078 |