Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
8563 | 1240 | 26.8 | 50% |
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 |
543 | 3 | PHYSICS OF PLASMAS//DUSTY PLASMA//DUSTY PLASMAS | 18619 |
928 | 2 | PHYSICS OF PLASMAS//JOURNAL OF PLASMA PHYSICS//THEORET PHYS 4 | 11071 |
8563 | 1 | LANGMUIR WAVES//LANGMUIR TURBULENCE//STRONG LANGMUIR TURBULENCE | 1240 |
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 | LANGMUIR WAVES | authKW | 229541 | 1% | 55% | 17 |
2 | LANGMUIR TURBULENCE | authKW | 126087 | 1% | 39% | 13 |
3 | STRONG LANGMUIR TURBULENCE | authKW | 110803 | 0% | 75% | 6 |
4 | SUN RADIO RADIATION | authKW | 102323 | 5% | 7% | 62 |
5 | ELECTROSTATIC DECAY | authKW | 98495 | 0% | 100% | 4 |
6 | GASDYNAMIC DESCRIPTION | authKW | 98495 | 0% | 100% | 4 |
7 | TYPE III BURSTS | authKW | 98491 | 0% | 67% | 6 |
8 | RADIO BURSTS TYPE III | authKW | 76945 | 0% | 63% | 5 |
9 | SPACE FUS ASTROPHYS | address | 73871 | 0% | 100% | 3 |
10 | THE ENSEMBLE METHOD | authKW | 73871 | 0% | 100% | 3 |
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 | Physics, Fluids & Plasmas | 24473 | 34% | 0% | 427 |
2 | Astronomy & Astrophysics | 8461 | 35% | 0% | 430 |
3 | Physics, Multidisciplinary | 1841 | 19% | 0% | 234 |
4 | Physics, Mathematical | 522 | 6% | 0% | 79 |
5 | Meteorology & Atmospheric Sciences | 230 | 5% | 0% | 56 |
6 | Mechanics | 222 | 6% | 0% | 70 |
7 | Geosciences, Multidisciplinary | 215 | 6% | 0% | 74 |
8 | Engineering, Aerospace | 37 | 1% | 0% | 13 |
9 | Geochemistry & Geophysics | 27 | 2% | 0% | 25 |
10 | Remote Sensing | 26 | 1% | 0% | 10 |
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 | SPACE FUS ASTROPHYS | 73871 | 0% | 100% | 3 |
2 | WAVE PHYS | 44320 | 0% | 60% | 3 |
3 | IONOSPHER PREDICT SERV | 32830 | 0% | 67% | 2 |
4 | OBSERV PARISLESIAUPMC | 32830 | 0% | 67% | 2 |
5 | WORLD SPACE ENVIRONM | 31656 | 0% | 43% | 3 |
6 | IPST | 27497 | 1% | 7% | 16 |
7 | ASTROPHYS PLANETARY ATMOSPHER | 24624 | 0% | 100% | 1 |
8 | ASTROPHYS PLANETARY ATMOSPHER SCI CB 391 | 24624 | 0% | 100% | 1 |
9 | CNRS 264 | 24624 | 0% | 100% | 1 |
10 | CNRS UMR 6115 | 24624 | 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 | PHYSICS OF PLASMAS | 40123 | 14% | 1% | 175 |
2 | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 25968 | 12% | 1% | 144 |
3 | PHYSICS OF FLUIDS B-PLASMA PHYSICS | 24113 | 4% | 2% | 44 |
4 | JOURNAL OF PLASMA PHYSICS | 15031 | 3% | 1% | 42 |
5 | SOLAR PHYSICS | 12282 | 5% | 1% | 59 |
6 | PHYSICS OF FLUIDS | 7294 | 5% | 0% | 65 |
7 | PLASMA PHYSICS REPORTS | 2569 | 1% | 1% | 17 |
8 | PLASMA PHYSICS AND CONTROLLED FUSION | 1783 | 2% | 0% | 22 |
9 | PHYSICA SCRIPTA | 1582 | 3% | 0% | 33 |
10 | PHYSICA D-NONLINEAR PHENOMENA | 1368 | 2% | 0% | 19 |
Author Key Words |
Rank | Term | Chi square | Shr. of publ. in class containing term |
Class's shr. of term's tot. occurrences |
#P with term in class |
LCSH search | Wikipedia search |
---|---|---|---|---|---|---|---|
1 | LANGMUIR WAVES | 229541 | 1% | 55% | 17 | Search LANGMUIR+WAVES | Search LANGMUIR+WAVES |
