Class information for: |
Basic class information |
| Class id | #P | Avg. number of references |
Database coverage of references |
|---|---|---|---|
| 30551 | 167 | 24.0 | 39% |
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 |
| 30551 | 1 | CIENCIAS CAT//CIENCIAS EXPT FIS//CLOUD EVAPORATION | 167 |
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 | CIENCIAS CAT | address | 182847 | 1% | 100% | 1 |
| 2 | CIENCIAS EXPT FIS | address | 182847 | 1% | 100% | 1 |
| 3 | CLOUD EVAPORATION | authKW | 182847 | 1% | 100% | 1 |
| 4 | CONDUCTIVE COOLING FRONTS | authKW | 182847 | 1% | 100% | 1 |
| 5 | EXPTL CIENCIAS FIS | address | 182847 | 1% | 100% | 1 |
| 6 | INSTABILITY GENERAL | authKW | 182847 | 1% | 100% | 1 |
| 7 | RADIATION DRIVEN THERMAL INSTABILITY | authKW | 182847 | 1% | 100% | 1 |
| 8 | SPHERICAL FLOWS DYNAMICS | authKW | 182847 | 1% | 100% | 1 |
| 9 | STARS PRE MAIN SEQUENCE MAGNETIC FIELDS | authKW | 182847 | 1% | 100% | 1 |
| 10 | TWO PHASE PLASMA | authKW | 182847 | 1% | 100% | 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 | 5866 | 77% | 0% | 128 |
| 2 | Physics, Fluids & Plasmas | 699 | 16% | 0% | 27 |
| 3 | Mechanics | 14 | 4% | 0% | 7 |
| 4 | Physics, Multidisciplinary | 7 | 5% | 0% | 8 |
| 5 | Geochemistry & Geophysics | 2 | 2% | 0% | 3 |
| 6 | Physics, Mathematical | 2 | 2% | 0% | 3 |
| 7 | Physics, Nuclear | 2 | 2% | 0% | 3 |
| 8 | Engineering, Aerospace | 1 | 1% | 0% | 1 |
| 9 | Computer Science, Hardware & Architecture | 0 | 1% | 0% | 1 |
| 10 | Meteorology & Atmospheric Sciences | -0 | 1% | 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 | CIENCIAS CAT | 182847 | 1% | 100% | 1 |
| 2 | CIENCIAS EXPT FIS | 182847 | 1% | 100% | 1 |
| 3 | EXPTL CIENCIAS FIS | 182847 | 1% | 100% | 1 |
| 4 | ASTROFIS TEOR | 121884 | 5% | 8% | 8 |
| 5 | ASTROPHYS TEOR | 91423 | 1% | 50% | 1 |
| 6 | ED HULBURT SPACE | 91423 | 1% | 50% | 1 |
| 7 | EO HULBERT SPACE | 36568 | 1% | 20% | 1 |
| 8 | IST FIS MATEMAT | 15235 | 1% | 8% | 1 |
| 9 | IST FIS GEN | 2981 | 1% | 1% | 2 |
| 10 | FIS FUNDAMENTAL | 1397 | 2% | 0% | 3 |
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 | ASTROPHYSICAL JOURNAL | 9883 | 39% | 0% | 65 |
| 2 | SOLAR PHYSICS | 3178 | 7% | 0% | 11 |
| 3 | PHYSICS OF FLUIDS B-PLASMA PHYSICS | 2310 | 3% | 0% | 5 |
| 4 | SOVIET ASTRONOMY LETTERS | 2052 | 2% | 0% | 4 |
| 5 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 1198 | 3% | 0% | 5 |
| 6 | GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS | 1137 | 2% | 0% | 3 |
| 7 | BULLETIN OF THE ASTRONOMICAL SOCIETY OF INDIA | 992 | 1% | 1% | 1 |
| 8 | PHYSICS OF PLASMAS | 961 | 6% | 0% | 10 |
| 9 | ASTROPHYSICS AND SPACE SCIENCE | 698 | 4% | 0% | 7 |
| 10 | REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA | 578 | 1% | 0% | 2 |
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 | SIGALOTTI, LDG , SIRA, E , TREMOLA, C , (2002) PROPAGATION OF SOUND AND THERMAL WAVES IN AN IONIZING-RECOMBINING HYDROGEN PLASMA: REVISION OF RESULTS.PHYSICS OF PLASMAS. VOL. 9. ISSUE 11. P. 4726 -4735 | 13 | 100% | 1 |
| 2 | IBANEZ, MH , BESSEGA, MC , (2000) DYNAMICS OF COOL FRONTS IN OPTICALLY THIN HOT PLASMAS.ASTROPHYSICAL JOURNAL. VOL. 531. ISSUE 2. P. 838 -845 | 15 | 65% | 3 |
| 3 | KAMAYA, H , (1999) MASS CONDENSATION ON PROTO-GLOBULAR CLUSTERS OF THE TWO-COMPONENT PROTOGALAXY.ASTROPHYSICAL JOURNAL. VOL. 514. ISSUE 1. P. L21 -L23 | 14 | 70% | 0 |
| 4 | KAMAYA, H , (1999) DAMPING EFFICIENCY OF THE VOID MODE IN A TWO-PHASE GAS MIXTURE WITH A PHASE TRANSITION.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN. VOL. 51. ISSUE 5. P. 617 -623 | 17 | 57% | 1 |
| 5 | STEELE, CDC , IBANEZ, MH , SIRA, E , (2000) NONLINEAR THERMAL INSTABILITY IN OPTICALLY THIN PLASMAS.PHYSICS OF PLASMAS. VOL. 7. ISSUE 9. P. 3781 -3789 | 15 | 60% | 4 |
| 6 | KAYAMA, H , (1998) STABILITY OF SMALL-SCALE KELVIN-HELMHOLTZ INSTABILITY FOR TWO-COMPONENT PROTOGALAXIES.ASTROPHYSICAL JOURNAL. VOL. 506. ISSUE 1. P. 289-291 | 15 | 58% | 8 |
| 7 | SIGALOTTI, LD , SIRA, E , RENDON, O , TREMOLA, C , MENDOZA-BRICENO, CA , (2004) PROPAGATION OF THERMAL AND HYDROMAGNETIC WAVES IN AN IONIZING-RECOMBINING HYDROGEN PLASMA.PHYSICS OF PLASMAS. VOL. 11. ISSUE 4. P. 1631-1644 | 9 | 75% | 1 |
| 8 | SPARKS, L , VANHOVEN, G , (1988) THERMAL-INSTABILITY OF A RADIATIVE AND RESISTIVE CORONAL PLASMA.ASTROPHYSICAL JOURNAL. VOL. 333. ISSUE 2. P. 953-964 | 13 | 93% | 7 |
| 9 | ARANSON, I , MEERSON, B , SASOROV, PV , (1993) NONLINEAR RADIATIVE-CONDENSATION INSTABILITY AND PATTERN-FORMATION - ONE-DIMENSIONAL DYNAMICS.PHYSICAL REVIEW E. VOL. 47. ISSUE 6. P. 4337-4348 | 9 | 100% | 19 |
| 10 | MEERSON, B , STEELE, CDC , MILNE, AM , PRIEST, ER , (1993) ON THE NONLINEAR-THEORY OF THE LONG-WAVELENGTH RADIATIVE CONDENSATION INSTABILITY.PHYSICS OF FLUIDS B-PLASMA PHYSICS. VOL. 5. ISSUE 9. P. 3417-3431 | 11 | 73% | 6 |
Classes with closest relation at Level 1 |