Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
14752 | 752 | 46.1 | 54% |
Hierarchy of classes |
The table includes all classes above and classes immediately below the current class. |
Cluster id | Level | Cluster label | #P |
---|---|---|---|
19 | 4 | ASTRONOMY & ASTROPHYSICS//ASTROPHYSICAL JOURNAL//ASTRON | 523489 |
170 | 3 | ICARUS//JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS//METEORITICS & PLANETARY SCIENCE | 58974 |
638 | 2 | METEORITICS & PLANETARY SCIENCE//COMETS//METEORS | 13723 |
14752 | 1 | PRESOLAR GRAINS//NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES//LUNAR FINES | 752 |
Terms with highest relevance score |
rank | Term | termType | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|---|
1 | PRESOLAR GRAINS | authKW | 444169 | 3% | 58% | 19 |
2 | NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES | authKW | 172121 | 11% | 5% | 84 |
3 | LUNAR FINES | authKW | 162417 | 1% | 100% | 4 |
4 | ISOTOPE ABUNDANCE ANOMALIES | authKW | 129932 | 1% | 80% | 4 |
5 | ISOTOPIC ANOMALIES | authKW | 124342 | 1% | 44% | 7 |
6 | BAII STAR | authKW | 121812 | 0% | 100% | 3 |
7 | CS STAR | authKW | 121812 | 0% | 100% | 3 |
8 | NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES STARS AGB AND POST AGB | authKW | 121812 | 0% | 100% | 3 |
9 | FISSION XENON | authKW | 91358 | 0% | 75% | 3 |
10 | COSMOCHEM | address | 90427 | 1% | 32% | 7 |
Web of Science journal categories |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | Geochemistry & Geophysics | 17332 | 42% | 0% | 317 |
2 | Astronomy & Astrophysics | 5519 | 36% | 0% | 270 |
3 | Nuclear Science & Technology | 281 | 6% | 0% | 48 |
4 | Geosciences, Multidisciplinary | 197 | 7% | 0% | 53 |
5 | Chemistry, Inorganic & Nuclear | 109 | 5% | 0% | 40 |
6 | Mineralogy | 74 | 2% | 0% | 12 |
7 | Physics, Nuclear | 66 | 4% | 0% | 27 |
8 | Chemistry, Analytical | 46 | 5% | 0% | 37 |
9 | AGRICULTURAL EXPERIMENT STATION REPORTS | 37 | 0% | 0% | 1 |
10 | Multidisciplinary Sciences | 17 | 1% | 0% | 8 |
Address terms |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | COSMOCHEM | 90427 | 1% | 32% | 7 |
2 | GEOPHYS GEOCHEM | 81208 | 0% | 100% | 2 |
3 | PARTICLE CHEM | 74753 | 2% | 12% | 16 |
4 | CHICAGO COSMOCHEM | 73073 | 1% | 20% | 9 |
5 | GEOSCI MINERAL | 50748 | 1% | 25% | 5 |
6 | MCDONNELL SPACE SCI | 48794 | 4% | 4% | 27 |
7 | ROBERT M WALKER SPACE SCI | 44127 | 1% | 22% | 5 |
8 | BIOL GEOCHEM ARCHITECTURE CIVIL ENVIRONM EN | 40604 | 0% | 100% | 1 |
9 | DIPARTMENTO FIS GEN | 40604 | 0% | 100% | 1 |
10 | ENRICO FERMI CHEM GEOPHYS SCI | 40604 | 0% | 100% | 1 |
Journals |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
---|---|---|---|---|---|
1 | METEORITICS | 41496 | 3% | 4% | 24 |
2 | METEORITICS & PLANETARY SCIENCE | 34822 | 6% | 2% | 47 |
3 | GEOKHIMIYA | 33537 | 7% | 2% | 50 |
4 | GEOCHIMICA ET COSMOCHIMICA ACTA | 19767 | 11% | 1% | 79 |
