Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
37491 | 56 | 15.5 | 38% |
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 |
19 | 3 | ASTRONOMY & ASTROPHYSICS//ASTROPHYSICAL JOURNAL//ASTRON | 118981 |
38 | 2 | STARS FORMATION//ISM CLOUDS//ISM MOLECULES | 31753 |
37491 | 1 | FRANCE ASTROPHYS THEOR 98 BIS BD ARAGO//INTENSITY RATIO CO C 12 COC 13//QUASARS ABSORPTION LINES QUASARS INDIVIDUAL Q 1100 264 | 56 |
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 | FRANCE ASTROPHYS THEOR 98 BIS BD ARAGO | address | 545281 | 2% | 100% | 1 |
2 | INTENSITY RATIO CO C 12 COC 13 | authKW | 545281 | 2% | 100% | 1 |
3 | QUASARS ABSORPTION LINES QUASARS INDIVIDUAL Q 1100 264 | authKW | 545281 | 2% | 100% | 1 |
4 | REYNOLD METHOD | authKW | 545281 | 2% | 100% | 1 |
5 | TURBULENT LINE FORMATION | authKW | 545281 | 2% | 100% | 1 |
6 | NLTE EFFECTS | authKW | 272639 | 2% | 50% | 1 |
7 | OBSERV ALGER | address | 272639 | 2% | 50% | 1 |
8 | ISM CLOUDS KINEMATICS AND DYNAMICS | authKW | 109055 | 2% | 20% | 1 |
9 | ISM INDIVIDUAL M17SW | authKW | 109055 | 2% | 20% | 1 |
10 | ZAA | address | 36350 | 2% | 7% | 1 |
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 | Astronomy & Astrophysics | 3141 | 96% | 0% | 54 |
2 | Spectroscopy | 6 | 4% | 0% | 2 |
3 | Optics | 1 | 4% | 0% | 2 |
4 | Meteorology & Atmospheric Sciences | 1 | 2% | 0% | 1 |
5 | Geosciences, Multidisciplinary | 0 | 2% | 0% | 1 |
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 | FRANCE ASTROPHYS THEOR 98 BIS BD ARAGO | 545281 | 2% | 100% | 1 |
2 | OBSERV ALGER | 272639 | 2% | 50% | 1 |
3 | ZAA | 36350 | 2% | 7% | 1 |
4 | ZENTRUM ASTRON ASTROPHYS | 33607 | 5% | 2% | 3 |
5 | MAIN PULKOVO ASTRON OBSERV | 15356 | 4% | 1% | 2 |
6 | CENT PULKOVO ASTRON OBSERV | 4160 | 2% | 1% | 1 |
7 | MAIN ASTRON OBSERV | 2268 | 4% | 0% | 2 |
8 | STERNBERG ASTRON | 904 | 4% | 0% | 2 |
9 | THEORET ASTROPHYS | 772 | 4% | 0% | 2 |
10 | THEORET PHYS | 394 | 13% | 0% | 7 |
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 | ASTRONOMY & ASTROPHYSICS | 7934 | 48% | 0% | 27 |
2 | ASTRONOMISCHE NACHRICHTEN | 4039 | 9% | 0% | 5 |
3 | SKY AND TELESCOPE | 2914 | 2% | 1% | 1 |
4 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 789 | 14% | 0% | 8 |
5 | SPACE SCIENCE REVIEWS | 672 | 4% | 0% | 2 |
6 | IAU SYMPOSIA | 619 | 5% | 0% | 3 |
7 | JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 315 | 4% | 0% | 2 |
8 | SOLAR PHYSICS | 312 | 4% | 0% | 2 |
9 | ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 236 | 2% | 0% | 1 |
