Pregled bibliografske jedinice broj: 988583
Granular temperature as an energy dissipation mechanism in bodies of the solar system
Granular temperature as an energy dissipation mechanism in bodies of the solar system // Philosophical transactions - Royal Society. Mathematical, Physical and engineering sciences, 463 (2007), 2485-2493 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 988583 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Granular temperature as an energy dissipation mechanism in bodies of the solar system
Autori
Kadish J ; Rougier E ; Munjiza, A ; Barber JR ;
Izvornik
Philosophical transactions - Royal Society. Mathematical, Physical and engineering sciences (1364-503X) 463
(2007);
2485-2493
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
Granular temperature asteroids commets
Sažetak
There is theoretical and observational evidence that asteroids and comets are conglomerations of particles ranging in size from dust grains to boulders. It is well known that energy added to such systems is dissipated by friction, plasticity and fracture. In addition to these physical phenomena, we find that energy can be dissipated in the form of particle kinetic energy due to random velocity distributions. ‘Dissipation’ in this manner is measured by what is called a granular temperature owing to its similarities with kinetic gas theory. This work has implications on our understanding of the growth of asteroids and comets.
Izvorni jezik
Engleski
Znanstvena područja
Fizika, Interdisciplinarne prirodne znanosti
POVEZANOST RADA
Ustanove:
Fakultet građevinarstva, arhitekture i geodezije, Split,
Hrvatska akademija znanosti i umjetnosti
Profili:
Ante Munjiza
(autor)
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus
- MEDLINE
