bow shock
71Solar telescope — The Swedish 1 m Solar Telescope at Roque de los Muchachos Observatory, La Palma in the Canary Islands. A solar telescope is a special purpose telescope used to observe the Sun. Solar telescopes usually detect light with wavelengths in, or not far …
72Coronal loop — Typical coronal loops observed by TRACE Coronal loops form the basic structure of the lower corona and transition region of the Sun. These highly structured and elegant loops are a direct consequence of the twisted solar magnetic flux within the… …
73List of radio propagation topics — This is a list of radio propagation terms. NOTOC A a index A index aa index active prominence active prominence region (APR) active region active surge region (ASR) active dark filament (ADF) AE index Air Force Geophysics Laboratory (AFGL) arch… …
74Межзвёздная среда — Карта местного межзвёздного облака Межзвёздная среда (МЗС)  вещество и поля, заполняющие межзвёздное пространство внутри галактик …
75Объект Хербига — Аро — Объект Хербига  Аро HH 47, снимок телескопа Хаббл. Отрезок обозначает расстояние в 1000 астрономических единиц (примерно 20 диаметров Солнечной системы). Объекты Хербига  Аро (англ. Herbig Haro object)& …
76Объект Хербига-Аро — HH47, снимок телескопа Хаббла. Отрезок обозначает расстояние в 1000 астрономических единиц (примерно 20 диаметров Солнечной системы). Объекты Хербига Аро (англ. Herbig Haro object) это небольшие участки туманностей, связанные с молодыми звёздами …
77magnetosphere — magnetospheric /mag nee teuh sfer ik/, adj. /mag nee teuh sfear /, n. Astron. 1. the outer region of the earth s ionosphere, where the earth s magnetic field controls the motion of charged particles, as in the Van Allen belts. Cf. magnetopause. 2 …
78Colliding-wind binary — A colliding wind binary is a binary star system in which the two members are massive stars that emit powerful, radiatively driven stellar winds. The location where these two winds collide produces a strong shock front that can cause radio, X ray… …
79Coronal radiative losses — In astronomy and in astrophysics, for radiative losses of the solar corona, it is meant the energy flux irradiated from the external atmosphere of the Sun (traditionally divided into chromosphere, transition region and corona), and, in particular …
80Stellar kinematics — is the study of the movement of stars without needing to understand how they acquired their motion. This differs from stellar dynamics, which takes into account gravitational effects. The motion of a star relative to the Sun can provide useful… …