10 | ADVANCES IN SPACE RESEARCH-SERIES | 147 | 2% | 0% | 1 |
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 | LEVSHAKOV, SA , KEGEL, WH , (1997) NEW ASPECTS OF ABSORPTION LINE FORMATION IN INTERVENING TURBULENT CLOUDS .1. GENERAL PRINCIPLES.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 288. ISSUE 3. P. 787-801 | 9 | 75% | 13 |
2 | LEVSHAKOV, SA , KEGEL, WH , MAZETS, IE , (1997) NEW ASPECTS OF ABSORPTION LINE FORMATION IN INTERVENING TURBULENT CLOUDS .2. MONTE CARLO SIMULATION OF INTERSTELLAR H+D LY ALPHA ABSORPTION PROFILES.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. VOL. 288. ISSUE 3. P. 802-816 | 9 | 45% | 4 |
3 | HEGMANN, M , KEGEL, WH , (2000) NON-LTE LINE FORMATION IN CLUMPY AND TURBULENT MOLECULAR CLOUDS.ASTRONOMY & ASTROPHYSICS. VOL. 359. ISSUE 1. P. 405 -412 | 5 | 56% | 10 |
4 | PIEHLER, G , KEGEL, WH , (1995) THE FORMATION OF INTERSTELLAR MOLECULAR LINES IN A TURBULENT VELOCITY-FIELD WITH FINITE CORRELATION LENGTH .3. SPHERICAL CLOUDS IN HYDROSTATIC EQUILIBRIUM.ASTRONOMY & ASTROPHYSICS. VOL. 297. ISSUE 3. P. 841 -853 | 3 | 100% | 7 |
5 | HEGMANN, M , HENGEL, C , ROLLIG, M , KEGEL, WH , (2006) THE FORMATION OF INTERSTELLAR MOLECULAR LINES IN A TURBULENT VELOCITY FIELD WITH FINITE CORRELATION LENGTH - IV. PHYSICAL PARAMETERS OF BOK GOBULES.ASTRONOMY & ASTROPHYSICS. VOL. 445. ISSUE 2. P. 591-600 | 5 | 42% | 1 |
6 | HEGMANN, M , KEGEL, WH , SEDLMAYR, E , (2007) CO COOLING RATES FOR CLUMPY AND TURBULENT MOLECULAR CLOUDS.ASTRONOMY & ASTROPHYSICS. VOL. 469. ISSUE 1. P. 223-232 | 6 | 33% | 3 |
7 | LOUCIF, ML , BEN JAFFEL, L , (2002) NON-LTE LINE TRANSFER WITH SPATIALLY CORRELATED TURBULENCE: FLUCTUATION AGAINST AVERAGE EMERGENT RADIATION FIELD.ASTRONOMY & ASTROPHYSICS. VOL. 389. ISSUE 1. P. 213-227 | 5 | 42% | 2 |
8 | DEISS, BM , JUST, A , KEGEL, WH , (1990) FLUCTUATIONS OF THE INTERSTELLAR-MEDIUM INDUCED BY THE STELLAR SYSTEM - MECHANICAL HEATING AND DYNAMIC FRICTION.ASTRONOMY & ASTROPHYSICS. VOL. 240. ISSUE 1. P. 123 -136 | 4 | 80% | 5 |
9 | SILANT'EV, NA , LEKHT, EE , MENDOZA-TORRES, JE , RUDNITSKIJ, GM , (2006) INFLUENCE OF TURBULENCE ON THE SHAPE OF A SPECTRAL LINE - THE ANALYTICAL APPROACH.ASTRONOMY & ASTROPHYSICS. VOL. 453. ISSUE 3. P. 989 -1002 | 4 | 40% | 0 |
10 | ALBRECHT, MA , KEGEL, WH , (1987) THE FORMATION OF INTERSTELLAR MOLECULAR LINES IN A TURBULENT VELOCITY-FIELD WITH FINITE CORRELATION LENGTH.ASTRONOMY & ASTROPHYSICS. VOL. 176. ISSUE 2. P. 317 -328 | 3 | 100% | 16 |
Classes with closest relation at Level 1 |