|
|
|
|
| LEADER |
01000caa a22002652 4500 |
| 001 |
NLM249960117 |
| 003 |
DE-627 |
| 005 |
20250218162645.0 |
| 007 |
tu |
| 008 |
231224s2013 xx ||||| 00| ||eng c |
| 028 |
5 |
2 |
|a pubmed25n0833.xml
|
| 035 |
|
|
|a (DE-627)NLM249960117
|
| 035 |
|
|
|a (NLM)26074632
|
| 040 |
|
|
|a DE-627
|b ger
|c DE-627
|e rakwb
|
| 041 |
|
|
|a eng
|
| 100 |
1 |
|
|a Wong, Michael H
|e verfasserin
|4 aut
|
| 245 |
1 |
0 |
|a Isotopes of nitrogen on Mars
|b Atmospheric measurements by Curiosity's mass spectrometer
|
| 264 |
|
1 |
|c 2013
|
| 336 |
|
|
|a Text
|b txt
|2 rdacontent
|
| 337 |
|
|
|a ohne Hilfsmittel zu benutzen
|b n
|2 rdamedia
|
| 338 |
|
|
|a Band
|b nc
|2 rdacarrier
|
| 500 |
|
|
|a Date Revised 20.11.2019
|
| 500 |
|
|
|a published: Print-Electronic
|
| 500 |
|
|
|a Citation Status Publisher
|
| 520 |
|
|
|a [1] The Sample Analysis at Mars (SAM) instrument suite on the Mars Science Laboratory (MSL) measured a Mars atmospheric14N/15N ratio of 173 ± 11 on sol 341 of the mission, agreeing with Viking's measurement of 168 ± 17. The MSL/SAM value was based on Quadrupole Mass Spectrometer measurements of an enriched atmospheric sample, with CO2 and H2O removed. Doubly ionized nitrogen data at m/z 14 and 14.5 had the highest signal/background ratio, with results confirmed by m/z 28 and 29 data. Gases in SNC meteorite glasses have been interpreted as mixtures containing a Martian atmospheric component, based partly on distinctive14N/15N and40Ar/14N ratios. Recent MSL/SAM measurements of the40Ar/14N ratio (0.51 ± 0.01) are incompatible with the Viking ratio (0.35 ± 0.08). The meteorite mixing line is more consistent with the atmospheric composition measured by Viking than by MSL
|
| 650 |
|
4 |
|a Journal Article
|
| 700 |
1 |
|
|a Atreya, Sushil K
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Mahaffy, Paul N
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Franz, Heather B
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Malespin, Charles
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Trainer, Melissa G
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Stern, Jennifer C
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Conrad, Pamela G
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Manning, Heidi L K
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Pepin, Robert O
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Becker, Richard H
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a McKay, Christopher P
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Owen, Tobias C
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Navarro-González, Rafael
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Jones, John H
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Jakosky, Bruce M
|e verfasserin
|4 aut
|
| 700 |
1 |
|
|a Steele, Andrew
|e verfasserin
|4 aut
|
| 773 |
0 |
8 |
|i Enthalten in
|t Geophysical research letters
|d 1984
|g 40(2013), 23 vom: 16. Dez., Seite 6033-6037
|w (DE-627)NLM098182501
|x 0094-8276
|7 nnns
|
| 773 |
1 |
8 |
|g volume:40
|g year:2013
|g number:23
|g day:16
|g month:12
|g pages:6033-6037
|
| 912 |
|
|
|a GBV_USEFLAG_A
|
| 912 |
|
|
|a SYSFLAG_A
|
| 912 |
|
|
|a GBV_NLM
|
| 912 |
|
|
|a GBV_ILN_350
|
| 951 |
|
|
|a AR
|
| 952 |
|
|
|d 40
|j 2013
|e 23
|b 16
|c 12
|h 6033-6037
|