Class information for: |
Basic class information |
ID | Publications | Average number of references |
Avg. shr. active ref. in WoS |
---|---|---|---|
536 | 3260 | 36.9 | 63% |
Classes in level above (level 2) |
ID, lev. above |
Publications | Label for level above |
---|---|---|
86 | 25897 | X RAYS BINARIES//PULSARS GENERAL//STARS NEUTRON |
Terms with highest relevance score |
Rank | Term | Type of term | Relevance score (tfidf) |
Class's shr. of term's tot. occurrences |
Shr. of publ. in class containing term |
Num. of publ. in class |
---|---|---|---|---|---|---|
1 | SUPERNOVA REMNANTS | Author keyword | 431 | 42% | 24% | 784 |
2 | ISM SUPERNOVA REMNANTS | Author keyword | 383 | 54% | 15% | 487 |
3 | ISM SUPERNOVA REMNANTS | Author keyword | 163 | 53% | 7% | 214 |
4 | ISM INDIVIDUAL CYGNUS LOOP | Author keyword | 162 | 100% | 1% | 43 |
5 | ISM INDIVIDUAL CASSIOPEIA A | Author keyword | 109 | 92% | 1% | 44 |
6 | X RAYS ISM | Author keyword | 97 | 35% | 7% | 227 |
7 | ACCELERATION OF PARTICLES | Author keyword | 86 | 18% | 13% | 425 |
8 | SHOCK WAVES | Author keyword | 63 | 11% | 17% | 546 |
9 | X RAYS ISM | Author keyword | 53 | 32% | 4% | 137 |
10 | GAMMA RAYS ISM | Author keyword | 47 | 49% | 2% | 70 |
Web of Science journal categories |
Author Key Words |
Rank | Web of Science journal category | Relevance score (tfidf) |
Class's shr. of term's tot. occurrences |
Shr. of publ. in class containing term |
Num. of publ. in class |
LCSH search | Wikipedia search |
---|---|---|---|---|---|---|---|
1 | SUPERNOVA REMNANTS | 431 | 42% | 24% | 784 | Search SUPERNOVA+REMNANTS | Search SUPERNOVA+REMNANTS |
2 | ISM SUPERNOVA REMNANTS | 383 | 54% | 15% | 487 | Search ISM+SUPERNOVA+REMNANTS | Search ISM+SUPERNOVA+REMNANTS |
3 | ISM SUPERNOVA REMNANTS | 163 | 53% | 7% | 214 | Search ISM++SUPERNOVA+REMNANTS | Search ISM++SUPERNOVA+REMNANTS |
4 | ISM INDIVIDUAL CYGNUS LOOP | 162 | 100% | 1% | 43 | Search ISM++INDIVIDUAL+CYGNUS+LOOP | Search ISM++INDIVIDUAL+CYGNUS+LOOP |
5 | ISM INDIVIDUAL CASSIOPEIA A | 109 | 92% | 1% | 44 | Search ISM++INDIVIDUAL+CASSIOPEIA+A | Search ISM++INDIVIDUAL+CASSIOPEIA+A |
6 | X RAYS ISM | 97 | 35% | 7% | 227 | Search X+RAYS++ISM | Search X+RAYS++ISM |
7 | ACCELERATION OF PARTICLES | 86 | 18% | 13% | 425 | Search ACCELERATION+OF+PARTICLES | Search ACCELERATION+OF+PARTICLES |
8 | SHOCK WAVES | 63 | 11% | 17% | 546 | Search SHOCK+WAVES | Search SHOCK+WAVES |
9 | X RAYS ISM | 53 | 32% | 4% | 137 | Search X+RAYS+ISM | Search X+RAYS+ISM |
10 | GAMMA RAYS ISM | 47 | 49% | 2% | 70 | Search GAMMA+RAYS+ISM | Search GAMMA+RAYS+ISM |
Key Words Plus |
Rank | Web of Science journal category | Relevance score (tfidf) |
Class's shr. of term's tot. occurrences |
Shr. of publ. in class containing term |
Num. of publ. in class |
---|---|---|---|---|---|
1 | SN 1006 | 251 | 74% | 6% | 189 |
2 | IC 443 | 175 | 76% | 4% | 123 |
3 | CYGNUS LOOP | 154 | 69% | 4% | 133 |
4 | CASSIOPEIA A | 139 | 50% | 6% | 204 |
