Class information for: |
Basic class information |
Class id | #P | Avg. number of references |
Database coverage of references |
---|---|---|---|
18406 | 553 | 22.6 | 41% |
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 |
45 | 3 | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS//ASTRONOMY & ASTROPHYSICS//SOLAR PHYSICS | 95613 |
53 | 2 | SOLAR PHYSICS//SUN CORONA//SUN MAGNETIC FIELDS | 29887 |
18406 | 1 | SUN RADIO RADIATION//RADIO EMISSION QUIET//SOLAR PHYSICS | 553 |
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 | SUN RADIO RADIATION | authKW | 550559 | 17% | 10% | 96 |
2 | RADIO EMISSION QUIET | authKW | 220866 | 1% | 100% | 4 |
3 | SOLAR PHYSICS | journal | 118644 | 22% | 2% | 122 |
4 | CRAAM | address | 115183 | 2% | 16% | 13 |
5 | CONACYT SCIESMEX | address | 110433 | 0% | 100% | 2 |
6 | NOAO SOLAR OBSERV | address | 110433 | 0% | 100% | 2 |
7 | RADIATIVE TRANSFER METHODS ANALYTICAL METHODS NUMERICAL | authKW | 110433 | 0% | 100% | 2 |
8 | SLOWLY VARYING COMPONENT OF SOLAR RADIO RADIATION | authKW | 110433 | 0% | 100% | 2 |
9 | SUN LIMB DARKENING | authKW | 110433 | 0% | 100% | 2 |
10 | THERMAL CYCLOTRON RADIATION | authKW | 110433 | 0% | 100% | 2 |
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 | 25356 | 87% | 0% | 483 |
2 | Geochemistry & Geophysics | 106 | 5% | 0% | 25 |
3 | Engineering, Aerospace | 92 | 2% | 0% | 12 |
4 | Meteorology & Atmospheric Sciences | 18 | 2% | 0% | 13 |
5 | Geosciences, Multidisciplinary | 7 | 3% | 0% | 14 |
6 | Multidisciplinary Sciences | 1 | 1% | 0% | 3 |
7 | Optics | 1 | 2% | 0% | 12 |
8 | Physics, Multidisciplinary | 1 | 3% | 0% | 14 |
9 | Spectroscopy | 1 | 1% | 0% | 6 |
10 | Telecommunications | 0 | 1% | 0% | 4 |
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 | CRAAM | 115183 | 2% | 16% | 13 |
2 | CONACYT SCIESMEX | 110433 | 0% | 100% | 2 |
3 | NOAO SOLAR OBSERV | 110433 | 0% | 100% | 2 |
4 | SPECIAL ASTROPHYS OBSERV | 105565 | 9% | 4% | 52 |
5 | ST PETERSBURG BRANCH | 79531 | 7% | 4% | 36 |
6 | BIG BEAR SOLAR OBSERV MAIL CODE 26433 | 55216 | 0% | 100% | 1 |
7 | CENT PULKOVO ASTRON OBSERV GAO | 55216 | 0% | 100% | 1 |
8 | COSM RADIO EMISS | 55216 | 0% | 100% | 1 |
9 | EQUIPE SOHO EIT | 55216 | 0% | 100% | 1 |
10 | GVAR OBSERVAT | 55216 | 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 | SOLAR PHYSICS | 118644 | 22% | 2% | 122 |
2 | ASTROPHYSICAL BULLETIN | 56305 | 4% | 5% | 20 |
3 | ASTRONOMICHESKII ZHURNAL | 25099 | 6% | 1% | 31 |
