Kaldnurk muutub järk-järgult kaheastmeliseks lülitusvormiks temperatuuril alla K. Tuleb jätkata jõupingutusi, et otsida arenenud perpendikulaarseid õhukesed kiled, mis näitavad head spin-polariseerumist P, madala Gilberti sumbumisparameetrit α, väikest küllastumismagnetatsiooni M S ja sobivat efektiivset risti magnetilist anisotroopset väljad H k Nagu on näidatud joonisel fig 1 a , on CFA kihis paksusega 2, 1 nm ilmselge tasapinnaline lihtne telg. The measured magnitude of the effect is consistent with the standard YORP model. Soovitatav Toimetaja Valik Mittepatogeenne Rhizobium radiobakter F4 viib taime kasulikku aktiivsust sõltumatult oma peremeesorganismist Piriformospora indica Mesenhümaalsete stromaalsete rakkude terapeutilise efektiivsuse parandamine, et taastada kriitilise jäsemeisheemia perfusioon pulseeritud fokuseeritud ultraheliga Üks suurusjärku kiirem faasimuutus vähendatud võimsusega Ti-Sb-Te-s
Nesvorny, David; Carruba, Valerio; Vokrouhlicky, David The Karin family formed by a collisional breakup of a ~km parent asteroid only 5. The young age can be demonstrated by numerically integrating the orbits of Karin family members backward in time and showing the convergence of orbital elements.
Previous work has pointed out that the convergence is not ideal if the backward integration only accounts for the gravitational perturbations from the Solar System planets. It improves when the thermal radiation force known as the Yarkovsky effect is accounted for.
Abstraktne
This method can be used to estimate the spin obliquities of Karin family members. The measured magnitude of the effect is consistent with the standard YORP model.
The surface thermal conductivity is found to be 0.
These results are consistent with surfaces composed of rough and rocky regolith. The obliquity values predicted here for members of the Karin cluster can be validated by the lightcurve inversion method. In broader context, the bimodal distribution of obliquities in the Karin cluster can be thought as an initial stage of dynamical evolution that later leads to a characteristically bi-lobed distribution of family Risti valus spin in the semimajor axis e.