5 | MAGNETIC FIELD AMPLIFICATION | 136 | 68% | 4% | 120 |
6 | NOVA REMNANT | 127 | 74% | 3% | 95 |
7 | COSMIC RAY ACCELERATION | 122 | 71% | 3% | 99 |
8 | RX J17137 3946 | 108 | 65% | 3% | 102 |
9 | FORMED DENSE SHELL | 99 | 88% | 1% | 46 |
10 | DIFFUSIVE SHOCK ACCELERATION | 97 | 47% | 5% | 155 |
Journals |
Reviews |
Title | Publ. year | Cit. | Active references | % act. ref. to same field |
---|---|---|---|---|
Supernova remnants at high energy | 2008 | 123 | 122 | 87% |
Nonlinear theory of diffusive acceleration of particles by shock waves | 2001 | 433 | 134 | 63% |
Supernova Remnants Interacting with Molecular Clouds: X-Ray and Gamma-Ray Signatures | 2015 | 1 | 112 | 87% |
Diffusive Shock Acceleration and Magnetic Field Amplification | 2012 | 36 | 70 | 80% |
The origin of galactic cosmic rays | 2013 | 18 | 141 | 73% |
Observational Signatures of Particle Acceleration in Supernova Remnants | 2012 | 24 | 303 | 72% |
Microphysics of Cosmic Ray Driven Plasma Instabilities | 2013 | 10 | 77 | 77% |
On the supernova remnants with flat radio spectra | 2013 | 6 | 92 | 89% |
Radio to gamma-ray emission from shell-type supernova remnants: Predictions from nonlinear shock acceleration models | 1999 | 136 | 73 | 64% |
Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebulae | 2012 | 22 | 112 | 57% |
Address terms |
Rank | Address term | Relevance score (tfidf) |
Class's shr. of term's tot. occurrences |
Shr. of publ. in class containing term |
Num. of publ. in class |
---|---|---|---|---|---|
1 | COSM RADIAT GRP | 8 | 100% | 0.2% | 5 |
2 | DOMINION RADIO ASTROPHYS OBSERV | 7 | 26% | 0.7% | 23 |
3 | POSTBUS 2 | 6 | 80% | 0.1% | 4 |
4 | DOMIN RADIO ASTROPHYS OBSERV | 5 | 23% | 0.5% | 17 |
5 | CNR IST RADIOASTRON VIA IRNERIO 46 | 2 | 67% | 0.1% | 2 |
6 | CP 596 | 2 | 67% | 0.1% | 2 |
7 | ASTRON UTRECHT | 2 | 29% | 0.2% | 6 |
8 | CURZA | 2 | 31% | 0.2% | 5 |
9 | FIS EPS | 2 | 31% | 0.2% | 5 |
10 | OBSERWATORIUM ASTRON | 2 | 13% | 0.4% | 13 |
Related classes at same level (level 1) |
Rank | Relatedness score | Related classes |
---|---|---|
1 | 0.0000093149 | RADIO RECOMBINATION LINES//CII REGIONS//CNRS 8617 |
2 | 0.0000089016 | PULSARS GENERAL//ISM INDIVIDUAL CRAB NEBULA//ISM INDIVIDUAL OBJECTS CRAB NEBULA |
3 | 0.0000071918 | SUPERNOVAE GENERAL//SUPERNOVAE INDIVIDUAL SN 1987A//SUPERNOVAE INDIVIDUAL SN 1993J |
4 | 0.0000068285 | SERV ELE PHYS//COSM RAY WORKING GRP//IST OSSERV ASTRON |
5 | 0.0000068008 | ICRAR M468//CORROS CHEM ENGN//HALOES OF |
6 | 0.0000064505 | WEIBEL INSTABILITY//LEHRSTUHL WELTRAUM ASTROPHYS 4//FILAMENTATION INSTABILITY |
7 | 0.0000061030 | FRED LAWRENCE WHIPPLE OBSERV//BL LACERTAE OBJECTS INDIVIDUAL MARKARIAN 421//BL LACERTAE OBJECTS INDIVIDUAL MARKARIAN 501 |
8 | 0.0000060423 | GALAXIES MAGNETIC FIELDS//GALAXIES MAGNETIC FIELDS//ISM MAGNETIC FIELDS |
9 | 0.0000058332 | STARS NEUTRON//STARS MAGNETARS//STARS INDIVIDUAL SGR 190014 |
10 | 0.0000057739 | GALAXY HALO//ISM BUBBLES//ISM STRUCTURE |