4 | ASTROPHYSICS | 11549 | 1% | 3% | 7 |
5 | GEOMAGNETISM AND AERONOMY | 10019 | 3% | 1% | 19 |
6 | ASTROPHYSICAL JOURNAL | 6679 | 18% | 0% | 98 |
7 | ASTRONOMY REPORTS | 4642 | 2% | 1% | 13 |
8 | JOURNAL OF THE RADIO RESEARCH LABORATORY | 3871 | 0% | 4% | 2 |
9 | ASTRONOMY & ASTROPHYSICS | 3492 | 10% | 0% | 57 |
10 | COSMIC RESEARCH | 3322 | 1% | 1% | 7 |
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 | LEE, J , (2007) RADIO EMISSIONS FROM SOLAR ACTIVE REGIONS.SPACE SCIENCE REVIEWS. VOL. 133. ISSUE 1-4. P. 73 -102 | 53 | 57% | 19 |
2 | SHIBASAKI, K , ALISSANDRAKIS, CE , POHJOLAINEN, S , (2011) RADIO EMISSION OF THE QUIET SUN AND ACTIVE REGIONS (INVITED REVIEW).SOLAR PHYSICS. VOL. 273. ISSUE 2. P. 309 -337 | 48 | 50% | 31 |
3 | BOGOD, VM , KAL'TMAN, TI , PETEROVA, NG , YASNOV, LV , (2017) STUDY OF THE MAGNETOSPHERES OF ACTIVE REGIONS ON THE SUN BY RADIO ASTRONOMY TECHNIQUES.COSMIC RESEARCH. VOL. 55. ISSUE 1. P. 1 -11 | 27 | 75% | 0 |
4 | YASNOV, LV , (2014) ON THE NATURE OF NEUTRAL-LINE-ASSOCIATED RADIO SOURCES.SOLAR PHYSICS. VOL. 289. ISSUE 4. P. 1215-1225 | 24 | 77% | 5 |
5 | WHITE, SM , KUNDU, MR , GOPALSWAMY, N , (1992) HIGH DYNAMIC-RANGE MULTIFREQUENCY RADIO OBSERVATIONS OF A SOLAR ACTIVE REGION.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. VOL. 78. ISSUE 2. P. 599-& | 37 | 93% | 18 |
6 | BOGOD, VM , YASNOV, LV , (2016) DETERMINATION OF THE STRUCTURE OF THE CORONAL MAGNETIC FIELD USING MICROWAVE POLARIZATION MEASUREMENTS.SOLAR PHYSICS. VOL. 291. ISSUE 11. P. 3317 -3328 | 19 | 86% | 0 |
7 | TUN, SD , GARY, DE , GEORGOULIS, MK , (2011) THREE-DIMENSIONAL STRUCTURE OF A SOLAR ACTIVE REGION FROM SPATIALLY AND SPECTRALLY RESOLVED MICROWAVE OBSERVATIONS.ASTROPHYSICAL JOURNAL. VOL. 728. ISSUE 1. P. - | 22 | 65% | 7 |
8 | BOGOD, VM , STUPISHIN, AG , YASNOV, LV , (2012) ON MAGNETIC FIELDS OF ACTIVE REGIONS AT CORONAL HEIGHTS.SOLAR PHYSICS. VOL. 276. ISSUE 1-2. P. 61-73 | 17 | 81% | 4 |
9 | KUZNETSOV, AA , KEPPENS, R , XIA, C , (2016) SYNTHETIC RADIO VIEWS OF SIMULATED SOLAR FLUX ROPES.SOLAR PHYSICS. VOL. 291. ISSUE 3. P. 823 -845 | 28 | 45% | 0 |
10 | BROSIUS, JW , LANDI, E , COOK, JW , NEWMARK, JS , GOPALSWAMY, N , LARA, A , (2002) MEASUREMENTS OF THREE-DIMENSIONAL CORONAL MAGNETIC FIELDS FROM COORDINATED EXTREME-ULTRAVIOLET AND RADIO OBSERVATIONS OF A SOLAR ACTIVE REGION SUNSPOT.ASTROPHYSICAL JOURNAL. VOL. 574. ISSUE 1. P. 453 -466 | 25 | 68% | 20 |
Classes with closest relation at Level 1 |