2 | LANGMUIR TURBULENCE | 126087 | 1% | 39% | 13 | Search LANGMUIR+TURBULENCE | Search LANGMUIR+TURBULENCE |
3 | STRONG LANGMUIR TURBULENCE | 110803 | 0% | 75% | 6 | Search STRONG+LANGMUIR+TURBULENCE | Search STRONG+LANGMUIR+TURBULENCE |
4 | SUN RADIO RADIATION | 102323 | 5% | 7% | 62 | Search SUN+RADIO+RADIATION | Search SUN+RADIO+RADIATION |
5 | ELECTROSTATIC DECAY | 98495 | 0% | 100% | 4 | Search ELECTROSTATIC+DECAY | Search ELECTROSTATIC+DECAY |
6 | GASDYNAMIC DESCRIPTION | 98495 | 0% | 100% | 4 | Search GASDYNAMIC+DESCRIPTION | Search GASDYNAMIC+DESCRIPTION |
7 | TYPE III BURSTS | 98491 | 0% | 67% | 6 | Search TYPE+III+BURSTS | Search TYPE+III+BURSTS |
8 | RADIO BURSTS TYPE III | 76945 | 0% | 63% | 5 | Search RADIO+BURSTS+TYPE+III | Search RADIO+BURSTS+TYPE+III |
9 | THE ENSEMBLE METHOD | 73871 | 0% | 100% | 3 | Search THE+ENSEMBLE+METHOD | Search THE+ENSEMBLE+METHOD |
10 | TYPE III RADIO BURSTS | 73871 | 0% | 100% | 3 | Search TYPE+III+RADIO+BURSTS | Search TYPE+III+RADIO+BURSTS |
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 | GRAHAM, DB , CAIRNS, IH , (2014) DYNAMICAL EVIDENCE FOR NONLINEAR LANGMUIR WAVE PROCESSES IN TYPE III SOLAR RADIO BURSTS.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS. VOL. 119. ISSUE 4. P. 2430 -2457 | 63 | 94% | 1 |
2 | GRAHAM, DB , CAIRNS, IH , PRABHAKAR, DR , ERGUN, RE , MALASPINA, DM , BALE, SD , GOETZ, K , KELLOGG, PJ , (2012) DO LANGMUIR WAVE PACKETS IN THE SOLAR WIND COLLAPSE?.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS. VOL. 117. ISSUE . P. - | 66 | 92% | 7 |
3 | ROBINSON, PA , (1997) NONLINEAR WAVE COLLAPSE AND STRONG TURBULENCE.REVIEWS OF MODERN PHYSICS. VOL. 69. ISSUE 2. P. 507 -573 | 122 | 54% | 256 |
4 | GRAHAM, DB , CAIRNS, IH , (2013) ELECTROSTATIC DECAY OF LANGMUIR/Z-MODE WAVES IN TYPE III SOLAR RADIO BURSTS.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS. VOL. 118. ISSUE 7. P. 3968-3984 | 55 | 90% | 12 |
5 | KRAFFT, C , VOLOKITIN, AS , KRASNOSELSKIKH, VV , (2015) LANGMUIR WAVE DECAY IN INHOMOGENEOUS SOLAR WIND PLASMAS: SIMULATION RESULTS.ASTROPHYSICAL JOURNAL. VOL. 809. ISSUE 2. P. - | 48 | 92% | 1 |
6 | MALASPINA, DM , CAIRNS, IH , ERGUN, RE , (2010) THE 2F(P) RADIATION FROM LOCALIZED LANGMUIR WAVES.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS. VOL. 115. ISSUE . P. - | 48 | 91% | 18 |
7 | ZIEBELL, LF , YOON, PH , PETRUZZELLIS, LT , GAELZER, R , PAVAN, J , (2015) PLASMA EMISSION BY NONLINEAR ELECTROMAGNETIC PROCESSES.ASTROPHYSICAL JOURNAL. VOL. 806. ISSUE 2. P. - | 53 | 76% | 0 |
8 | REID, HAS , RATCLIFFE, H , (2014) A REVIEW OF SOLAR TYPE III RADIO BURSTS.RESEARCH IN ASTRONOMY AND ASTROPHYSICS. VOL. 14. ISSUE 7. P. 773 -804 | 76 | 41% | 31 |
9 | CAIRNS, IH , (2000) ROLE OF COLLECTIVE EFFECTS IN DOMINANCE OF SCATTERING OFF THERMAL IONS OVER LANGMUIR WAVE DECAY: ANALYSIS, SIMULATIONS, AND SPACE APPLICATIONS.PHYSICS OF PLASMAS. VOL. 7. ISSUE 12. P. 4901-4915 | 57 | 98% | 23 |
10 | GRAHAM, DB , ROBINSON, RA , CAIRNS, LH , (2012) BEAM-DRIVEN THREE-DIMENSIONAL ELECTROMAGNETIC STRONG TURBULENCE.PHYSICS OF PLASMAS. VOL. 19. ISSUE 8. P. - | 42 | 98% | 0 |
Classes with closest relation at Level 1 |