5 | GEOCHEMICAL JOURNAL | 13623 | 3% | 2% | 22 |
6 | ASTROPHYSICAL JOURNAL | 8636 | 17% | 0% | 130 |
7 | GEOCHEMISTRY INTERNATIONAL | 5756 | 2% | 1% | 16 |
8 | NEW ASTRONOMY REVIEWS | 4769 | 2% | 1% | 12 |
9 | TENNESSEE FARM & HOME SCIENCE | 4510 | 0% | 11% | 1 |
10 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 4020 | 1% | 1% | 10 |
Author Key Words |
Core articles |
The table includes core articles in the class. The following variables is taken into account for the relevance score of an article in a cluster c: (1) Number of references referring to publications in the class. (2) Share of total number of active references referring to publications in the class. (3) Age of the article. New articles get higher score than old articles. (4) Citation rate, normalized to year. |
Rank | Reference | # ref. in cl. |
Shr. of ref. in cl. |
Citations |
---|---|---|---|---|
1 | AMARI, S , ZINNER, E , GALLINO, R , (2014) PRESOLAR GRAPHITE FROM THE MURCHISON METEORITE: AN ISOTOPIC STUDY.GEOCHIMICA ET COSMOCHIMICA ACTA. VOL. 133. ISSUE . P. 479-522 | 83 | 73% | 6 |
2 | LODDERS, K , AMARI, S , (2005) PRESOLAR GRAINS FROM METEORITES: REMNANTS FROM THE EARLY TIMES OF THE SOLAR SYSTEM.CHEMIE DER ERDE-GEOCHEMISTRY. VOL. 65. ISSUE 2. P. 93 -166 | 114 | 50% | 87 |
3 | HOPPE, P , (2008) RESERVOIR FOR COMET MATERIAL: CIRCUMSTELLAR GRAINS.SPACE SCIENCE REVIEWS. VOL. 138. ISSUE 1-4. P. 43 -57 | 61 | 90% | 16 |
4 | CLAYTON, DD , NITTLER, LR , (2004) ASTROPHYSICS WITH PRESOLAR STARDUST.ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS. VOL. 42. ISSUE . P. 39-78 | 86 | 59% | 151 |
5 | FLOSS, C , HAENECOUR, P , (2016) PRESOLAR SILICATE GRAINS: ABUNDANCES, ISOTOPIC AND ELEMENTAL COMPOSITIONS, AND THE EFFECTS OF SECONDARY PROCESSING.GEOCHEMICAL JOURNAL. VOL. 50. ISSUE 1. P. 3 -25 | 54 | 52% | 7 |
6 | HOPPE, P , LEITNER, J , GRONER, E , MARHAS, KK , MEYER, BS , AMARI, S , (2010) NANOSIMS STUDIES OF SMALL PRESOLAR SIC GRAINS: NEW INSIGHTS INTO SUPERNOVA NUCLEOSYNTHESIS, CHEMISTRY, AND DUST FORMATION.ASTROPHYSICAL JOURNAL. VOL. 719. ISSUE 2. P. 1370-1384 | 57 | 78% | 24 |
7 | NGUYEN, AN , NITTLER, LR , STADERMANN, FJ , STROUD, RM , ALEXANDER, CMO , (2010) COORDINATED ANALYSES OF PRESOLAR GRAINS IN THE ALLAN HILLS 77307 AND QUEEN ELIZABETH RANGE 99177 METEORITES.ASTROPHYSICAL JOURNAL. VOL. 719. ISSUE 1. P. 166-189 | 63 | 66% | 47 |
8 | ZINNER, E , (2013) LABORATORY ANALYSIS OF STARDUST.ANALYTICAL CHEMISTRY. VOL. 85. ISSUE 3. P. 1264-1270 | 44 | 96% | 2 |
9 | BESMEHN, A , HOPPE, P , OTT, U , (2011) SEARCH FOR EXTINCT ALUMINUM-26 AND TITANIUM-44 IN NANODIAMONDS FROM THE ALLENDE CV3 AND MURCHISON CM2 METEORITES.METEORITICS & PLANETARY SCIENCE. VOL. 46. ISSUE 9. P. 1265 -1275 | 48 | 89% | 1 |
10 | OTT, U , (2014) PLANETARY AND PRE-SOLAR NOBLE GASES IN METEORITES.CHEMIE DER ERDE-GEOCHEMISTRY. VOL. 74. ISSUE 4. P. 519 -544 | 77 | 42% | 9 |
Classes with closest relation at Level 1 |