Consolidate Radio Resolution For Free

A lung consolidation can also be fluid, but it is present inside the lungs, unlike pleural effusion, which is present in the space outside the lungs. Hence, lung consolidation cannot move when the position is changed. This criterion is used to differentiate pleural effusion and lung consolidation.

Since pleural effusion is a fluid in a space, it moves when the position of the patient changes. A lung consolidation can also be fluid, but it is present inside the lungs, unlike pleural effusion, which is present in the space outside the lungs. Hence, lung consolidation cannot move when the position is changed.

Consolidation indicates filling of the alveoli and bronchioles in the lung with pus (pneumonia), fluid (pulmonary oedema), blood or neoplastic cells.

Definition. Consolidation refers to an area of homogeneous increase in lung parenchymal attenuation that obscures the margins of vessels and airway walls [1]. Air bronchograms may be present with consolidative area.

Results. The most common causes of pleural effusion are congestive heart failure, cancer, pneumonia, and pulmonary embolism. Pleural fluid puncture (pleural tap) enables the differentiation of a transudate from an exudate, which remains, at present, the foundation of the further diagnostic work-up.

Consolidation is an alveolar-filling process that replaces air within the affected airspac- es, increasing in pulmonary attenuation and obscuring the margins of adjacent airways and vessels on radiographs and CT scans [2].

Consolidation refers to an area of homogeneous increase in lung parenchymal attenuation that obscures the margins of vessels and airway walls [1]. Air bronchograms may be present with consolidative area.

As well as having much lower resolution than a similarly sized optical telescope, radio telescopes usually only have a 1-pixel view of the sky.

An astronomical interferometer or telescope array is a set of separate telescopes, mirror segments, or radio telescope antennas that work together as a single telescope to provide higher resolution images of astronomical objects such as stars, nebulas and galaxies by means of interferometry.

Since the resolving power of a telescope is inversely proportional to the wavelengths of radiation it receives, the only way to increase the resolving power of a radio telescope is to increase the diameter of its dish.